[1991] J.a. Caldeira, W.L.K. Wu, B. Nord, C. Avestruz, S. Trivedi, K.T. Story, DeepCMB: lensing reconstruction of the cosmic microwave background with deep neural networks, Astron. Comput. 28 (2019) 100307, arXiv:1810.01483 [astro-ph.CO].

[1992] S. He, Y. Li, Y. Feng, S. Ho, S. Ravanbakhsh, W. Chen, B. Póczos, Learning to predict the cosmological structure formation, Proc. Nat. Acad. Sci. 116 (28) (2019) 13825-13832, arXiv:1811.06533 [astro-ph.CO].

[1993] S. Ravanbakhsh, F. Lanusse, R. Mandelbaum, J. Schneider, B. Poczos, Enabling dark energy science with deep generative models of galaxy images, 2016, arXiv:1609.05796 [astro-ph.IM].

[1994] C. Escamilla-Rivera, M.A.C. Quintero, S. Capozziello, A deep learning approach to cosmological dark energy models, J. Cosmol. Astropart. Phys. 03 (2020) 008, arXiv:1910.02788 [astro-ph.CO].

[1995] ANTARES Collaboration, G. Narayan, et al., Machine learning-based brokers for real-time classification of the LSST alert stream, Astrophys. J. Suppl. 236 (1) (2018) 9, arXiv:1801.07323 [astro-ph.IM].

[1996] F. Lanusse, Q. Ma, N. Li, T.E. Collett, C.-L. Li, S. Ravanbakhsh, R. Mandelbaum, B. Poczos, CMU DeepLens: deep learning for automatic image-based galaxy-galaxy strong lens finding, Mon. Not. R. Astron. Soc. 473 (3) (2018) 3895-3906, arXiv:1703.02642 [astro-ph.IM].

[1997] G. Carleo, I. Cirac, K. Cranmer, L. Daudet, M. Schuld, N. Tishby, L. Vogt-Maranto, L. Zdeborová, Machine learning and the physical sciences, Rev. Modern Phys. 91 (4) (2019) 045002, arXiv:1903.10563 [physics.comp-ph].

[1998] P. Mehta, M. Bukov, C.-H. Wang, A.G.R. Day, C. Richardson, C.K. Fisher, D.J. Schwab, A high-bias, low-variance introduction to Machine Learning for physicists, Phys. Rep. 810 (2019) 1-124, arXiv:1803.08823 [physics.comp-ph].

[1999] C. Aggarwal, Neural Networks and Deep Learning: A Textbook, Springer International Publishing, 2018, https://books.google.com.mt/books?id=achqDwAAQBAJ.

[2000] Y.-C. Wang, Y.-B. Xie, T.-J. Zhang, H.-C. Huang, T. Zhang, K. Liu, Likelihood-free cosmological constraints with artificial neural networks: an application on hubble parameters and SNe Ia, Astrophys. J. Supp. 254 (2) (2021) 43, arXiv:2005.10628 [astro-ph.CO].

[2001] I. Gómez-Vargas, R.M. Esquivel, R. García-Salcedo, J.A. Vázquez, Neural network reconstructions for the Hubble parameter, growth rate and distance modulus, Eur. Phys. J. C 83 (4) (2023) 304, arXiv:2104.00595.

[2002] G.-J. Wang, C. Cheng, Y.-Z. Ma, J.-Q. Xia, A. Abebe, A. Beesham, CoLFI: Cosmological likelihood-free inference with neural density estimators, Astrophys. J. Suppl. 268 (1) (2023) 7, arXiv:2306.11102.

[2003] A. Manrique-Yus, E. Sellentin, Euclid-era cosmology for everyone: neural net assisted MCMC sampling for the joint 3 × 2 likelihood, Mon. Not. R. Astron. Soc. 491 (2) (2020) 2655-2663, arXiv:1907.05881.

[2004] A. Spurio Mancini, D. Piras, J. Alsing, B. Joachimi, M.P. Hobson, CosmoPower: emulating cosmological power spectra for accelerated Bayesian inference from next-generation surveys, Mon. Not. R. Astron. Soc. 511 (2) (2022) 1771-1788, arXiv:2106.03846.

[2005] J. Albers, C. Fidler, J. Lesgourgues, N. Schöneberg, J. Torrado, CosmicNet. Part I. Physics-driven implementation of neural networks within Einstein-Boltzmann solvers, J. Cosmol. Astropart. Phys. 09 (2019) 028, arXiv:1907.05764.

[2006] S. Günther, J. Lesgourgues, G. Samaras, N. Schöneberg, F. Stadtmann, C. Fidler, J. Torrado, CosmicNet II: emulating extended cosmologies with efficient and accurate neural networks, J. Cosmol. Astropart. Phys. 11 (2022) 035, arXiv:2207.05707.

[2007] T. Auld, M. Bridges, M.P. Hobson, S.F. Gull, Fast cosmological parameter estimation using neural networks, Mon. Not. R. Astron. Soc. 376 (2007) L11-L15, arXiv:astro-ph/0608174.

[2008] D. Grandón, E. Sellentin, Bayesian error propagation for neural-net based parameter inference, Open J. Astrophys. (2022) arXiv:2205.11587.

[2009] G.-J. Wang, S.-Y. Li, J.-Q. Xia, ECoPANN: A framework for estimating cosmological parameters using artificial neural networks, Astrophys. J. Suppl. 249 (2) (2020) 25, arXiv:2005.07089.

[2010] J. Asorey, M. Crocce, E. Gaztanaga, A. Lewis, Recovering 3D clustering information with angular correlations, Mon. Not. R. Astron. Soc. 427 (2012) 1891, arXiv:1207.6487.

[2011] C.G. Sabiu, K. Kadota, J. Asorey, I. Park, Probing ultra-light axion dark matter from 21 cm tomography using Convolutional Neural Networks, J. Cosmol. Astropart. Phys. 01 (01) (2022) 020, arXiv:2108.07972.

[2012] M. Andrés-Carcasona, M. Martinez, L.M. Mir, Fast Bayesian gravitational wave parameter estimation using convolutional neural networks, Mon. Not. R. Astron. Soc. 527 (2) (2023) 2887-2894, arXiv:2309.04303.

[2013] E. Jones, T. Do, B. Boscoe, J. Singal, Y. Wan, Z. Nguyen, Improving photometric redshift estimation for cosmology with LSST using Bayesian neural networks, Astrophys. J. 964 (2) (2024) 130, arXiv:2306.13179.

[2014] H. Aihara, et al., Second data release of the hyper supreme-cam subaru strategic program, Publ. Astron. Soc. Jap. 71 (6) (2019) 114, arXiv:1905.12221.

[2015] M. Mancarella, J. Kennedy, B. Bose, L. Lombriser, Seeking new physics in cosmology with Bayesian neural networks: Dark energy and modified gravity, Phys. Rev. D 105 (2) (2022) 023531, arXiv:2012.03992.

[2016] L. Thummel, B. Bose, A. Pourtsidou, L. Lombriser, Classifying modified gravity and dark energy theories with Bayesian neural networks: massive neutrinos, baryonic feedback, and the theoretical error, Mon. Not. R. Astron. Soc. 535 (4) (2024) 3141-3161, arXiv:2403.16949.

[2017] G.R. Dvali, G. Gabadadze, M. Porrati, 4-D gravity on a brane in 5-D Minkowski space, Phys. Lett. B 485 (2000) 208-214, arXiv:hep-th/0005016.

[2018] R. Shah, S. Saha, P. Mukherjee, U. Garain, S. Pal, LADDER: Revisiting the cosmic distance ladder with deep learning approaches and exploring its applications, Astrophys. J. Suppl. 273 (2) (2024) 27, arXiv:2401.17029.

[2019] P. Mukherjee, J. Levi Said, J. Mifsud, Neural network reconstruction of H(z) and its application in teleparallel gravity, J. Cosmol. Astropart. Phys. 12 (2022) 029, arXiv:2209.01113.

[2020] G.-J. Wang, X.-J. Ma, S.-Y. Li, J.-Q. Xia, Reconstructing functions and estimating parameters with artificial neural networks: A test with a hubble parameter and SNe Ia, Astrophys. J. Suppl. 246 (1) (2020) 13, arXiv:1910.03636.

[2021] C. Escamilla-Rivera, M. Carvajal, C. Zamora, M. Hendry, Neural networks and standard cosmography with newly calibrated high redshift GRB observations, J. Cosmol. Astropart. Phys. 04 (04) (2022) 016, arXiv:2109.00636.

[2022] J.d.R. Olvera, I. Gómez-Vargas, J.A. Vázquez, Observational cosmology with artificial neural networks, Universe 8 (2) (2022) 120, arXiv:2112.12645.

[2023] I. Gómez-Vargas, J.B. Andrade, J.A. Vázquez, Neural networks optimized by genetic algorithms in cosmology, Phys. Rev. D 107 (4) (2023) 043509, arXiv:2209.02685.

[2024] L. Giambagli, D. Fanelli, G. Risaliti, M. Signorini, Nonparametric analysis of the Hubble diagram with neural networks, Astron. Astrophys. 678 (2023) A13, arXiv:2302.12582.

[2025] K.F. Dialektopoulos, P. Mukherjee, J. Levi Said, J. Mifsud, Neural network reconstruction of cosmology using the Pantheon compilation, Eur. Phys. J. C 83 (10) (2023) 956, arXiv:2305.15499.

[2026] K.F. Dialektopoulos, P. Mukherjee, J. Levi Said, J. Mifsud, Neural network reconstruction of scalar-tensor cosmology, Phys. Dark Univ. 43 (2024) 101383, arXiv:2305.15500.

[2027] P. Mukherjee, K.F. Dialektopoulos, J. Levi Said, J. Mifsud, A possible late-time transition of $M_B$ inferred via neural networks, J. Cosmol. Astropart. Phys. 09 (2024) 060, arXiv:2402.10502.

[2028] B. Zhang, H. Wang, X. Nong, G. Wang, P. Wu, N. Liang, Model-independent gamma-ray bursts constraints on cosmological models using machine learning, Astrophys. Space Sci. 370 (1) (2025) 10, arXiv:2312.09440.

[2029] J.-C. Zhang, Y. Hu, K. Jiao, H.-F. Wang, Y.-B. Xie, B. Yu, L.-L. Zhao, T.-J. Zhang, A nonparametric reconstruction of the Hubble parameter H(z) based on radial basis function neural networks, Astrophys. J. Suppl. 270 (2) (2024) 23, arXiv:2311.13938.

[2030] H. Xie, X. Nong, H. Wang, B. Zhang, Z. Li, N. Liang, Constraints on cosmological models with gamma-ray bursts in cosmology-independent way, Internat. J. Modern Phys. D 34 (02) (2025) 2450073, arXiv:2307.16467.

[2031] L. Tang, X. Li, H.-N. Lin, L. Liu, Model-independent calibrating the luminosity correlations of gamma-ray bursts using deep learning, Astrophys. J. 907 (2) (2021) 121, arXiv:2011.14040.

[2032] L. Liu, L.-J. Hu, L. Tang, Y. Wu, Solving the spatial curvature of the local universe with deep learning, Res. Astron. Astrophys. 23 (12) (2023) 125012, arXiv:2309.11334.

[2033] Pan-STARRS1 Collaboration, D.M. Scolnic, et al., The complete light-curve sample of spectroscopically confirmed SNe Ia from pan-STARRS1 and cosmological constraints from the combined pantheon sample, Astrophys. J. 859 (2) (2018) 101, arXiv:1710.00845.

[2034] R. Shah, P. Mukherjee, S. Saha, U. Garain, S. Pal, Deep learning based recalibration of SDSS and DESI BAO alleviates hubble and clustering tensions, 2024, arXiv:2412.14750.

[2035] G. Papamakarios, E. Nalisnick, D. Jimenez Rezende, S. Mohamed, B. Lakshminarayanan, Normalizing flows for probabilistic modeling and inference, 2019, http://dx.doi.org/10.48550/arXiv.1912.02762, arXiv E-Prints. arXiv:1912.02762.

[2036] J. Sohl-Dickstein, E.A. Weiss, N. Maheswaranathan, S. Ganguli, Deep unsupervised learning using nonequilibrium thermodynamics, 2015, http://dx.doi.org/10.48550/arXiv.1503.03585, arXiv E-Prints. arXiv:1503.03585.

[2037] J. Song, C. Meng, S. Ermon, Denoising diffusion implicit models, 2020, http://dx.doi.org/10.48550/arXiv.2010.02502, arXiv E-Prints. arXiv:2010.02502.

[2038] H.T.J. Bevins, W.J. Handley, P. Lemos, P.H. Sims, E.d. Acedo, A. Fialkov, J. Alsing, Marginal post-processing of Bayesian inference products with normalizing flows and kernel density estimators, Mon. Not. R. Astron. Soc. 526 (3) (2023) 4613-4626, arXiv:2205.12841.

[2039] R. Friedman, S. Hassan, HIGlow: Conditional normalizing flows for high-fidelity HI map modeling, 2022, arXiv:2211.12742.

[2040] A. Mootoovaloo, C. García-García, D. Alonso, J. Ruiz-Zapatero, emuflow: normalizing flows for joint cosmological analysis, Mon. Not. R. Astron. Soc. 536 (1) (2024) 190-202, arXiv:2409.01407.

[2041] M. Raveri, C. Doux, Non-Gaussian estimates of tensions in cosmological parameters, Phys. Rev. D 104 (4) (2021) 043504, arXiv:2105.03324.

[2042] B. Dai, U. Seljak, Translation and rotation equivariant normalizing flow (TRENF) for optimal cosmological analysis, Mon. Not. R. Astron. Soc. 516 (2) (2022) 2363-2373, arXiv:2202.05282.
[2043] B. Dai, U. Seljak, Multiscale flow for robust and optimal cosmological analysis, Proc. Nat. Acad. Sci. 121 (9) (2024) e2306.04689.

[2044] N. Mudur, C. Cuesta-Lazaro, D.P. Finkbeiner, Cosmological field emulation and parameter inference with diffusion models, in: 37th Conference on Neural Information Processing Systems, 2023, arXiv:2312.07534.

[2045] N. Mudur, C. Cuesta-Lazaro, D.P. Finkbeiner, Diffusion-HMC: Parameter inference with diffusion-model-driven Hamiltonian Monte Carlo, Astrophys. J. 978 (1) (2025) 64, arXiv:2405.05255.

[2046] R.C. Bernardo, D. Grandón, J. Said Levi, V.H. Cárdenas, Parametric and nonparametric methods hint dark energy evolution, Phys. Dark Univ. 36 (2022) 101017, arXiv:2111.08289.

[2047] M. Wang, X. Fu, B. Xu, Y. Yang, Z. Chen, Testing the FLRW metric with Hubble and transverse BAO measurements, Phys. Rev. D 108 (10) (2023) 103506, arXiv:2305.01268.

[2048] N. Rani, D. Jain, S. Mahajan, A. Mukherjee, N. Pires, Transition Redshift: New constraints from parametric and nonparametric methods, J. Cosmol. Astropart. Phys. 12 (2015) 045, arXiv:1503.08543.

[2049] H.K. Jassal, J.S. Bagla, T. Padmanabhan, WMAP constraints on low redshift evolution of dark energy, Mon. Not. R. Astron. Soc. 356 (2005) L11–L16, arXiv:astro-ph/0404378.

[2050] B. Wang, E. Abdalla, F. Atrio-Barandela, D. Pavon, Dark matter and dark energy interactions: Theoretical challenges, cosmological implications and observational signatures, Rep. Progr. Phys. 79 (9) (2016) 096901, arXiv: 1603.08299.

[2051] L. Amendola, Coupled quintessence, Phys. Rev. D 62 (2000) 043511, arXiv: astro-ph/9908023.

[2052] V.H. Cárdenas, D. Grandón, S. Lepe, Dark energy and dark matter interaction in light of the second law of thermodynamics, Eur. Phys. J. C 79 (4) (2019) 357, arXiv:1812.03540.

[2053] D. Grandón, V.H. Cárdenas, Exploring evidence of interaction between dark energy and dark matter, Gen. Relativity Gravitation 51 (3) (2019) 42, arXiv: 1804.03296.

[2054] C.-Y. Sun, R.-H. Yue, New interaction between dark energy and dark matter changes sign during cosmological evolution, Phys. Rev. D 85 (2012) 043010, arXiv:1009.1214.

[2055] Y. Wang, P.M. Garnavich, Measuring time dependence of dark energy density from type Ia supernova data, Astrophys. J. 552 (2001) 445, arXiv:astro-ph/0101040.

[2056] Y. Wang, G. Lovelace, Unbiased estimate of dark energy density from type IA supernova data, Astrophys. J. Lett. 562 (2001) L115–L120, arXiv:astro-ph/0109233.

[2057] V.H. Cardenas, Exploring hints for dark energy density evolution in light of recent data, Phys. Lett. B 750 (2015) 128–134, arXiv:1405.5116.

[2058] D. Grandon, V.H. Cardenas, Studies on dark energy evolution, Cl. Quant. Grav. 38 (14) (2021) 145008, arXiv:2107.04876.

[2059] E.V. Linder, Cosmic growth history and expansion history, Phys. Rev. D 72 (2005) 043529, arXiv:astro-ph/0507263.

[2060] N.-M. Nguyen, D. Huterer, Y. Wen, Evidence for suppression of structure growth in the concordance cosmological model, Phys. Rev. Lett. 131 (11) (2023) 111001, arXiv:2302.01331.

[2061] R. Caldwell, A. Cooray, A. Melchiorri, Constraints on a new post-general relativity cosmological parameter, Phys. Rev. D 76 (2007) 023507, arXiv:astro-ph/0703375.

[2062] L. Amendola, S. Fogli, A. Guarnizo, M. Kunz, A. Vollmer, Model-independent constraints on the cosmological anisotropic stress, Phys. Rev. D 89 (6) (2014) 063538, arXiv:1311.4765.

[2063] M. Ranjbar, S. Akhshabi, M. Shadmehri, Gravitational slip parameter and gravitational waves in Einstein–Cartan theory, Eur. Phys. J. C 84 (3) (2024) 316, arXiv:2401.02129.

[2064] R.R. Caldwell, A Phantom menace? Phys. Lett. B 545 (2002) 23–29, arXiv: astro-ph/9908168.

[2065] E. Elizalde, S. Nojiri, S.D. Odintsov, Late-time cosmology in (phantom) scalar-tensor theory: Dark energy and the cosmic speed-up, Phys. Rev. D 70 (2004) 043539, arXiv:hep-th/0405034.

[2066] Y.-F. Cai, E.N. Saridakis, M.R. Setare, J.-Q. Xia, Quintom Cosmology: Theoretical implications and observations, Phys. Rep. 493 (2010) 1–60, arXiv: 0909.2776.

[2067] Z.-K. Guo, Y.-S. Piao, X.-M. Zhang, Y.-Z. Zhang, Cosmological evolution of a quintom model of dark energy, Phys. Lett. B 608 (2005) 177–182, arXiv:astro-ph/0410654.

[2068] J. Tot, B. Yildirim, A. Coley, G. Leon, The dynamics of scalar-field quintom cosmological models, Phys. Dark Univ. 39 (2023) 101155, arXiv:2204.06538.

[2069] J.A. Vázquez, D. Tamayo, G. Garcia-Arroyo, I. Gómez-Vargas, I. Quiros, A.A. Sen, Coupled multiscalar field dark energy, Phys. Rev. D 109 (2) (2024) 023511, arXiv:2305.11396.

[2070] C. Armendariz-Picon, V.F. Mukhanov, P.J. Steinhardt, Essentials of k essence, Phys. Rev. D 63 (2001) 103510, arXiv:astro-ph/0006373.

[2071] G.W. Horndeski, Second-order scalar-tensor field equations in a four-dimensional space, Internat. J. Theoret. Phys. 10 (1974) 363–384.

[2072] T. Clifton, P.G. Ferreira, A. Padilla, C. Skordis, Modified gravity and cosmology, Phys. Rep. 513 (2012) 1–189, arXiv:1106.2476.

[2073] J. Gleyzes, D. Langlois, F. Piazza, F. Vernizzi, Healthy theories beyond Horndeski, Phys. Rev. Lett. 114 (21) (2015) 211101, arXiv:1404.6495.

[2074] A.A. Starobinsky, A new type of isotropic cosmological models without singularity, in: I.M. Khalatnikov, V.P. Mineev (Eds.), Phys. Lett. B 91 (1980) 99–102.

[2075] M. Leizerovich, L. Kraiselburd, S.J. Landau, C.G. Scóccola, Testing f(R) gravity models with quasar x-ray and UV fluxes, Phys. Rev. D 105 (10) (2022) 103526, arXiv:2112.01492.

[2076] Y. Pan, Y. He, J. Qi, J. Li, S. Cao, T. Liu, J. Wang, Testing f(R) gravity with the simulated data of gravitational waves from the Einstein Telescope, Astrophys. J. 911 (2) (2021) 135, arXiv:2103.05212.

[2077] P. Bode, J.P. Ostriker, N. Turok, Halo formation in warm dark matter models, Astrophys. J. 556 (2001) 93–107, arXiv:astro-ph/0010389.

[2078] B. Liu, H. Shan, J. Zhang, New galaxy UV luminosity constraints on warm dark matter from JWST, Astrophys. J. 968 (2) (2024) 79, arXiv:2404.13596.

[2079] S. Lin, et al., Can we constrain warm dark matter masses with individual galaxies? Astrophys. J. 970 (2) (2024) 170, arXiv:2401.17940.

[2080] K.A. Oman, C.S. Frenk, R.A. Crain, M.R. Lovell, J. Pfeffer, A warm dark matter cosmogony may yield more low-mass galaxy detections in 21-cm surveys than a cold dark matter one, Mon. Not. R. Astron. Soc. 533 (1) (2024) 67–78, arXiv:2401.11878.

[2081] J.C. Rose, P. Torrey, F. Villaescusa-Navarro, M. Vogelsberger, S. O’Neil, M.V. Medvedev, R. Low, R. Adhikari, D. Angles-Alcazar, Inferring warm dark matter masses with deep learning, Mon. Not. R. Astron. Soc. 527 (1) (2023) 739–755, arXiv:2304.14432.

[2082] D.N. Spergel, P.J. Steinhardt, Observational evidence for selfinteracting cold dark matter, Phys. Rev. Lett. 84 (2000) 3760–3763, arXiv:astro-ph/9909386.

[2083] DES Collaboration, D. Cross, et al., Examining the self-interaction of dark matter through central cluster galaxy offsets, Mon. Not. R. Astron. Soc. 529 (1) (2024) 52–58, arXiv:2304.10128.

[2084] D. Yang, E.O. Nadler, H.-B. Yu, Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations, Phys. Dark Univ. 47 (2025) 101807, arXiv:2406.10753.

[2085] T. Bringmann, F. Kahlhoefer, K. Schmidt-Hoberg, P. Walia, Strong constraints on self-interacting dark matter with light mediators, Phys. Rev. Lett. 118 (14) (2017) 141802, arXiv:1612.00845.

[2086] M. Visser, Jerk and the cosmological equation of state, Cl. Quant. Grav. 21 (2004) 2603–2616, arXiv:gr-qc/0309109.

[2087] M. Visser, Cosmography: Cosmology without the Einstein equations, in: D.E. McClelland, S.M. Scott (Eds.), Gen. Relativity Gravitation 37 (2005) 1541–1548, arXiv:gr-qc/0411131.

[2088] C. Cattoen, M. Visser, Cosmographic hubble fits to the supernova data, Phys. Rev. D 78 (2008) 063501, arXiv:0809.0537.

[2089] P.K.S. Dunsby, O. Luongo, On the theory and applications of modern cosmography, Int. J. Geom. Meth. Mod. Phys. 13 (03) (2016) 1630002, arXiv:1511.06532.

[2090] S. Capozziello, R. D’Agostino, O. Luongo, Extended gravity cosmography, Internat. J. Modern Phys. D 28 (10) (2019) 1930016, arXiv:1904.01427.

[2091] D. Tamayo, J.A. Vazquez, Fourier-series expansion of the dark-energy equation of state, Mon. Not. R. Astron. Soc. 487 (1) (2019) 729–736, arXiv:1901.08679.

[2092] C. Deffayet, O. Pujolas, I. Sawicki, A. Vikman, Imperfect dark energy from kinetic gravity braiding, J. Cosmol. Astropart. Phys. 10 (2010) 026, arXiv: 1008.0048.

[2093] C. Gruber, O. Luongo, Cosmographic analysis of the equation of state of the universe through Padé approximations, Phys. Rev. D 89 (10) (2014) 103506, arXiv:1309.3215.

[2094] A. Aviles, A. Bravetti, S. Capozziello, O. Luongo, Precision cosmology with Padé rational approximations: Theoretical predictions versus observational limits, Phys. Rev. D 90 (4) (2014) 043531, arXiv:1405.6935.

[2095] H. Wei, X.-P. Yan, Y.-N. Zhou, Cosmological applications of Padé approximant, J. Cosmol. Astropart. Phys. 01 (2014) 045, arXiv:1312.1117.

[2096] S. Capozziello, R. D'Agostino, Reconstructing the distortion function of non-local cosmology: A model-independent approach, Phys. Dark Univ. 42 (2023) 101346, arXiv:2310.03136.

[2097] S. Capozziello, R. D'Agostino, O. Luongo, Rational approximations of f(R) cosmography through Padé polynomials, J. Cosmol. Astropart. Phys. 05 (2018) 008, arXiv:1709.08407.

[2098] A. Hojjati, L. Pogosian, G.-B. Zhao, Detecting features in the dark energy equation of state: A wavelet approach, J. Cosmol. Astropart. Phys. 04 (2010) 007, arXiv:0912.4843.

[2099] J. Wagner, S. Meyer, Generalised model-independent characterisation of strong gravitational lenses V: reconstructing the lensing distance ratio by supernovae for a general friedmann universe, Mon. Not. R. Astron. Soc. 490 (2) (2019) 1913–1927, arXiv:1812.04002.

[2100] C. Mignone, M. Bartelmann, Model-independent determination of the cosmic expansion rate. I. Application to type-Ia supernovae, Astron. Astrophys. 481 (2) (2008) 295–303, arXiv:0711.0370.

[2101] C.S. Lorenz, L. Funcke, M. Löffler, E. Calabrese, Reconstruction of the neutrino mass as a function of redshift, Phys. Rev. D 104 (12) (2021) 123518, arXiv: 2102.13618.
[2102] D.K. Hazra, A. Shafieloo, G.F. Smoot, Reconstruction of broad features in the primordial spectrum and inflaton potential from Planck, J. Cosmol. Astropart. Phys. 12 (2013) 035, arXiv:1310.3038.

[2103] L.A. Escamilla, J.A. Vazquez, Model selection applied to reconstructions of the dark energy, Eur. Phys. J. C 83 (3) (2023) 251, arXiv:2111.10457.

[2104] Y. Wang, L. Pogosian, G.-B. Zhao, A. Zucca, Evolution of dark energy reconstructed from the latest observations, Astrophys. J. Lett. 869 (2018) L8, arXiv:1807.03772.

[2105] G.-B. Zhao, R.G. Crittenden, L. Pogosian, X. Zhang, Examining the evidence for dynamical dark energy, Phys. Rev. Lett. 109 (2012) 171301, arXiv:1207.3804.

[2106] G.-B. Zhao, et al., Dynamical dark energy in light of the latest observations, Nat. Astron. 1 (9) (2017) 627–632, arXiv:1701.08165.

[2107] R.-G. Cai, Q. Su, On the dark sector interactions, Phys. Rev. D—Part., Fields, Gravit., Cosmol. 81 (10) (2010) 103514.

[2108] A. Moss, E. Copeland, S. Bamford, T. Clarke, A model-independent reconstruction of dark energy to very high redshift, 2021, arXiv:2109.14848.

[2109] L. Amendola, M. Kunz, D. Sapone, Measuring the dark side (with weak lensing), J. Cosmol. Astropart. Phys. 04 (2008) 013, arXiv:0704.2421.

[2110] E. Bertschinger, P. Zukin, Distinguishing modified gravity from dark energy, Phys. Rev. D 78 (2008) 024015, arXiv:0801.2431.

[2111] L. Pogosian, A. Silvestri, K. Koyama, G.-B. Zhao, How to optimally parametrize deviations from general relativity in the evolution of cosmological perturbations, Phys. Rev. D 81 (10) (2010) 104023, arXiv:1002.2382.

[2112] M. Raveri, L. Pogosian, M. Martinelli, K. Koyama, A. Silvestri, G.-B. Zhao, Principal reconstructed modes of dark energy and gravity, J. Cosmol. Astropart. Phys. 02 (2023) 061, arXiv:2107.12990.

[2113] L. Pogosian, M. Raveri, K. Koyama, M. Martinelli, A. Silvestri, G.-B. Zhao, J. Li, S. Peirone, A. Zucca, Imprints of cosmological tensions in reconstructed gravity, Nat. Astron. 6 (12) (2022) 1484–1490, arXiv:2107.12992.

[2114] S. Hee, J.A. Vázquez, W.J. Handley, M.P. Hobson, A.N. Lasenby, Constraining the dark energy equation of state using Bayes theorem and the Kullback-Leibler divergence, Mon. Not. R. Astron. Soc. 466 (1) (2017) 369–377, arXiv:1607.00270.

[2115] Z.-K. Guo, D.J. Schwarz, Y.-Z. Zhang, Reconstruction of the primordial power spectrum from CMB data, J. Cosmol. Astropart. Phys. 08 (2011) 031, arXiv:1105.5916.

[2116] A. Ravenni, L. Verde, A.J. Cuesta, Red, straight, no bends: primordial power spectrum reconstruction from CMB and large-scale structure, J. Cosmol. Astropart. Phys. 08 (2016) 028, arXiv:1605.06637.

[2117] G. Aslanyan, L.C. Price, K.N. Abazajian, R. Easther, The knotted sky I: Planck constraints on the primordial power spectrum, J. Cosmol. Astropart. Phys. 08 (2014) 052, arXiv:1403.5849.

[2118] W.J. Handley, A.N. Lasenby, H.V. Peiris, M.P. Hobson, Bayesian inflationary reconstructions from Planck 2018 data, Phys. Rev. D 100 (10) (2019) 103511, arXiv:1908.00906.

[2119] J. Alberto Vazquez, M. Bridges, M.P. Hobson, A.N. Lasenby, Reconstruction of the dark energy equation of state, J. Cosmol. Astropart. Phys. 09 (2012) 020, arXiv:1205.0847.

[2120] I. Tutusaus, B. Lamine, A. Blanchard, Model-independent cosmic acceleration and redshift-dependent intrinsic luminosity in type-Ia supernovae, Astron. Astrophys. 625 (2019) A15, arXiv:1803.06197.

[2121] F. Gerardi, M. Martinelli, A. Silvestri, Reconstruction of the dark energy equation of state from latest data: the impact of theoretical priors, J. Cosmol. Astropart. Phys. 07 (2019) 042, arXiv:1902.09423.

[2122] A. Aviles, C. Gruber, O. Luongo, H. Quevedo, Cosmography and constraints on the equation of state of the Universe in various parametrizations, Phys. Rev. D 86 (2012) 123516, arXiv:1204.2007.

[2123] K. Bamba, S. Capozziello, S. Nojiri, S.D. Odintsov, Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests, Astrophys. Space Sci. 342 (2012) 155–228, arXiv:1205.3421.

[2124] S. Capozziello, R. D'Agostino, O. Luongo, Model-independent reconstruction of $f(T)$ teleparallel cosmology, Gen. Relativity Gravitation 49 (11) (2017) 141, arXiv:1706.02962.

[2125] S. Capozziello, R. D'Agostino, O. Luongo, Thermodynamic parametrization of dark energy, Phys. Dark Univ. 36 (2022) 101045, arXiv:2202.03300.

[2126] C. Cattoen, M. Visser, The Hubble series: Convergence properties and redshift variables, Cl. Quant. Grav. 24 (2007) 5985–5998, arXiv:0710.1887.

[2127] S. Capozziello, R. D'Agostino, Model-independent reconstruction of $f(Q)$ non-metric gravity, Phys. Lett. B 832 (2022) 137229, arXiv:2204.01015.

[2128] S. Capozziello, R. D'Agostino, A cosmographic outlook on dark energy and modified gravity, in: A. Antonelli, R. Fusco Femiano, A. Morselli, G.C. Trincherero (Eds.), Frascati Phys. Ser. 74 (2022) 193–208, arXiv:2211.17194.

[2129] R. D'Agostino, R.C. Nunes, Cosmographic view on the H0 and $\sigma_8$ tensions, Phys. Rev. D 108 (2) (2023) 023523, arXiv:2307.13464.

[2130] S. Capozziello, R. D'Agostino, O. Luongo, Cosmographic analysis with Chebyshev polynomials, Mon. Not. R. Astron. Soc. 476 (3) (2018) 3924–3938, arXiv:1712.04380.

[2131] S. Capozziello, R. D'Agostino, O. Luongo, Cosmographic reconstruction to discriminate between modified gravity and dark energy, Acta Phys. Pol. Supp. 13 (2020) 271.

[2132] A. Gómez-Valent, Quantifying the evidence for the current speed-up of the universe with low and intermediate-redshift data. A more model-independent approach, J. Cosmol. Astropart. Phys. 05 (2019) 026, arXiv:1810.02278.

[2133] C.E. Rasmussen, C.K. Williams, et al., Gaussian Processes for Machine Learning, 1, Springer, 2006.

[2134] C.K. Williams, Gaussian Processes for Machine Learning, MIT Press, 2005.

[2135] M. Seikel, C. Clarkson, M. Smith, Reconstruction of dark energy and expansion dynamics using Gaussian processes, J. Cosmol. Astropart. Phys. 06 (2012) 036, arXiv:1204.2832.

[2136] W. Sun, K. Jiao, T.-J. Zhang, Influence of the bounds of the hyperparameters on the reconstruction of the hubble constant with the Gaussian process, Astrophys. J. 915 (2) (2021) 123, arXiv:2105.12618.

[2137] S. Dhawan, J. Alsing, S. Vagnozzi, Non-parametric spatial curvature inference using late-universe cosmological probes, Mon. Not. R. Astron. Soc. 506 (1) (2021) L1–L5, arXiv:2104.02485.

[2138] S.-g. Hwang, B. L'Huillier, R.E. Keeley, M.J. Jee, A. Shafieloo, How to use GP: effects of the mean function and hyperparameter selection on Gaussian process regression, J. Cosmol. Astropart. Phys. 02 (2023) 014, arXiv:2206.15081.

[2139] F. Avila, A. Bernui, A. Bonilla, R.C. Nunes, Inferring $S_8(z)$ and $\gamma(z)$ with cosmic growth rate measurements using machine learning, Eur. Phys. J. C 82 (7) (2022) 594, arXiv:2201.07829.

[2140] S. Joudaki, M. Kaplinghat, R. Keeley, D. Kirby, Model independent inference of the expansion history and implications for the growth of structure, Phys. Rev. D 97 (12) (2018) 123501, arXiv:1710.04236.

[2141] R.E. Keeley, A. Shafieloo, B. L'Huillier, E.V. Linder, Debiasing cosmic gravitational wave sirens, Mon. Not. R. Astron. Soc. 491 (3) (2020) 3983–3989, arXiv:1905.10216.

[2142] R. Calderón, B. L'Huillier, D. Polarski, A. Shafieloo, A.A. Starobinsky, Joint reconstructions of growth and expansion histories from stage-IV surveys with minimal assumptions: Dark energy beyond $\Lambda$, Phys. Rev. D 106 (8) (2022) 083513, arXiv:2206.13820.

[2143] R. Calderón, B. L'Huillier, D. Polarski, A. Shafieloo, A.A. Starobinsky, Joint reconstructions of growth and expansion histories from stage-IV surveys with minimal assumptions. II. Modified gravity and massive neutrinos, Phys. Rev. D 108 (2) (2023) 023504, arXiv:2301.00640.

[2144] M. Reyes, C. Escamilla-Rivera, On the degeneracy between $f_\sigma$ tension and its Gaussian process forecasting, Universe 8 (8) (2022) 394, arXiv:2203.03574.

[2145] M.A. Sabogal, Ò. Akarsu, A. Bonilla, E. Di Valentino, R.C. Nunes, Exploring new physics in the late Universe's expansion through non-parametric inference, Eur. Phys. J. C 84 (7) (2024) 703, arXiv:2407.04223.

[2146] M.-J. Zhang, H. Li, Gaussian processes reconstruction of dark energy from observational data, Eur. Phys. J. C 78 (6) (2018) 460, arXiv:1806.02981.

[2147] R. Briffa, S. Capozziello, J. Levi Said, J. Mifsud, E.N. Saridakis, Constraining teleparallel gravity through Gaussian processes, Cl. Quant. Grav. 38 (5) (2020) 055007, arXiv:2009.14582.

[2148] N. Banerjee, P. Mukherjee, D. Pavón, Spatial curvature and thermodynamics, Mon. Not. R. Astron. Soc. 521 (4) (2023) 5473–5482, arXiv:2301.09823.

[2149] N. Banerjee, P. Mukherjee, D. Pavón, Checking the second law at cosmic scales, J. Cosmol. Astropart. Phys. 11 (2023) 092, arXiv:2309.12298.

[2150] P. Mukherjee, N. Banerjee, Revisiting a non-parametric reconstruction of the deceleration parameter from combined background and the growth rate data, Phys. Dark Univ. 36 (2022) 100998, arXiv:2007.15941.

[2151] A. Shafieloo, A.G. Kim, E.V. Linder, Gaussian process cosmography, Phys. Rev. D 85 (12) (2012) 123530, arXiv:1204.2272.

[2152] M.-J. Zhang, J.-Q. Xia, Test of the cosmic evolution using Gaussian processes, J. Cosmol. Astropart. Phys. 12 (2016) 005, arXiv:1606.04398.

[2153] K. Liao, A. Shafieloo, R.E. Keeley, E.V. Linder, A model-independent determination of the Hubble constant from lensed quasars and supernovae using Gaussian process regression, Astrophys. J. Lett. 886 (1) (2019) L23, arXiv:1908.04967.

[2154] P. Mukherjee, A. Mukherjee, Assessment of the cosmic distance duality relation using Gaussian process, Mon. Not. R. Astron. Soc. 504 (3) (2021) 3938–3946, arXiv:2104.06066.

[2155] F. Renzi, N.B. Hogg, W. Giarè, The resilience of the Etherington-Hubble relation, Mon. Not. R. Astron. Soc. 513 (3) (2022) 4004–4014, arXiv:2112.05701.

[2156] P. Mukherjee, N. Banerjee, Non-parametric reconstruction of the cosmological jerk parameter, Eur. Phys. J. C 81 (1) (2021) 36, arXiv:2007.10124.

[2157] J.F. Jesus, R. Valentim, A.A. Escobal, S.H. Pereira, D. Benndorf, Gaussian processes reconstruction of the dark energy potential, J. Cosmol. Astropart. Phys. 11 (2022) 037, arXiv:2112.09722.

[2158] D. Wang, X.-H. Meng, Improved constraints on the dark energy equation of state using Gaussian processes, Phys. Rev. D 95 (2) (2017) 023508, arXiv:1708.07750.

[2159] T. Holsclaw, U. Alam, B. Sanso, H. Lee, K. Heitmann, S. Habib, D. Higdon, Nonparametric dark energy reconstruction from supernova data, Phys. Rev. Lett. 105 (2010) 241302, arXiv:1011.3079.

[2160] M. Aljaf, D. Gregoris, M. Khurshudyan, Constraints on interacting dark energy models through cosmic chronometers and Gaussian process, Eur. Phys. J. C 81 (6) (2021) 544, arXiv:2005.01891.
[2161] A. Bonilla, S. Kumar, R.C. Nunes, S. Pan, Reconstruction of the dark sectors' interaction: A model-independent inference and forecast from GW standard sirens, Mon. Not. R. Astron. Soc. 512 (3) (2022) 4231-4238, arXiv:2102.06149.

[2162] L.A. Escamilla, O. Akarsu, E. Di Valentino, J.A. Vazquez, Model-independent reconstruction of the interacting dark energy kernel: Binned and Gaussian process, J. Cosmol. Astropart. Phys. 11 (2023) 051, arXiv:2305.16290.

[2163] P. Mukherjee, N. Banerjee, Nonparametric reconstruction of interaction in the cosmic dark sector, Phys. Rev. D 103 (12) (2021) 123530, arXiv:2105.09995.

[2164] A.M. Pinho, S. Casas, L. Amendola, Model-independent reconstruction of the linear anisotropic stress $\eta$, J. Cosmol. Astropart. Phys. 11 (2018) 027, arXiv:1805.00027.

[2165] Y. Mu, E.-K. Li, L. Xu, Model-independent reconstruction of growth index via Gaussian process, Classical Quantum Gravity 40 (22) (2023) 225003.

[2166] J.A.S. Fortunato, P.H.R.S. Moraes, J.G.d.L. Júnior, E. Brito, Search for the $f(R, T)$ gravity functional form via gaussian processes, Eur. Phys. J. C 84 (2) (2024) 198, arXiv:2305.01325.

[2167] A.K. Singha, A. Sardar, U. Debnath, F(Q) reconstruction: In the light of various modified gravity models, Phys. Dark Universe 41 (2023) 101240.

[2168] F. Oliveira, F. Avila, A. Bernui, A. Bonilla, R.C. Nunes, Reconstructing the growth index $\gamma$ with Gaussian processes, Eur. Phys. J. C 84 (6) (2024) 636, arXiv:2311.14216.

[2169] G.N. Gadbai, S. Mandal, P.K. Sahoo, Gaussian process approach for model-independent reconstruction of $f(Q)$ gravity with direct hubble measurements, Astrophys. J. 972 (2) (2024) 174, arXiv:2404.13095.

[2170] Y. Mu, E.-K. Li, L. Xu, Data-driven and almost model-independent reconstruction of modified gravity, J. Cosmol. Astropart. Phys. 06 (2023) 022, arXiv:2302.09777.

[2171] J. Sultana, M.K. Yennapureddy, F. Melia, D. Kazanas, Constraining $f(R)$ models with cosmic chronometers and the Hii galaxy Hubble diagram, Mon. Not. R. Astron. Soc. 514 (4) (2022) 5827-5839, arXiv:2206.10761.

[2172] E. Elizalde, M. Khurshudyan, Swampland criteria for $f(r)$ gravity derived with a Gaussian process, Eur. Phys. J. C 82 (9) (2022) 811.

[2173] D. Wang, Pantheon+ constraints on dark energy and modified gravity: An evidence of dynamical dark energy, Phys. Rev. D 106 (6) (2022) 063515, arXiv:2207.07164.

[2174] A. Sardar, U. Debnath, Reconstruction of extended $f(P)$ cubic gravity from other modified gravity models, Phys. Dark Universe 35 (2022) 100926.

[2175] X. Ren, S.-F. Yan, Y. Zhao, Y.-F. Cai, E.N. Saridakis, Gaussian processes and effective field theory of $f(T)$ gravity under the $H_0$ tension, Astrophys. J. 932 (2022) 2, arXiv:2203.01926.

[2176] Y.-F. Cai, M. Khurshudyan, E.N. Saridakis, Model-independent reconstruction of $f(T)$ gravity from Gaussian processes, Astrophys. J. 888 (2020) 62, arXiv:1907.10813.

[2177] Y. Liu, S. Cao, T. Liu, X. Li, S. Geng, Y. Lian, W. Guo, Model-independent constraints on cosmic curvature: implication from updated Hubble diagram of high-redshift standard candles, Astrophys. J. 901 (2) (2020) 129, arXiv:2008.08378.

[2178] P. Mukherjee, N. Banerjee, Constraining the curvature density parameter in cosmology, Phys. Rev. D 105 (6) (2022) 063516, arXiv:2202.07886.

[2179] Y. Pan, J. Diao, J.-Z. Qi, J. Li, S. Cao, Q.-Q. Jiang, Testing the spatial geometry of the Universe with TianQin: Prospect of using supermassive black hole binaries, Astron. Astrophys. 683 (2024) A91, arXiv:2310.14723.

[2180] J.-Z. Qi, P. Meng, J.-F. Zhang, X. Zhang, Model-independent measurement of cosmic curvature with the latest $H(z)$ and $SNe$ la data: A comprehensive investigation, Phys. Rev. D 108 (6) (2023) 063522, arXiv:2302.08889.

[2181] Y.-J. Wang, J.-Z. Qi, B. Wang, J.-F. Zhang, J.-L. Cui, X. Zhang, Cosmological model-independent measurement of cosmic curvature using distance sum rule with the help of gravitational waves, Mon. Not. R. Astron. Soc. 516 (4) (2022) 5187-5195, arXiv:2201.12553.

[2182] P.-J. Wu, J.-Z. Qi, X. Zhang, Null test for cosmic curvature using Gaussian process®, Chin. Phys. C 47 (5) (2023) 055106, arXiv:2209.08502.

[2183] Y. Yang, Y. Gong, Measurement on the cosmic curvature using the Gaussian process method, Mon. Not. R. Astron. Soc. 504 (2) (2021) 3092-3097, arXiv:2007.05714.

[2184] G.-J. Wang, X.-J. Ma, J.-Q. Xia, Machine learning the cosmic curvature in a model-independent way, Mon. Not. R. Astron. Soc. 501 (4) (2021) 5714-5722, arXiv:2004.13913.

[2185] E. Belgacem, S. Foffa, M. Maggiore, T. Yang, Gaussian processes reconstruction of modified gravitational wave propagation, Phys. Rev. D 101 (6) (2020) 063505, arXiv:1911.11497.

[2186] X. Zheng, S. Cao, Y. Liu, M. Biesiada, T. Liu, S. Geng, Y. Lian, W. Guo, Model-independent constraints on cosmic curvature: implication from the future space gravitational-wave antenna DECIGO, Eur. Phys. J. C 81 (1) (2021) 14, arXiv:2012.14607.

[2187] R. Shah, A. Bhaumik, P. Mukherjee, S. Pal, A thorough investigation of the prospects of eLISA in addressing the Hubble tension: Fisher forecast, MCMC and machine learning, J. Cosmol. Astropart. Phys. 06 (2023) 038, arXiv:2301.12708.

[2188] G. Cañas-Herrera, J. Torrado, A. Achúcarro, Bayesian reconstruction of the inflaton's speed of sound using CMB data, Phys. Rev. D 103 (2021) 123531, arXiv:2012.04640.

[2189] B.R. Dinda, N. Banerjee, Model independent bounds on type Ia supernova absolute peak magnitude, Phys. Rev. D 107 (6) (2023) 063513, arXiv:2208.14740.

[2190] A. Favale, A. Gómez-Valent, M. Migliaccio, Quantification of 2D vs 3D BAO tension using SNIa as a redshift interpolator and test of the Etherington relation, Phys. Lett. B 858 (2024) 139027, arXiv:2405.12142.

[2191] G. Rodrigues, C. Bengaly, A model-independent test of speed of light variability with cosmological observations, J. Cosmol. Astropart. Phys. 07 (07) (2022) 029, arXiv:2112.01963.

[2192] P. Mukherjee, R. Shah, A. Bhaumik, S. Pal, Reconstructing the Hubble parameter with future gravitational-wave missions using machine learning, Astrophys. J. 960 (1) (2024) 61, arXiv:2303.05169.

[2193] J.-L. Li, Y.-P. Yang, S.-X. Yi, J.-P. Hu, F.-Y. Wang, Y.-K. Qu, Constraints on the cosmological parameters with three-parameter correlation of Gamma-ray bursts, Astrophys. J. 953 (1) (2023) 58, arXiv:2306.12840.

[2194] P. Mukherjee, A.A. Sen, Model-independent cosmological inference post DESI DR1 BAO measurements, Phys. Rev. D 110 (12) (2024) 123502, arXiv:2405.19178.

[2195] M. Khurshudyan, E. Elizalde, Constraints on prospective deviations from the cold dark matter model using a Gaussian process, Galaxies 12 (4) (2024) 31, arXiv:2402.08630.

[2196] R. von Martens, J.E. Gonzalez, J. Alcaniz, V. Marra, L. Casarini, Model-independent reconstruction of dark sector interactions, Phys. Rev. D 104 (4) (2021) 043515, arXiv:2011.10846.

[2197] P. Mukherjee, Non-Parametric Reconstruction of Some Cosmological Parameters (Ph.D. thesis), IISER, Kolkata, 2022, arXiv:2207.07857.

[2198] P. Mukherjee, G. Rodrigues, C. Bengaly, Examining the validity of the minimal varying speed of light model through cosmological observations: Relaxing the null curvature constraint, Phys. Dark Univ. 43 (2024) 101380, arXiv:2302.00867.

[2199] K. Dialektopoulos, J.L. Said, J. Mifsud, J. Sultana, K.Z. Adami, Neural network reconstruction of late-time cosmology and null tests, J. Cosmol. Astropart. Phys. 02 (02) (2022) 023, arXiv:2111.11462.

[2200] M.K. Sharma, M. Sami, Reconciling early and late time tensions with reinforcement learning, J. Cosmol. Astropart. Phys. 05 (2025) 002, arXiv:2408.04204.

[2201] A. Mitra, I. Gómez-Vargas, V. Zarikas, Dark energy reconstruction analysis with artificial neural networks: Application on simulated Supernova Ia data from Rubin Observatory, Phys. Dark Univ. 46 (2024) 101706, arXiv:2402.18124.

[2202] T.-X. Mao, J. Wang, B. Li, Y.-C. Cai, B. Falck, M. Neyrinck, A. Szalay, Baryon acoustic oscillations reconstruction using convolutional neural networks, Mon. Not. R. Astron. Soc. 501 (1) (2021) 1499-1510, arXiv:2002.10218.

[2203] G. Garcia-Arroyo, I. Gómez-Vargas, J.A. Vázquez, Reconstructing rotation curves with artificial neural networks, 2024, arXiv:2404.05833.

[2204] A. Shafieloo, U. Alam, V. Sahni, A.A. Starobinsky, Smoothing Supernova data to reconstruct the expansion history of the universe and its age, Mon. Not. R. Astron. Soc. 366 (2006) 1081-1095, arXiv:astro-ph/0505329.

[2205] A. Shafieloo, Model independent reconstruction of the expansion history of the universe and the properties of dark energy, Mon. Not. R. Astron. Soc. 380 (2007) 1573-1580, arXiv:astro-ph/0703034.

[2206] A. Shafieloo, C. Clarkson, Model independent tests of the standard cosmological model, Phys. Rev. D 81 (2010) 083537, arXiv:0911.4858.

[2207] A. Shafieloo, B. L'Huillier, A.A. Starobinsky, Falsifying ΛCDM: Model-independent tests of the concordance model with eBOSS DR14Q and Pantheon, Phys. Rev. D 98 (8) (2018) 083526, arXiv:1804.04320.

[2208] A. Shafieloo, Crossing statistic: Reconstructing the expansion history of the universe, J. Cosmol. Astropart. Phys. 08 (2012) 002, arXiv:1204.1109.

[2209] H. Koo, A. Shafieloo, R.E. Keeley, B. L'Huillier, Model selection and parameter estimation using the iterative smoothing method, J. Cosmol. Astropart. Phys. 03 (2021) 034, arXiv:2009.12045.

[2210] B. L'Huillier, A. Shafieloo, Model-independent test of the FLRW metric, the flatness of the universe, and non-local measurement of $H_0r_d$, J. Cosmol. Astropart. Phys. 01 (2017) 015, arXiv:1606.06832.

[2211] B. L'Huillier, A. Shafieloo, H. Kim, Model-independent cosmological constraints from growth and expansion, Mon. Not. R. Astron. Soc. 476 (3) (2018) 3263-3268, arXiv:1712.04865.

[2212] B. L'Huillier, A. Mitra, A. Shafieloo, R.E. Keeley, H. Koo, Litmus tests of the flat ΛCDM model and model-independent measurement of $H_0r_d$ with LSST and DESI, 2024, arXiv:2407.07847.

[2213] A. Montiel, R. Lazkoz, I. Sendra, C. Escamilla-Rivera, V. Salzano, Nonparametric reconstruction of the cosmic expansion with local regression smoothing and simulation extrapolation, Phys. Rev. D 89 (4) (2014) 043007, arXiv:1401.4188.

[2214] L.M. Fernández-Hernández, A. Montiel, M.A. Rodríguez-Meza, Galaxy rotation curves using a non-parametric regression method: core, cuspy and fuzzy scalar field dark matter models, Mon. Not. R. Astron. Soc. 488 (4) (2019) 5127-5144, arXiv:1809.06875.
[2215] C. Escamilla-Rivera, J. Levi Said, J. Mifsud, Performance of non-parametric reconstruction techniques in the late-time universe, J. Cosmol. Astropart. Phys. 10 (2021) 016, arXiv:2105.14332.

[2216] A. Rana, D. Jain, S. Mahajan, A. Mukherjee, Revisiting the distance duality relation using a non-parametric regression method, J. Cosmol. Astropart. Phys. 07 (2016) 026, arXiv:1511.09223.

[2217] C. Escamilla-Rivera, J.C. Fabris, Nonparametric reconstruction of the $O_m$ diagnostic to test $\Lambda$CDM, Galaxies 4 (4) (2016) 76, arXiv:1511.07066.

[2218] G. Rudolph, Convergence analysis of canonical genetic algorithms, IEEE Trans. Neural Netw. 5 (1) (1994) 96-101.

[2219] Y. Akrami, P. Scott, J. Edsjo, J. Conrad, L. Bergstrom, A profile likelihood analysis of the constrained MSSM with genetic algorithms, JHEP 04 (2010) 057, arXiv:0910.3950.

[2220] J. Crowder, N.J. Cornish, L. Reddinger, Darwin meets Einstein: LISA data analysis using genetic algorithms, Phys. Rev. D 73 (2006) 063011, arXiv:gr-qc/0601036.

[2221] C. Bogdanos, S. Nesseris, Genetic algorithms and supernovae type Ia analysis, J. Cosmol. Astropart. Phys. 05 (2009) 006, arXiv:0903.2805.

[2222] S. Nesseris, A. Shafieloo, A model independent null test on the cosmological constant, Mon. Not. R. Astron. Soc. 408 (2010) 1879-1885, arXiv:1004.0960.

[2223] S. Nesseris, J. Garcia-Bellido, A new perspective on dark energy modeling via genetic algorithms, J. Cosmol. Astropart. Phys. 11 (2012) 033, arXiv:1205.0364.

[2224] R. Medel-Esquivel, I. Gómez-Vargas, A.A.M. Sánchez, R. García-Salcedo, J. Alberto Vázquez, Cosmological parameter estimation with genetic algorithms, Universe 10 (1) (2024) 11, arXiv:2311.05699.

[2225] A.F. Gad, Pygad: An intuitive genetic algorithm python library, Multimedia Tools Appl. (2023) 1-14.

[2226] R.C. Bernardo, J. Levi Said, Towards a model-independent reconstruction approach for late-time Hubble data, J. Cosmol. Astropart. Phys. 08 (2021) 027, arXiv:2106.08688.

[2227] M.B. Bainbridge, J.K. Webb, Artificial intelligence applied to the automatic analysis of absorption spectra. Objective measurement of the fine structure constant, Mon. Not. R. Astron. Soc. 468 (2) (2017) 1639-1670, arXiv:1606.07393.

[2228] M.B. Bainbridge, J.K. Webb, Evaluating the new automatic method for the analysis of absorption spectra using synthetic spectra, Universe 3 (2) (2017) 34, arXiv:1704.08710.

[2229] C.-C. Lee, J.K. Webb, R.F. Carswell, D. Milaković, Artificial intelligence and quasar absorption system modelling; application to fundamental constants at high redshift, Mon. Not. R. Astron. Soc. 504 (2) (2021) 1787-1800, arXiv:2008.02583.

[2230] J.K. Webb, C.-C. Lee, R.F. Carswell, D. Milaković, Getting the model right: an information criterion for spectroscopy, Mon. Not. R. Astron. Soc. 501 (2) (2021) 2268-2278, arXiv:2009.08336.

[2231] C. Escamilla-Rivera, Bayesian deep learning for dark energy, 2020, http://dx.doi.org/10.5772/intechopen.91466, arXiv:2005.06412.

[2232] C. Escamilla-Rivera, Deep learning for cosmology, in: B. Escalante, F. Carmi-nati, G. Barnafoldi, G. Paic, L. Nellen, R. Mayo, S. Schramm, Z. Ivezic (Eds.), PoS AISIS2019 (2020) 021.

[2233] C.Z. Munóz, C. Escamilla-Rivera, Inverse Cosmography: testing the effec-tiveness of cosmographic polynomials using machine learning, J. Cosmol. Astropart. Phys. 12 (2020) 007, arXiv:2005.02807.

[2234] M. Gendreau, J.-Y. Potvin (Eds.), A modern introduction to memetic algo-rithms, in: Handbook of Metaheuristics, Springer US, Boston, MA, 2010, pp. 141-183, http://dx.doi.org/10.1007/978-1-4419-1665-5_6.

[2235] O.H.M. Ross, A review of quantum-inspired metaheuristics: Going from classical computers to real quantum computers, IEEE Access 8 (2020) 814-838.

[2236] G. Acampora, R. Schiattarella, A. Vitiello, Using quantum amplitude amplification in genetic algorithms, Expert Syst. Appl. 209 (2022) 118203.

[2237] G. Acampora, A. Vitiello, Implementing evolutionary optimization on actual quantum processors, Info. Sci. 575 (2021) 542-562.

[2238] R. Ibarrondo, G. Gatti, M. Sanz, Quantum vs classical genetic algorithms: A numerical comparison shows faster convergence, in: 2022 IEEE Symposium Series on Computational Intelligence, 2022, arXiv:2207.09251.

[2239] R. Ibarrondo, G. Gatti, M. Sanz, Quantum genetic algorithm with individuals in multiple registers, IEEE Trans. Evol. Comput. 28 (2024) 788-797, arXiv:2203.15039.

[2240] G. Sarracino, et al., A quantum genetic algorithm for cosmological functions, 2024, (in preparation).

[2241] J. Prasad, T. Souradeep, Cosmological parameter estimation using particle swarm optimization (PSO), Phys. Rev. D 85 (12) (2012) 123008, arXiv:1108.5600; Erratum-, Phys. Rev. D 90 (2014) 109903.

[2242] A.N. Ruiz, et al., Calibration of semi-analytic models of galaxy formation using particle swarm optimization, Astrophys. J. 801 (2) (2015) 139, arXiv:1310.7034.

[2243] C. Skokos, K.E. Parsopoulos, P.A. Patsis, M.N. Vrahatis, Particle swarm optimization: An efficient method for tracing periodic orbits in 3-D Galactic potentials, Mon. Not. R. Astron. Soc. 359 (2005) 251-260, arXiv:astro-ph/0502164.

[2244] DarkMachines High Dimensional Sampling Group Collaboration, C. Balázs, et al., A comparison of optimisation algorithms for high-dimensional particle and astrophysics applications, JHEP 05 (2021) 108, arXiv:2101.04525.

[2245] T. Toni, D. Welch, N. Strellkowa, A. Ipsen, M.P.H. Stumpf, Approximate Bayesian computation scheme for parameter inference and model selection in dynamical systems, J. R. Soc. Interface 6 (31) (2010) 187-202, arXiv:0901.1925. URL https://royalsocietypublishing.org/doi/abs/10.1098/rsif.2008.0172.

[2246] T. Toni, M.P.H. Stumpf, Simulation-based model selection for dynamical systems in systems and population biology, Bioinformatics 26 (1) (2009) 104-110, arXiv:0911.1705. http://dx.doi.org/10.1093/bioinformatics/btp619.

[2247] T. Toni, M.P.H. Stumpf, Tutorial on ABC rejection and ABC SMC for parameter estimation and model selection, 2009, http://dx.doi.org/10.48550/arXiv:0910.4472, arXiv E-Prints. arXiv:0910.4472.

[2248] R.C. Bernardo, D. Grandón, J. Levi Said, V.H. Cárdenas, Dark energy by natural evolution: Constraining dark energy using approximate Bayesian computation, Phys. Dark Univ. 40 (2023) 101213, arXiv:2211.05482.

[2249] R.C. Bernardo, Y.-R. Lee, Hubble constant by natural selection: Evolution chips in the Hubble tension, Astron. Comput. 44 (2023) 100740, arXiv:2212.02203.

[2250] K.M. Sallam, S.M. Elsayed, R.K. Chakrabarty, M.J. Ryan, Improved multi-operator differential evolution algorithm for solving unconstrained problems, in: 2020 IEEE Congress on Evolutionary Computation, CEC, 2020, pp. 1-8.

[2251] E.A.T. Enriquez, R.G. Mendoza, A.C.T. Velasco, Philippine eagle optimization algorithm, 2021, arXiv E-Prints. arXiv:2112.10318.

[2252] R.C. Bernardo, R. Mendoza, E.A. Enriquez, A.C. Velasco, R. Reyes, Meta-heuristic cosmological parameter estimation: The Philippine Eagle hunts down cosmic expansion, 2025, (in preparation).

[2253] K.Y. Kim, H.W. Lee, Investigating the suitability of data-driven methods for extracting physical parameters in cosmological models, Astron. Comput. 45 (2023) 100762.

[2254] K. Lodha, L. Pinol, S. Nesseris, A. Shafieloo, W. Sohn, M. Fasiello, Searching for local features in primordial power spectrum using genetic algorithms, Mon. Not. R. Astron. Soc. 530 (2) (2024) 1424-1435, arXiv:2308.04940.

[2255] A. Antony, F. Finelli, D.K. Hazra, A. Shafieloo, Discordances in cosmology and the violation of slow-roll inflationary dynamics, Phys. Rev. Lett. 130 (11) (2023) 111001, arXiv:2202.14028.

[2256] D.K. Hazra, A. Antony, A. Shafieloo, One spectrum to cure them all: signature from early Universe solves major anomalies and tensions in cosmology, J. Cosmol. Astropart. Phys. 08 (08) (2022) 063, arXiv:2201.12000.

[2257] G. Alestas, L. Kazantzidis, S. Nesseris, Machine learning constraints on devi-ations from general relativity from the large scale structure of the Universe, Phys. Rev. D 106 (10) (2022) 103519, arXiv:2209.12799.

[2258] EUCLID Collaboration, M. Martinelli, et al., Euclid: Forecast constraints on the cosmic distance duality relation with complementary external probes, Astron. Astrophys. 644 (2020) A80, arXiv:2007.16153.

[2259] Euclid Collaboration, M. Martinelli, et al., Euclid: Constraining dark energy coupled to electromagnetism using astrophysical and laboratory data, Astron. Astrophys. 654 (2021) A148, arXiv:2105.09746.

[2260] Euclid Collaboration, S. Nesseris, et al., Euclid: Forecast constraints on consistency tests of the $\Lambda$CDM model, Astron. Astrophys. 660 (2022) A67, arXiv:2110.11421.

[2261] M. Moresco, R. Jimenez, L. Verde, A. Cimatti, L. Pozzetti, Setting the stage for cosmic chronometers. II. Impact of stellar population synthesis models systematics and full covariance matrix, Astrophys. J. 898 (1) (2020) 82, arXiv:2003.07362.

[2262] D. Brout, et al., The pantheon+ analysis: SuperCal-fragilistic cross calibration, retrained SALT2 light-curve model, and calibration systematic uncertainty, Astrophys. J. 938 (2) (2022) 111, arXiv:2112.03864.

[2263] R.C. Bernardo, Y. Chen, Demystifying genetic algorithm for cosmological parameter estimation and such, 2024, (in preparation).

[2264] A.B. Abdessalem, N. Dervilis, D.J. Wagg, K. Worden, Automatic kernel selec-tion for Gaussian processes regression with approximate Bayesian computation and sequential Monte Carlo, Front. Built Environ. 3 (2017) 52.

[2265] H. Zhang, Y.-C. Wang, T.-J. Zhang, T.-t. Zhang, Kernel selection for Gaussian process in cosmology: With approximate Bayesian computation rejection and nested sampling, Astrophys. J. Suppl. 266 (2) (2023) 27, arXiv:2304.03911.

[2266] V.K. Oikonomou, G. Kafanelis, Primordial cosmology of an emergent-like uni-verse from modified gravity: Reconstruction and phenomenology optimization with a genetic algorithm, Internat. J. Modern Phys. D 33 (1) (2024) 2350114, arXiv:2312.16324.

[2267] A. Aizpuru, R. Arjona, S. Nesseris, Machine learning improved fits of the sound horizon at the baryon drag epoch, Phys. Rev. D 104 (4) (2021) 043521, arXiv:2106.00428.

[2268] R. Arjona, A. Melchiorri, S. Nesseris, Testing the $\Lambda$CDM paradigm with growth rate data and machine learning, J. Cosmol. Astropart. Phys. 05 (05) (2022) 047, arXiv:2107.04343.

[2269] M.R. Gangopadhyay, M. Sami, M.K. Sharma, Phantom dark energy as a natural selection of evolutionary processes a la genetic algorithm and cosmological tensions, Phys. Rev. D 108 (10) (2023) 103526, arXiv:2303.07301.
[2270] L. Kazantzidis, L. Perivolaropoulos, Evolution of the $f\sigma_8$ tension with the Planck15/ΛCDM determination and implications for modified gravity theories, Phys. Rev. D 97 (10) (2018) 103503, arXiv:1803.01337.

[2271] V. Springel, N. Yoshida, S.D.M. White, GADGET: A code for collisionless and gasdynamical cosmological simulations, New Astron. 6 (2001) 79, arXiv:astro-ph/0003162.

[2272] V. Springel, The cosmological simulation code GADGET-2, Mon. Not. R. Astron. Soc. 364 (2005) 1105-1134, arXiv:astro-ph/0505010.

[2273] V. Springel, R. Pakmor, O. Zier, M. Reinecke, Simulating cosmic structure formation with the gadget-4 code, Mon. Not. R. Astron. Soc. 506 (2) (2021) 2871-2949, arXiv:2010.03567.

[2274] V. Springel, E pur si muove: Galilean-invariant cosmological hydrodynamical simulations on a moving mesh, Mon. Not. R. Astron. Soc. 401 (2010) 791, arXiv:0901.4107.

[2275] P.F. Hopkins, A new class of accurate, mesh-free hydrodynamic simulation methods, Mon. Not. R. Astron. Soc. 450 (1) (2015) 53-110, arXiv:1409.7395.

[2276] SWIFT Collaboration, M. Schaller, et al., Swift: a modern highly parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications, Mon. Not. R. Astron. Soc. 530 (2) (2024) 2378-2419, arXiv:2305.13380.

[2277] R. Teyssier, Cosmological hydrodynamics with adaptive mesh refinement: a new high resolution code called RAMSES, Astron. Astrophys. 385 (2002) 337-364, arXiv:astro-ph/0111367.

[2278] V. Springel, et al., Simulating the joint evolution of quasars, galaxies and their large-scale distribution, Nature 435 (2005) 629-636, arXiv:astro-ph/0504097.

[2279] J. Kim, C. Park, R. Gott III, J. Dubinski, The horizon run N-body simulation: Baryon acoustic oscillations and topology of large scale structure of the universe, Astrophys. J. 701 (2009) 1547-1559, arXiv:0812.1392.

[2280] M. Vogelsberger, S. Genel, V. Springel, P. Torrey, D. Sijacki, D. Xu, G.F. Snyder, D. Nelson, L. Hernquist, Introducing the illustris project: Simulating the coevolution of dark and visible matter in the universe, Mon. Not. R. Astron. Soc. 444 (2) (2014) 1518-1547, arXiv:1405.2921.

[2281] V. Springel, et al., First results from the IllustrisTNG simulations: matter and galaxy clustering, Mon. Not. R. Astron. Soc. 475 (1) (2018) 676-698, arXiv:1707.03397.

[2282] A. Klypin, S. Trujillo-Gomez, J. Primack, Halos and galaxies in the standard cosmological model: results from the bolshoi simulation, Astrophys. J. 740 (2011) 102, arXiv:1002.3660.

[2283] J. Schaye, et al., The EAGLE project: Simulating the evolution and assembly of galaxies and their environments, Mon. Not. R. Astron. Soc. 446 (2015) 521-554, arXiv:1407.7040.

[2284] R.A. Crain, et al., The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations, Mon. Not. R. Astron. Soc. 450 (2) (2015) 1937-1961, arXiv:1501.01311.

[2285] F. Villaescusa-Navarro, et al., The quijote simulations, Astrophys. J. Suppl. 250 (1) (2020) 2, arXiv:1909.05273.

[2286] G. Kauffmann, J.M. Colberg, A. Diaferio, S.D.M. White, Clustering of galaxies in a hierarchical universe: 1. Methods and results at $z=0$, Mon. Not. R. Astron. Soc. 303 (1999) 188-206, arXiv:astro-ph/9805283.

[2287] A. Mead, J. Peacock, C. Heymans, S. Joudaki, A. Heavens, An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models, Mon. Not. R. Astron. Soc. 454 (2) (2015) 1958-1975, arXiv:1505.07833.

[2288] H.J. Hortua, Constraining cosmological parameters from N-body simulations with Bayesian neural networks, in: 35th Conference on Neural Information Processing Systems, 2021, arXiv:2112.11865.

[2289] A. Lazanu, Extracting cosmological parameters from N-body simulations using machine learning techniques, J. Cosmol. Astropart. Phys. 09 (2021) 039, arXiv:2106.11061.

[2290] C. Zhang, L. Zu, H.-Z. Chen, Y.-L.S. Tsai, Y.-Z. Fan, Weak lensing constraints on dark matter-baryon interactions with N-body simulations and machine learning, J. Cosmol. Astropart. Phys. 08 (2024) 003, arXiv:2402.18880.

[2291] M.R. Lovell, C.S. Frenk, V.R. Eke, A. Jenkins, L. Gao, T. Theuns, The properties of warm dark matter haloes, Mon. Not. R. Astron. Soc. 439 (2014) 300-317, arXiv:1308.1399.

[2292] S. Bose, W.A. Hellwing, C.S. Frenk, A. Jenkins, M.R. Lovell, J.C. Helly, B. Li, The copernicus complexio: Statistical properties of warm dark matter haloes, Mon. Not. R. Astron. Soc. 455 (1) (2016) 318-333, arXiv:1507.01998.

[2293] Y. Shtanov, V.I. Zhdanov, Discreteness effects in N-body simulations of warm dark matter, Phys. Rev. D 109 (6) (2024) 063031, arXiv:2307.07778.

[2294] F. Villaescusa-Navarro, F. Marulli, M. Viel, E. Branchini, E. Castorina, E. Sefusatti, S. Saito, Cosmology with massive neutrinos I: towards a realistic modeling of the relation between matter, haloes and galaxies, J. Cosmol. Astropart. Phys. 03 (2014) 011, arXiv:1311.0866.

[2295] J. Adamek, R. Durrer, M. Kunz, Relativistic N-body simulations with massive neutrinos, J. Cosmol. Astropart. Phys. 11 (2017) 004, arXiv:1707.06938.

[2296] J. Liu, S. Bird, J.M.Z. Matilla, J.C. Hill, Z. Haiman, M.S. Madhavacheril, A. Petri, D.N. Spergel, MassiveNuS: Cosmological massive neutrino simulations, J. Cosmol. Astropart. Phys. 03 (2018) 049, arXiv:1711.10524.

[2297] B. Li, G.-B. Zhao, R. Teyssier, K. Koyama, ECOSMOG: An efficient code for simulating modified gravity, J. Cosmol. Astropart. Phys. 01 (2012) 051, arXiv:1110.1379.

[2298] E. Puchwein, M. Baldi, V. Springel, Modified gravity-GADGET: A new code for cosmological hydrodynamical simulations of modified gravity models, Mon. Not. R. Astron. Soc. 436 (2013) 348, arXiv:1305.2418.

[2299] J. Zhang, R. An, S. Liao, W. Luo, Z. Li, B. Wang, Fully self-consistent cosmological simulation pipeline for interacting dark energy models, Phys. Rev. D 98 (10) (2018) 103530, arXiv:1811.01519.

[2300] C. Arnold, M. Leo, B. Li, Realistic simulations of galaxy formation in $f(R)$ modified gravity, Nat. Astron. 3 (10) (2019) 945-954, arXiv:1907.02977.

[2301] B.S. Wright, H.A. Winther, K. Koyama, COLA with massive neutrinos, J. Cosmol. Astropart. Phys. 10 (2017) 054, arXiv:1705.08165.

[2302] M. Baldi, F. Villaescusa-Navarro, Quijote simulations: Modified gravity, 2025, https://quijote-simulations.readthedocs.io/en/latest/mg.html. (Accessed 30 January 2025).

[2303] X.-I. Chen, S. Hannestad, R.J. Scherrer, Cosmic microwave background and large scale structure limits on the interaction between dark matter and baryons, Phys. Rev. D 65 (2002) 123515, arXiv:astro-ph/0202496.

[2304] D.V. Nguyen, D. Sarnaak, K.K. Boddy, E.O. Nadler, V. Gluscевic, Observational constraints on dark matter scattering with electrons, Phys. Rev. D 104 (10) (2021) 103521, arXiv:2107.12380.

[2305] P. Serra, F. Zalamea, A. Cooray, G. Mangano, A. Melchiorri, Constraints on neutrino – dark matter interactions from cosmic microwave background and large scale structure data, Phys. Rev. D 81 (2010) 043507, arXiv:0911.4411.

[2306] G. Mangano, A. Melchiorri, P. Serra, A. Cooray, M. Kamionkowski, Cosmological bounds on dark matter-neutrino interactions, Phys. Rev. D 74 (2006) 043517, arXiv:astro-ph/0606190.

[2307] R.J. Wilkinson, C. Boehm, J. Lesgourgues, Constraining dark matter-neutrino interactions using the CMB and large-scale structure, J. Cosmol. Astropart. Phys. 05 (2014) 011, arXiv:1401.7597.

[2308] F.-Y. Cyr-Racine, K. Sigurdson, J. Zavala, T. Bringmann, M. Vogelsberger, C. Pfrommer, ETHOS—an effective theory of structure formation: From dark particle physics to the matter distribution of the Universe, Phys. Rev. D 93 (12) (2016) 123527, arXiv:1512.05344.

[2309] M. Vogelsberger, J. Zavala, F.-Y. Cyr-Racine, C. Pfrommer, T. Bringmann, K. Sigurdson, ETHOS – an effective theory of structure formation: dark matter physics as a possible explanation of the small-scale CDM problems, Mon. Not. R. Astron. Soc. 460 (2) (2016) 1399-1416, arXiv:1512.05349.

[2310] L. Zu, C. Zhang, H.-Z. Chen, W. Wang, Y.-L.S. Tsai, Y. Tsai, W. Luo, Y.-Z. Fan, Exploring mirror twin higgs cosmology with present and future weak lensing surveys, J. Cosmol. Astropart. Phys. 08 (2023) 023, arXiv:2304.06308.

[2311] S. Bohr, J. Zavala, F.-Y. Cyr-Racine, M. Vogelsberger, T. Bringmann, C. Pfrommer, ETHOS – an effective parametrization and classification for structure formation: the non-linear regime at $z \ge 5$, Mon. Not. R. Astron. Soc. 498 (3) (2020) 3403-3419, arXiv:2006.01842.

[2312] V. Ajani, A. Peel, V. Pettorino, J.-L. Starck, Z. Li, J. Liu, Constraining neutrino masses with weak-lensing multiscale peak counts, Phys. Rev. D 102 (10) (2020) 103531, arXiv:2001.10993.

[2313] A. Peel, V. Pettorino, C. Giocoli, J.-L. Starck, M. Baldi, Breaking degeneracies in modified gravity with higher (than 2nd) order weak-lensing statistics, Astron. Astrophys. 619 (2018) A38, arXiv:1805.05146.

[2314] V. Ajani, J.-L. Starck, V. Pettorino, Starlet $\ell_1$-norm for weak lensing cosmology, Astron. Astrophys. 645 (2021) L11, arXiv:2101.01542.

[2315] J. Harnois-Déraps, N. Martinet, T. Castro, K. Dolag, B. Giblin, C. Heymans, H. Hildebrandt, Q. Xia, Cosmic shear cosmology beyond two-point statistics: a combined peak count and correlation function analysis of DES-Y1, MNRAS 506 (2) (2021) 1623-1650, arXiv:2012.02777.

[2316] J. Jasche, B.D. Wandelt, Bayesian physical reconstruction of initial conditions from large scale structure surveys, Mon. Not. R. Astron. Soc. 432 (2013) 894, arXiv:1203.3639.

[2317] J. Jasche, G. Lavaux, Physical Bayesian modelling of the non-linear matter distribution: new insights into the nearby universe, Astron. Astrophys. 625 (2019) A64, arXiv:1806.11117.

[2318] N. Porqueres, A. Heavens, D. Mortlock, G. Lavaux, Bayesian forward modelling of cosmic shear data, Mon. Not. R. Astron. Soc. 502 (2) (2021) 3035-3044, arXiv:2011.07722.

[2319] N. Porqueres, A. Heavens, D. Mortlock, G. Lavaux, Lifting weak lensing degeneracies with a field-based likelihood, Mon. Not. R. Astron. Soc. 509 (3) (2021) 3194-3202, arXiv:2108.04825.

[2320] N. Porqueres, A. Heavens, D. Mortlock, G. Lavaux, T.L. Makinen, Field-level inference of cosmic shear with intrinsic alignments and baryons, 2023, arXiv:2304.04785.

[2321] T.L. Makinen, C. Sui, B.D. Wandelt, N. Porqueres, A. Heavens, Hybrid summary statistics, 2024, arXiv:2410.07548.

[2322] DES Collaboration, N. Jeffrey, et al., Dark Energy Survey Year 3 results: likelihood-free, simulation-based $\omega$CDM inference with neural compression of weak-lensing map statistics, Mon. Not. R. Astron. Soc. 536 (2) (2025) 1303-1322, arXiv:2403.02314.
[2323] N. MacCrann, J. Zuntz, S. Bridle, B. Jain, M.R. Becker, Cosmic discordance: Are Planck CMB and CFHTLeNS weak lensing measurements out of tune? Mon. Not. R. Astron. Soc. 451 (3) (2015) 2877-2888, arXiv:1408.4742.

[2324] H. Rubira, A. Mazoun, M. Garny, Full-shape BOSS constraints on dark matter interacting with dark radiation and lifting the S8 tension, J. Cosmol. Astropart. Phys. 01 (2023) 034, arXiv:2209.03974.

[2325] T. Brinckmann, J.H. Chang, P. Du, M. LoVerde, Confronting interacting dark radiation scenarios with cosmological data, Phys. Rev. D 107 (12) (2023) 123517, arXiv:2212.13264.

[2326] DES Collaboration, A. Chen, et al., Constraints on dark matter to dark radiation conversion in the late universe with DES-Y1 and external data, Phys. Rev. D 103 (12) (2021) 123528, arXiv:2011.04606.

[2327] A. He, M.M. Ivanov, R. An, V. Gluscevic, S<sub>8</sub> tension in the context of dark matter-baryon scattering, Astrophys. J. Lett. 954 (1) (2023) L8, arXiv:2301.08260.

[2328] E. Di Valentino, C. Boehm, E. Hivon, F.R. Bouchet, Reducing the H<sub>0</sub> and σ<sub>8</sub> tensions with dark matter-neutrino interactions, Phys. Rev. D 97 (4) (2018) 043513, arXiv:1710.02559.

[2329] L. Zu, W. Giarbè, C. Zhang, E. Di Valentino, Y.-L.S. Tsai, S. Trojanowski, Can vDM interactions solve the S<sub>8</sub> discrepancy?, 2025, arXiv:2501.13785.

[2330] H. Zhan, The wide-field multiband imaging and slitsless spectroscopy survey to be carried out by the Survey Space Telescope of China Manned Space Program, Chin. Sci. Bull. 66 (2021) 1290-1298.

[2331] R.A.C. Croft, D.H. Weinberg, M. Bolte, S. Burles, L. Hernquist, N. Katz, D. Kirkman, D. Tytler, Towards a precise measurement of matter clustering: Lyman alpha forest data at redshifts 2-4, Astrophys. J. 581 (2002) 20-52, arXiv:astro-ph/0012324.

[2332] M. Viel, The Lyman-α forest as a probe of the coldness of dark matter, in: 19th Conference on High Energy Physics, 2008, pp. 255-260.

[2333] M. Viel, G.D. Becker, J.S. Bolton, M.G. Haehnelt, Warm dark matter as a solution to the small scale crisis: New constraints from high redshift Lyman-α forest data, Phys. Rev. D 88 (2013) 043502, arXiv:1306.2314.

[2334] M. Viel, M.G. Haehnelt, V. Springel, Infrerring the dark matter power spectrum from the Lyman-alpha forest in high-resolution QSO absorption spectra, Mon. Not. R. Astron. Soc. 354 (2004) 684, arXiv:astro-ph/0404600.

[2335] A. Boyarsky, J. Lesgourgues, O. Ruchayskiy, M. Viel, Lyman-alpha constraints on warm and on warm-plus-cold dark matter models, J. Cosmol. Astropart. Phys. 05 (2009) 012, arXiv:0812.0010.

[2336] K.K. Rogers, H.V. Peiris, Strong bound on canonical ultralight axion dark matter from the lyman-alpha forest, Phys. Rev. Lett. 126 (7) (2021) 071302, arXiv:2007.12705.

[2337] M. Garny, T. Konstandin, L. Sagunski, M. Viel, Neutrino mass bounds from confronting an effective model with BOSS Lyman-α data, J. Cosmol. Astropart. Phys. 03 (2021) 049, arXiv:2011.03050.

[2338] N. Palanque-Delabrouille, et al., Neutrino masses and cosmology with Lyman-alpha forest power spectrum, J. Cosmol. Astropart. Phys. 11 (2015) 011, arXiv:1506.05976.

[2339] J.S. Bolton, A. Caputo, H. Liu, M. Viel, Comparison of low-redshift Lyman-α forest observations to hydrodynamical simulations with dark photon dark matter, Phys. Rev. Lett. 129 (21) (2022) 211102, arXiv:2206.13520.

[2340] D.C. Hooper, M. Lucca, Hints of dark matter-neutrino interactions in lyman-α data, Phys. Rev. D 105 (10) (2022) 103504, arXiv:2110.04024.

[2341] S. Furlanetto, S.P. Oh, F. Briggs, Cosmology at low frequencies: The 21 cm transition and the high-redshift universe, Phys. Rep. 433 (2006) 181-301, arXiv:astro-ph/0608032.

[2342] J.R. Pritchard, A. Loeb, 21-Cm cosmology, Rep. Progr. Phys. 75 (2012) 086901, arXiv:1109.6012.

[2343] A. Schneider, Constraining noncold dark matter models with the global 21-cm signal, Phys. Rev. D 98 (6) (2018) 063021, arXiv:1805.00021.

[2344] L. Lopez-Honorez, O. Mena, P. Villanueva-Domingo, Dark matter microphysics and 21 cm observations, Phys. Rev. D 99 (2) (2019) 023522, arXiv:1811.02716.

[2345] M. Escudero, L. Lopez-Honorez, O. Mena, S. Palomares-Ruiz, P. Villanueva-Domingo, A fresh look into the interacting dark matter scenario, J. Cosmol. Astropart. Phys. 06 (2018) 007, arXiv:1803.08427.

[2346] J.B. Muñoz, C. Dvorkin, F.-Y. Cyr-Racine, Probing the small-scale matter power spectrum with large-scale 21-cm data, Phys. Rev. D 101 (6) (2020) 063526, arXiv:1911.11144.

[2347] S. Yoshiura, K. Takahashi, T. Takahashi, Probing small scale primordial power spectrum with 21cm line global signal, Phys. Rev. D 101 (8) (2020) 083520, arXiv:1911.07442.

[2348] J.B. Muñoz, S. Bohr, F.-Y. Cyr-Racine, J. Zavala, M. Vogelsberger, ETHOS - an effective theory of structure formation: Impact of dark acoustic oscillations on cosmic daw, Phys. Rev. D 103 (4) (2021) 043512, arXiv:2011.05333.

[2349] M.R. Lovell, J. Zavala, M. Vogelsberger, X. Shen, F.-Y. Cyr-Racine, C. Pfromer, K. Sigurdson, M. Boylan-Kolchin, A. Pillepich, ETHOS - an effective theory of structure formation: predictions for the high-redshift Universe - abundance of galaxies and reionization, Mon. Not. R. Astron. Soc. 477 (3) (2018) 2886-2899, arXiv:1711.10497.

[2350] S. Hassan, R. Davé, K. Finlator, M.G. Santos, Simulating the 21 cm signal from reionization including non-linear ionizations and inhomogeneous re-combinations, Mon. Not. R. Astron. Soc. 457 (2) (2016) 1550-1567, arXiv: 1510.04280.

[2351] LOFAR Collaboration, M.P. van Haarlem, et al., LOFAR: The LOw-frequency array, Astron. Astrophys. 556 (2013) A2, arXiv:1305.3550.

[2352] D.R. DeBoer, et al., Hydrogen epoch of reionization array (HERA), Publ. Astron. Soc. Pac. 129 (974) (2017) 045001, arXiv:1606.07473.

[2353] L.V.E. Koopmans, et al., The cosmic daw and epoch of reionization with the square kilometre array, in: T.L. Bourke, et al. (Eds.), PoS AASKA14 (2015) 001, arXiv:1505.07568.

[2354] J.S. Bullock, M. Boylan-Kolchin, Small-scale challenges to the ΛCDM paradigm, Ann. Rev. Astron. Astrophys. 55 (2017) 343-387, arXiv:1707.04256.

[2355] J.F. Navarro, C.S. Frenk, S.D.M. White, The structure of cold dark matter halos, Astrophys. J. 462 (1996) 563-575, arXiv:astro-ph/9508025.

[2356] W.J.G. de Blok, The core-cusp problem, Adv. Astron. 2010 (2010) 789293, arXiv:0910.3538.

[2357] G. Gentile, P. Salucci, U. Klein, D. Vergani, P. Kalberla, The cored distribution of dark matter in spiral galaxies, Mon. Not. R. Astron. Soc. 351 (2004) 903, arXiv:astro-ph/0403154.

[2358] J.S. Bullock, T.S. Kolatt, Y. Sigad, R.S. Somerville, A.V. Kravtsov, A.A. Klypin, J.R. Primack, A. Dekel, Profiles of dark haloes. Evolution, scatter, and environment, Mon. Not. R. Astron. Soc. 321 (2001) 559-575, arXiv:astro-ph/9908159.

[2359] K.A. Oman, et al., The unexpected diversity of dwarf galaxy rotation curves, Mon. Not. R. Astron. Soc. 452 (4) (2015) 3650-3665, arXiv:1504.01437.

[2360] A.A. Klypin, A.V. Kravtsov, O. Valenzuela, F. Prada, Where are the missing galactic satellites? Astrophys. J. 522 (1999) 82-92, arXiv:astro-ph/9901240.

[2361] B. Moore, S. Ghigna, F. Governato, G. Lake, T.R. Quinn, J. Stadel, P. Tozzi, Dark matter substructure within galactic halos, Astrophys. J. Lett. 524 (1999) L19-L22, arXiv:astro-ph/9907411.

[2362] M. Boylan-Kolchin, J.S. Bullock, M. Kaplinghat, Too big to fail? The puzzling darkness of massive Milky Way subhaloes, Mon. Not. R. Astron. Soc. 415 (2011) L40, arXiv:1103.0007.

[2363] M. Boylan-Kolchin, J.S. Bullock, M. Kaplinghat, The Milky Way's bright satellites as an apparent failure of LCDM, Mon. Not. R. Astron. Soc. 422 (2012) 1203-1218, arXiv:1111.2048.

[2364] J.F. Navarro, V.R. Eke, C.S. Frenk, The cores of dwarf galaxy halos, Mon. Not. R. Astron. Soc. 283 (1996) L72-L78, arXiv:astro-ph/9610187.

[2365] S.-H. Oh, C. Brook, F. Governato, E. Brinks, L. Mayer, W.J.G. de Blok, A. Brooks, F. Walter, The central slope of dark matter cores in dwarf galaxies: Simulations vs. THINGS, Astron. J. 142 (2011) 24, arXiv:1011.2777.

[2366] A. Zolotov, A.M. Brooks, B. Willman, F. Governato, A. Pontzen, C. Christensen, A. Dekel, T. Quinn, S. Shen, J. Wadsley, Baryons matter: Why luminous satellite galaxies have reduced central masses, Astrophys. J. 761 (2012) 71, arXiv:1207.0007.

[2367] K.S. Arraki, A. Klypin, S. More, S. Trujillo-Gomez, Effects of baryon removal on the structure of dwarf spheroidal galaxies, Mon. Not. R. Astron. Soc. 438 (2) (2014) 1466-1482, arXiv:1212.6651.

[2368] A.M. Brooks, A. Zolotov, Why baryons matter: The kinematics of dwarf spheroidal satellites, Astrophys. J. 786 (2014) 87, arXiv:1207.2468.

[2369] C.B. Brook, A. Di Cintio, Expanded haloes, abundance matching and too-big-to-fail in the local group, Mon. Not. R. Astron. Soc. 450 (4) (2015) 3920-3934, arXiv:1410.3825.

[2370] A.A. Dutton, A.V. Macciò, J. Frings, L. Wang, G.S. Stinson, C. Penzo, X. Kang, NIHAO V: too big does not fail - reconciling the conflict between ΛCDM predictions and the circular velocities of nearby field galaxies, Mon. Not. R. Astron. Soc. 457 (1) (2016) L74-L78, arXiv:1512.00453.

[2371] W. Hu, R. Barkana, A. Gruzinov, Cold and fuzzy dark matter, Phys. Rev. Lett. 85 (2000) 1158-1161, arXiv:astro-ph/0003365.

[2372] B. Moore, S. Gelato, A. Jenkins, F.R. Pearce, V. Quilis, Collisional versus collisionless dark matter, Astrophys. J. Lett. 535 (2000) L21-L24, arXiv:astro-ph/0002308.

[2373] N. Yoshida, V. Springel, S.D.M. White, G. Tormen, Collisional dark matter and the structure of dark halos, Astrophys. J. Lett. 535 (2000) L103, arXiv:astro-ph/0002362.

[2374] A. Burkert, The structure and evolution of weakly selfinteracting cold dark matter halos, Astrophys. J. Lett. 534 (2000) L143-L146, arXiv:astro-ph/0002409.

[2375] C.S. Kochanek, M.J. White, A quantitative study of interacting dark matter in halos, Astrophys. J. 543 (2000) 514, arXiv:astro-ph/0003483.

[2376] N. Yoshida, V. Springel, S.D.M. White, G. Tormen, Weakly self-interacting dark matter and the structure of dark halos, Astrophys. J. Lett. 544 (2000) L87-L90, arXiv:astro-ph/0006134.

[2377] R. Dave, D.N. Spergel, P.J. Steinhardt, B.D. Wandelt, Halo properties in cosmological simulations of selfinteracting cold dark matter, Astrophys. J. 547 (2001) 574-589, arXiv:astro-ph/0006218.

[2378] J. Mirałda-Escude, A test of the collisional dark matter hypothesis from cluster lensing, Astrophys. J. 564 (2002) 60, arXiv:astro-ph/0002050.
[2379] M. Rocha, A.H.G. Peter, J.S. Bullock, M. Kaplinghat, S. Garrison-Kimmel, J. Onorbe, L.A. Moustakas, Cosmological simulations with self-interacting dark matter I: Constant density cores and substructure, Mon. Not. R. Astron. Soc. 430 (2013) 81–104, arXiv:1208.3025.

[2380] A.H.G. Peter, M. Rocha, J.S. Bullock, M. Kaplinghat, Cosmological simulations with self-interacting dark matter II: Halo shapes vs. Observations, Mon. Not. R. Astron. Soc. 430 (2013) 105, arXiv:1208.3026.

[2381] M. Vogelsberger, J. Zavala, A. Loeb, Subhaloes in self-interacting galactic dark matter haloes, Mon. Not. R. Astron. Soc. 423 (2012) 3740, arXiv:1201.5892.

[2382] O.D. Elbert, J.S. Bullock, S. Garrison-Kimmel, M. Rocha, J. Onorbe, A.H.G. Peter, Core formation in dwarf haloes with self-interacting dark matter: no fine-tuning necessary, Mon. Not. R. Astron. Soc. 453 (1) (2015) 29–37, arXiv:1412.1477.

[2383] H.-Y. Schive, T. Chiueh, T. Broadhurst, Cosmic structure as the quantum interference of a coherent dark wave, Nat. Phys. 10 (2014) 496–499, arXiv: 1406.6586.

[2384] P. Mocz, M. Vogelsberger, V.H. Robles, J. Zavala, M. Boylan-Kolchin, A. Fialkov, L. Hernquist, Galaxy formation with BECDM – I. Turbulence and relaxation of idealized haloes, Mon. Not. R. Astron. Soc. 471 (4) (2017) 4559–4570, arXiv:1705.05845.

[2385] J. Veltmaat, J.C. Niemeyer, B. Schwabe, Formation and structure of ultralight bosonic dark matter halos, Phys. Rev. D 98 (4) (2018) 043509, arXiv:1804. 09647.

[2386] L. Herold, E.G.M. Ferreira, L. Heinrich, Profile likelihoods in cosmology: When, why, and how illustrated with $Λ$CDM, massive neutrinos, and dark energy, Phys. Rev. D 111 (8) (2025) 083504, arXiv:2408.07700.

[2387] J. Neyman, Outline of a theory of statistical estimation based on the classical theory of probability, Phil. Trans. Roy. Soc. Lond. A 236 (767) (1937) 333–380.

[2388] S.S. Wilks, The large-sample distribution of the likelihood ratio for testing composite hypotheses, Ann. Math. Stat. 9 (1) (1938) 60–62.

[2389] Y. Pawitan, In All Likelihood: Statistical Modelling and Inference Using Likelihood, Oxford Science Publications, OUP Oxford, 2001, URL https:// books.google.com/books?id=M-3pSCVxV5oC.

[2390] R. Trotta, Bayesian methods in cosmology, 2017, arXiv E-Prints. arXiv:1701. 01467.

[2391] G.J. Feldman, R.D. Cousins, A unified approach to the classical statistical analysis of small signals, Phys. Rev. D 57 (1998) 3873–3889, arXiv:physics/ 9711021.

[2392] R.D. Cousins, Why isn't every physicist a Bayesian? Am. J. Phys. 63 (1995) 398.

[2393] LiteBIRD Collaboration, P. Campeti, et al., LiteBIRD science goals and forecasts. A case study of the origin of primordial gravitational waves using large-scale CMB polarization, J. Cosmol. Astropart. Phys. 06 (2024) 008, arXiv:2312.00717.

[2394] SPIDER Collaboration, P.A.R. Ade, et al., A constraint on primordial B-modes from the first flight of the spider balloon-borne telescope, Astrophys. J. 927 (2) (2022) 174, arXiv:2103.13334.

[2395] B.A. Reid, L. Verde, R. Jimenez, O. Mena, Robust neutrino constraints by combining low redshift observations with the CMB, J. Cosmol. Astropart. Phys. 01 (2010) 003, arXiv:0910.0008.

[2396] W. Giarè, A. Gómez-Valent, E. Di Valentino, C. van de Bruck, Hints of neutrino dark matter scattering in the CMB? Constraints from the marginalizedized and profile distributions, Phys. Rev. D 109 (6) (2024) 063516, arXiv:2311.09116.

[2397] T. Karwal, Y. Patel, A. Bartlett, V. Poulin, T.L. Smith, D.N. Pfeffer, Procoli: Profiles of cosmological likelihoods, 2024, arXiv:2401.14225.

[2398] E.B. Holm, A. Nygaard, J. Dakin, S. Hannestad, T. Tram, PROSPECT: a profile likelihood code for frequentist cosmological parameter inference, Mon. Not. R. Astron. Soc. 535 (4) (2024) 3686–3699, arXiv:2312.02972.

[2399] F. James, M. Roos, Minuit - a system for function minimization and analysis of the parameter errors and correlations, Comput. Phys. Comm. 10 (6) (1975) 343–367, URL https://www.sciencedirect.com/science/article/pii/ 0010465575900399.

[2400] G. Galloni, S. Henrot-Versillé, M. Tristram, Robust constraints on tensor perturbations from cosmological data: A comparative analysis from Bayesian and frequentist perspectives, Phys. Rev. D 110 (6) (2024) 063511, arXiv: 2405.04455.

[2401] C. Moretti, M. Tsedrik, P. Carrilho, A. Pourtsidou, Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for stage IV surveys, J. Cosmol. Astropart. Phys. 12 (2023) 025, arXiv:2306.09275.

[2402] P. Campeti, O. Özsoy, I. Obata, M. Shiraishi, New constraints on axion-gauge field dynamics during inflation from Planck and BICEP/Keck data sets, J. Cosmol. Astropart. Phys. 07 (07) (2022) 039, arXiv:2203.03401.

[2403] P. Campeti, E. Komatsu, New constraint on the tensor-to-scalar ratio from the Planck and BICEP/Keck array data using the profile likelihood, Astrophys. J. 941 (2) (2022) 110, arXiv:2205.05617.

[2404] Planck Collaboration, P.A.R. Ade, et al., Planck intermediate results. XVI. Profile likelihoods for cosmological parameters, Astron. Astrophys. 566 (2014) A54, arXiv:1311.1657.

[2405] S. Hannestad, Stochastic optimization methods for extracting cosmological parameters from cosmic microwave background radiation power spectra, Phys. Rev. D 61 (2000) 023002, arXiv:astro-ph/9911330.

[2406] S. Kirkpatrick, C.D. Gelatt, M.P. Vecchi, Optimization by simulated annealing, Science 220 (1983) 671–680.

[2407] S. Henrot-Versillé, O. Perdereau, S. Plaszczyński, B.R. d'Orfeuil, M. Spinelli, M. Tristram, Agnostic cosmology in the CAMEL framework, 2016, arXiv: 1607.02964.

[2408] A. Nygaard, E.B. Holm, S. Hannestad, T. Tram, CONNECT: a neural network based framework for emulating cosmological observables and cosmological parameter inference, J. Cosmol. Astropart. Phys. 05 (2023) 025, arXiv:2205. 15726.

[2409] A. Nygaard, E.B. Holm, S. Hannestad, T. Tram, Fast and effortless computation of profile likelihoods using CONNECT, J. Cosmol. Astropart. Phys. 11 (2023) 064, arXiv:2308.06379.

[2410] T. Bringmann, F. Kahlhoefer, K. Schmidt-Hoberg, P. Walia, Converting non-relativistic dark matter to radiation, Phys. Rev. D 98 (2) (2018) 023543, arXiv:1803.03644.

[2411] F. Couchot, S. Henrot-Versillé, O. Perdereau, S. Plaszczyński, B. Rouillé d'Orfeuil, M. Spinelli, M. Tristram, Cosmological constraints on the neutrino mass including systematic uncertainties, Astron. Astrophys. 606 (2017) A104, arXiv:1703.10829.

[2412] A.X. Gonzalez-Morales, R. Poltis, B.D. Sherwin, L. Verde, Are priors responsible for cosmology favoring additional neutrino species?, 2011, arXiv:1106.5052.

[2413] L. Herold, M. Kamionkowski, Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data, Phys. Rev. D 111 (8) (2025) 083518, arXiv:2412.03546.

[2414] S. Henrot-Versille, et al., Improved constraint on the primordial gravitational-wave density using recent cosmological data and its impact on cosmic string models, Cl. Quant. Grav. 32 (4) (2015) 045003, arXiv:1408.5299.

[2415] A.J.S. Capistrano, R.C. Nunes, L.A. Cabral, Lower tensor-to-scalar ratio as possible signature of modified gravity, Phys. Rev. D 109 (12) (2024) 123517, arXiv:2403.13860.

[2416] B. Hu, J. Torrado, Searching for primordial localized features with CMB and LSS spectra, Phys. Rev. D 91 (6) (2015) 064039, arXiv:1410.4804.

[2417] A. Avilez, C. Skordis, Cosmological constraints on Brans-Dicke theory, Phys. Rev. Lett. 113 (1) (2014) 011101, arXiv:1303.4330.

[2418] J. de Cruz Pérez, J. Solà Peracaula, Brans-Dicke cosmology mimicking running vacuum, Modern Phys. Lett. A 33 (38) (2018) 1850228, arXiv:1809.03329.

[2419] J. Solà Peracaula, A. Gomez-Valent, J. de Cruz Pérez, C. Moreno-Pulido, Brans-Dicke gravity with a cosmological constant smoothes out $Λ$CDM tensions, Astrophys. J. Lett. 886 (1) (2019) L6, arXiv:1909.02554.

[2420] J. Solà Peracaula, A. Gómez-Valent, J. de Cruz Pérez, C. Moreno-Pulido, Brans-Dicke cosmology with a $Λ$-term: a possible solution to $Λ$CDM tensions, Cl. Quant. Grav. 37 (24) (2020) 245003, arXiv:2006.04273.

[2421] S. Joudaki, P.G. Ferreira, N.A. Lima, H.A. Winther, Testing gravity on cosmic scales: A case study of Jordan-Brans-Dicke theory, Phys. Rev. D 105 (4) (2022) 043522, arXiv:2010.15278.

[2422] C. Wetterich, The cosmom model for an asymptotically vanishing time dependent cosmological 'constant', Astron. Astrophys. 301 (1995) 321–328, arXiv: hep-th/9408025.

[2423] V. Pettorino, L. Amendola, C. Baccigalupi, C. Quercellini, Constraints on coupled dark energy using CMB data from WMAP and SPT, Phys. Rev. D 86 (2012) 103507, arXiv:1207.3293.

[2424] V. Pettorino, Testing modified gravity with Planck: the case of coupled dark energy, Phys. Rev. D 88 (2013) 063519, arXiv:1305.7457.

[2425] Planck Collaboration, P.A.R. Ade, et al., Planck 2015 results. XIV. Dark energy and modified gravity, Astron. Astrophys. 594 (2016) A14, arXiv:1502.01590.

[2426] B.J. Barros, L. Amendola, T. Barreiro, N.J. Nunes, Coupled quintessence with a $Λ$CDM background: removing the $σ_8$ tension, J. Cosmol. Astropart. Phys. 01 (2019) 007, arXiv:1802.09216.

[2427] A. Gómez-Valent, V. Pettorino, L. Amendola, Update on coupled dark energy and the $H_0$ tension, Phys. Rev. D 101 (12) (2020) 123513, arXiv:2004.00610.

[2428] A. Gómez-Valent, Z. Zheng, L. Amendola, C. Wetterich, V. Pettorino, Coupled and uncoupled early dark energy, massive neutrinos, and the cosmological tensions, Phys. Rev. D 106 (10) (2022) 103522, arXiv:2207.14487.

[2429] L.W.K. Goh, A. Gómez-Valent, V. Pettorino, M. Kilbinger, Constraining constant and tomographic coupled dark energy with low-redshift and high-redshift probes, Phys. Rev. D 107 (8) (2023) 083503, arXiv:2211.13588.

[2430] P.J.E. Peebles, B. Ratra, Cosmology with a time variable cosmological constant, Astrophys. J. Lett. 325 (1988) L17.

[2431] P. Brax, C. van de Bruck, E. Di Valentino, W. Giarè, S. Trojanowski, New insights on $ν$-DM interactions, Mon. Not. R. Astron. Soc. 527 (1) (2023) L122–L126, arXiv:2303.16895.

[2432] P. Brax, C. van de Bruck, E. Di Valentino, W. Giarè, S. Trojanowski, Extended analysis of neutrino-dark matter interactions with small-scale CMB experiments, Phys. Dark Univ. 42 (2023) 101321, arXiv:2305.01383.

[2433] BOSS Collaboration, L. Anderson, et al., The clustering of galaxies in the SDSS-III baryon oscillation spectroscopic survey: Baryon acoustic oscillations in the data release 9 spectroscopic galaxy sample, Mon. Not. R. Astron. Soc. 427 (4) (2013) 3435–3467, arXiv:1203.6594.
[2434] eBOSS Collaboration, M. Ata, et al., The clustering of the SDSS-IV extended baryon oscillation spectroscopic survey DR14 quasar sample: first measurement of baryon acoustic oscillations between redshift 0.8 and 2.2, Mon. Not. R. Astron. Soc. 473 (4) (2018) 4773-4794, arXiv:1705.06373.

[2435] DES Collaboration, T.M.C. Abbott, et al., Dark energy survey year 1 results: Measurement of the baryon acoustic oscillation scale in the distribution of galaxies to redshift 1, Mon. Not. R. Astron. Soc. 483 (4) (2019) 4866-4883, arXiv:1712.06209.

[2436] DES Collaboration, K.C. Chan, et al., BAO from angular clustering: Optimization and mitigation of theoretical systematics, Mon. Not. R. Astron. Soc. 480 (3) (2018) 3031-3051, arXiv:1801.04390.

[2437] R. Ruggeri, C. Blake, How accurately can we measure the baryon acoustic oscillation feature? Mon. Not. R. Astron. Soc. 498 (3) (2020) 3744-3757, arXiv:1909.13011.

[2438] A. Cuceu, A. Font-Ribera, B. Joachimi, Bayesian methods for fitting baryon acoustic oscillations in the Lyman-α forest, J. Cosmol. Astropart. Phys. 07 (2020) 035, arXiv:2004.02761.

[2439] A.G. Sanchez, Arguments against using $h^{-1}Mpc$ units in observational cosmology, Phys. Rev. D 102 (12) (2018) 123511, arXiv:2002.07829.

[2440] L.F. Secco, T. Karwal, W. Hu, E. Krause, Role of the Hubble scale in the weak lensing versus CMB tension, Phys. Rev. D 107 (8) (2023) 083532, arXiv:2209.12997.

[2441] M. Forconi, A. Favale, A. Gómez-Valent, Illustrating the consequences of a misuse of $\sigma_8$ in cosmology, 2025, arXiv:2501.11571.

[2442] V. Poulin, T.L. Smith, R. Calderón, T. Simon, Implications of the cosmic calibration tension beyond H0 and the synergy between early- and late-time new physics, Phys. Rev. D 111 (8) (2025) 083552, arXiv:2407.18292.

[2443] D. Pedrotti, J.-Q. Jiang, L.A. Escamilla, S.S. da Costa, S. Vagnozzi, Multidimensionality of the Hubble tension: The roles of $\Omega_m$ and $\omega_c$, Phys. Rev. D 111 (2) (2025) 023506, arXiv:2408.04530.

[2444] M. Kamionkowski, A.G. Riess, The Hubble tension and early dark energy, Ann. Rev. Nucl. Part. Sci. 73 (2023) 153-180, arXiv:2211.04492.

[2445] V. Poulin, T.L. Smith, T. Karwal, The ups and downs of early dark energy solutions to the Hubble tension: A review of models, hints and constraints circa 2023, Phys. Dark Univ. 42 (2023) 101348, arXiv:2302.09032.

[2446] E. McDonough, J.C. Hill, M.M. Ivanov, A. La Posta, M.W. Toomey, Observational constraints on early dark energy, Internat. J. Modern Phys. D 33 (11) (2024) 2430003, arXiv:2310.19899.

[2447] A. Albrecht, C. Skordis, Phenomenology of a realistic accelerating universe using only Planck scale physics, Phys. Rev. Lett. 84 (2000) 2076-2079, arXiv:astro-ph/9908085.

[2448] M. Doran, M.J. Lilley, J. Schwindt, C. Wetterich, Quintessence and the separation of CMB peaks, Astrophys. J. 559 (2001) 501-506, arXiv:astro-ph/0012139.

[2449] C. Wetterich, Phenomenological parameterization of quintessence, Phys. Lett. B 594 (2004) 17-22, arXiv:astro-ph/0403289.

[2450] M. Doran, G. Robbers, Early dark energy cosmologies, J. Cosmol. Astropart. Phys. 06 (2006) 026, arXiv:astro-ph/0601544.

[2451] M. Kamionkowski, J. Pradler, D.G.E. Walker, Dark energy from the string axiverse, Phys. Rev. Lett. 113 (25) (2014) 251302, arXiv:1409.0549.

[2452] T. Karwal, M. Kamionkowski, Dark energy at early times, the Hubble parameter, and the string axiverse, Phys. Rev. D 94 (10) (2016) 103532, arXiv:1608.01309.

[2453] V. Poulin, T.L. Smith, D. Grin, T. Karwal, M. Kamionkowski, Cosmological implications of ultralight axionlike fields, Phys. Rev. D 98 (8) (2018) 083525, arXiv:1806.10608.

[2454] V. Poulin, T.L. Smith, T. Karwal, M. Kamionkowski, Early dark energy can resolve the Hubble tension, Phys. Rev. Lett. 122 (22) (2019) 221301, arXiv:1811.04083.

[2455] T.L. Smith, V. Poulin, M.A. Amin, Oscillating scalar fields and the Hubble tension: a resolution with novel signatures, Phys. Rev. D 101 (6) (2020) 063523, arXiv:1908.06995.

[2456] A.R. Khalife, M.B. Zanjani, S. Galli, S. Günther, J. Lesgourgues, K. Benabed, Review of Hubble tension solutions with new SHOES and SPT-3G data, J. Cosmol. Astropart. Phys. 04 (2024) 059, arXiv:2312.09814.

[2457] J.C. Hill, E. McDonough, M.W. Toomey, S. Alexander, Early dark energy does not restore cosmological concordance, Phys. Rev. D 102 (4) (2020) 043507, arXiv:2003.07355.

[2458] V. Poulin, T.L. Smith, A. Bartlett, Dark energy at early times and ACT data: A larger Hubble constant without late-time priors, Phys. Rev. D 104 (12) (2021) 123550, arXiv:2109.06229.

[2459] E. McDonough, M.-X. Lin, J.C. Hill, W. Hu, S. Zhou, Early dark sector, the Hubble tension, and the swampland, Phys. Rev. D 106 (4) (2022) 043525, arXiv:2112.09128.

[2460] S. Alexander, E. McDonough, Axion-dilaton destabilization and the Hubble tension, Phys. Lett. B 797 (2019) 134830, arXiv:1904.08912.

[2461] M. Cicoli, M. Licheri, R. Mahanta, E. McDonough, F.G. Pedro, M. Scalisi, Early dark energy in type IIB string theory, JHEP 06 (2023) 052, arXiv:2303.03414.

[2462] E. McDonough, M. Scalisi, Towards early dark energy in string theory, JHEP 10 (2023) 118, arXiv:2209.00011.

[2463] R. Kappl, H.P. Nilles, M.W. Winkler, Modulated natural inflation, Phys. Lett. B 753 (2016) 653-659, arXiv:1511.05560.

[2464] L. Yin, Reducing the $H_0$ tension with exponential acoustic dark energy, Eur. Phys. J. C 82 (1) (2022) 78, arXiv:2012.13917.

[2465] G. Ye, Y.-S. Piao, Is the Hubble tension a hint of AdS phase around recombination? Phys. Rev. D 101 (8) (2020) 083507, arXiv:2001.02451.

[2466] A. Adil, A. Albrecht, L. Knox, Quintessential cosmological tensions, Phys. Rev. D 107 (6) (2023) 063521, arXiv:2207.10235.

[2467] P. Agrawal, F.-Y. Cyr-Racine, D. Pinner, L. Randall, Rock 'n' roll solutions to the Hubble tension, Phys. Dark Univ. 42 (2023) 101347, arXiv:1904.01016.

[2468] M.-X. Lin, G. Benevento, W. Hu, M. Raveri, Acoustic dark energy: Potential conversion of the hubble tension, Phys. Rev. D 100 (6) (2019) 063542, arXiv:1905.12618.

[2469] R. Jackiw, S.Y. Pi, Chern-Simons modification of general relativity, Phys. Rev. D 68 (2003) 104012, arXiv:gr-qc/0308071.

[2470] M.J. Duncan, N. Kaloper, K.A. Olive, Axion hair and dynamical torsion from anomalies, Nuclear Phys. B 387 (1992) 215-235.

[2471] S. Basilakos, N.E. Mavromatos, J. Solà Peracaula, Gravitational and chiral anomalies in the running vacuum universe and matter-antimatter asymmetry, Phys. Rev. D 101 (4) (2020) 045001, arXiv:1907.04890.

[2472] S. Basilakos, N.E. Mavromatos, J. Solà Peracaula, Quantum anomalies in string-inspired running vacuum universe: Inflation and axion dark matter, Phys. Lett. B 803 (2020) 135342, arXiv:2001.03465.

[2473] N.E. Mavromatos, J. Solà Peracaula, Stringy-running-vacuum-model inflation: from primordial gravitational waves and stiff axion matter to dynamical dark energy, Eur. Phys. J. ST 230 (9) (2021) 2077-2110, arXiv:2012.07971.

[2474] E. Guendelman, R. Herrera, D. Benisty, Unifying inflation with early and late dark energy with multiple fields: Spontaneously broken scale invariant two measures theory, Phys. Rev. D 105 (12) (2022) 124035, arXiv:2201.06470.

[2475] E.L.D. Perico, J.A.S. Lima, S. Basilakos, J. Sola, Complete cosmic history with a dynamical $\Lambda = \Lambda(H)$ term, Phys. Rev. D 88 (2013) 063531, arXiv:1306.0591.

[2476] J.A.S. Lima, S. Basilakos, J. Sola, Expansion history with decaying vacuum: A complete cosmological scenario, Mon. Not. R. Astron. Soc. 431 (2013) 923-929, arXiv:1209.2802.

[2477] J. Solà, A. Gómez-Valent, The $\bar{\Lambda}$CDM cosmology: From inflation to dark energy through running $\Lambda$, Internat. J. Modern Phys. D 24 (2015) 1541003, arXiv:1501.03832.

[2478] J. Solà Peracaula, H. Yu, Particle and entropy production in the running vacuum universe, Gen. Relativity Gravitation 52 (2) (2020) 17, arXiv:1910.01638.

[2479] N.E. Mavromatos, J. Solà Peracaula, Inflationary physics and trans-Planckian conjecture in the stringy running vacuum model: from the phantom vacuum to the true vacuum, Eur. Phys. J. Plus 136 (11) (2012) 1152, arXiv:2105.02659.

[2480] P. Svrcek, E. Witten, Axions in string theory, JHEP 06 (2006) 051, arXiv:hep-th/0605206.

[2481] P. Dorlis, N.E. Mavromatos, S.-N. Vlachos, Condensate-induced inflation from primordial gravitational waves in string-inspired Chern-Simons gravity, Phys. Rev. D 110 (6) (2024) 063512, arXiv:2403.09005.

[2482] N.E. Mavromatos, P. Dorlis, S.-N. Vlachos, Torsion-induced axions in string theory, quantum gravity and the cosmological tensions, in: Workshop on the Standard Model and beyond, 2024, arXiv:2404.18741.

[2483] L. McAllister, E. Silverstein, A. Westphal, Gravity waves and linear inflation from axion monodromy, Phys. Rev. D 82 (2010) 046003, arXiv:0808.0706.

[2484] A. Gómez-Valent, N.E. Mavromatos, J. Solà Peracaula, Stringy running vacuum model and current tensions in cosmology, Cl. Quant. Grav. 41 (1) (2024) 015026, arXiv:2305.15774.

[2485] A. Gómez-Valent, J. Solà Peracaula, Phantom matter: A challenging solution to the cosmological tensions, Astrophys. J. 975 (1) (2024) 64, arXiv:2404.18845.

[2486] R. Kallosh, A. Linde, Universality class in conformal inflation, J. Cosmol. Astropart. Phys. 07 (2013) 002, arXiv:1306.5220.

[2487] R. Kallosh, A. Linde, D. Roest, Superconformal inflationary $\alpha$-attractors, JHEP 11 (2013) 198, arXiv:1311.0472.

[2488] M. Galante, R. Kallosh, A. Linde, D. Roest, Unity of cosmological inflation attractors, Phys. Rev. Lett. 114 (14) (2015) 141302, arXiv:1412.3797.

[2489] M. Braglia, W.T. Emond, F. Finelli, A.E. Gumrukcuoglu, K. Koyama, Unified framework for early dark energy from $\alpha$-attractors, Phys. Rev. D 102 (8) (2020) 083513, arXiv:2005.14053.

[2490] L. Brissenden, K. Dimopoulos, S. Sánchez López, Non-oscillating early dark energy and quintessence from $\alpha$-attractors, Astropart. Phys. 157 (2024) 102925, arXiv:2301.03572.

[2491] D. Chowdhury, G. Tasinato, I. Zavala, Dark energy, D-branes and pulsar timing arrays, J. Cosmol. Astropart. Phys. 11 (2023) 090, arXiv:2307.01188.

[2492] O.F. Ramadan, T. Karwal, J. Sakstein, Attractive proposal for resolving the Hubble tension: Dynamical attractors that unify early and late dark energy, Phys. Rev. D 109 (6) (2024) 063525, arXiv:2309.08082.

[2493] E.J. Copeland, A.R. Liddle, D. Wands, Exponential potentials and cosmological scaling solutions, Phys. Rev. D 57 (1998) 4686-4690, arXiv:gr-qc/9711068.

[2494] T. Barreiro, E.J. Copeland, N.J. Nunes, Quintessence arising from exponential potentials, Phys. Rev. D 61 (2000) 127301, arXiv:astro-ph/9910214.
[2495] A. Gómez-Valent, Z. Zheng, L. Amendola, V. Pettorino, C. Wetterich, Early dark energy in the pre- and postrecombination epochs, Phys. Rev. D 104 (8) (2021) 083536, arXiv:2107.11065.

[2496] V. Pettorino, L. Amendola, C. Wetterich, How early is early dark energy? Phys. Rev. D 87 (2013) 083009, arXiv:1301.5279.

[2497] E.J. Copeland, A. Moss, S. Sevillano Muñoz, J.M.M. White, Scaling solutions as early dark energy resolutions to the Hubble tension, J. Cosmol. Astropart. Phys. 05 (2024) 078, arXiv:2309.15295.

[2498] T. Karwal, M. Raveri, B. Jain, J. Khoury, M. Trodden, Chameleon early dark energy and the Hubble tension, Phys. Rev. D 105 (6) (2022) 063535, arXiv:2106.13290.

[2499] M.-X. Lin, E. McDonough, J.C. Hill, W. Hu, Dark matter trigger for early dark energy coincidence, Phys. Rev. D 107 (10) (2023) 103523, arXiv:2212.08098.

[2500] G. Liu, Z. Zhou, Y. Mu, L. Xu, Alleviating cosmological tensions with a coupled scalar fields model, Phys. Rev. D 108 (8) (2023) 083523, arXiv:2307.07228.

[2501] G. Garcia-Arroyo, L.A.UREÑA-LÓPEZ, J.A. Vázquez, Interacting scalar fields: Dark matter and early dark energy, Phys. Rev. D 110 (2) (2024) 023529, arXiv:2402.08815.

[2502] A. Talebian, Early dark energy and dark photon dark matter from waterfall symmetry breaking, Phys. Rev. D 109 (12) (2024) 123526, arXiv:2312.08254.

[2503] K.V. Berghaus, T. Karwal, Thermal friction as a solution to the hubble tension, Phys. Rev. D 101 (8) (2020) 083537, arXiv:1911.06281.

[2504] J. Sakstein, M. Trodden, Early dark energy from massive neutrinos as a natural resolution of the hubble tension, Phys. Rev. Lett. 124 (16) (2020) 161301, arXiv:1911.11760.

[2505] M. Carrillo González, Q. Liang, J. Sakstein, M. Trodden, Neutrino-assisted early dark energy: Theory and cosmology, J. Cosmol. Astropart. Phys. 04 (2021) 063, arXiv:2011.09895.

[2506] D.H.F. de Souza, R. Rosenfeld, Can neutrino-assisted early dark energy models ameliorate the H0 tension in a natural way? Phys. Rev. D 108 (8) (2023) 083512, arXiv:2302.04644.

[2507] M. Carrillo González, Q. Liang, J. Sakstein, M. Trodden, Neutrino-assisted early dark energy is a natural resolution of the hubble tension, 2023, arXiv: 2302.09091.

[2508] X. Li, A. Shafieloo, A simple phenomenological emergent dark energy model can resolve the hubble tension, Astrophys. J. Lett. 883 (1) (2019) L3, arXiv: 1906.08275.

[2509] LÁ. GÁRCIA, L. CASTAÑEDA, J.M. TEJEIRO, A novel early dark energy model, New Astron. 84 (2021) 101503, arXiv:2009.07357.

[2510] H.B. Benaoum, LÁ. García, L. Castañeda, Early dark energy induced by non-linear electrodynamics, 2023, arXiv:2307.05917.

[2511] X. Li, A. Shafieloo, Evidence for emergent dark energy, Astrophys. J. 902 (1) (2020) 58, arXiv:2001.05103.

[2512] S. Nojiri, S.D. Odintsov, D. Saez-Chillon Gomez, G.S. Sharov, Modeling and testing the equation of state for (Early) dark energy, Phys. Dark Univ. 32 (2001) 100837, arXiv:2103.05304.

[2513] V.I. Sabla, R.R. Caldwell, Microphysics of early dark energy, Phys. Rev. D 106 (6) (2022) 063526, arXiv:2202.08291.

[2514] H. Moshafi, H. Firouzjahi, A. Talebian, Multiple transitions in vacuum dark energy and H₀ tension, Astrophys. J. 940 (2) (2022) 121, arXiv:2208.05583.

[2515] A.J. Ross, L. Samushia, C. Howlett, W.J. Percival, A. Burden, M. Manera, The clustering of the SDSS DR7 main galaxy sample - I. A 4 per cent distance measure at z = 0.15, Mon. Not. R. Astron. Soc. 449 (1) (2015) 835-847, arXiv:1409.3242.

[2516] E.-M. Mueller, W. Percival, E. Linder, S. Alam, G.-B. Zhao, A.G. Sánchez, F. Beutler, J. Brinkmann, The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity, Mon. Not. R. Astron. Soc. 475 (2) (2018) 2122-2131, arXiv:1612.00812.

[2517] A.G. Riess, et al., Milky way cepheid standards for measuring cosmic distances and application to gaia DR2: Implications for the hubble constant, Astrophys. J. 861 (2) (2018) 126, arXiv:1804.10655.

[2518] S. Vagnozzi, Consistency tests of ΛCDM from the early integrated Sachs-Wolfe effect: Implications for early-time new physics and the Hubble tension, Phys. Rev. D 104 (6) (2021) 063524, arXiv:2105.10425.

[2519] G. Ye, B. Hu, Y.-S. Piao, Implication of the Hubble tension for the primordial universe in light of recent cosmological data, Phys. Rev. D 104 (6) (2021) 063510, arXiv:2103.09729.

[2520] I.d.O.C. Pedreira, M. Benetti, E.G.M. Ferreira, L.L. Graef, L. Herold, Visual tool for assessing tension-resolving models in the H0-σ8 plane, Phys. Rev. D 109 (10) (2024) 103525, arXiv:2311.04977.

[2521] BOSS Collaboration, H. Gil-Marín, et al., The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies, Mon. Not. R. Astron. Soc. 460 (4) (2016) 4188-4209, arXiv:1509.06386.

[2522] BOSS Collaboration, H. Gil-Marín, et al., The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: BAO measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies, Mon. Not. R. Astron. Soc. 460 (4) (2016) 4210-4219, arXiv:1509.06373.

[2523] eBOSS Collaboration, V. de Sainte Agathe, et al., Baryon acoustic oscillations at z=2.34 from the correlations of lyα absorption in eBOSS DR14, Astron. Astrophys. 629 (2019) A85, arXiv:1904.03400.

[2524] M.M. Ivanov, E. McDonough, J.C. Hill, M. Simonović, M.W. Toomey, S. Alexander, M. Zaldarriaga, Constraining early dark energy with large-scale structure, Phys. Rev. D 102 (10) (2020) 103502, arXiv:2006.11235.

[2525] G. D'Amico, L. Senatore, P. Zhang, H. Zheng, The hubble tension in light of the full-shape analysis of large-scale structure data, J. Cosmol. Astropart. Phys. 05 (2021) 072, arXiv:2006.12420.

[2526] F. Beutler, P. McDonald, Unified galaxy power spectrum measurements from 6dFGS, BOSS, and eBOSS, J. Cosmol. Astropart. Phys. 11 (2021) 031, arXiv: 2106.06324.

[2527] D. Piras, L. Herold, L. Lucie-Smith, E. Komatsu, ΛCDM and early dark energy in latent space: A data-driven parametrization of the CMB temperature power spectrum, Phys. Rev. D 111 (8) (2025) 083537, arXiv:2502.09810.

[2528] J.C. Hill, et al., Atacama Cosmology Telescope: Constraints on prerecombination early dark energy, Phys. Rev. D 105 (12) (2022) 123536, arXiv: 2109.04451.

[2529] A. La Posta, T. Louis, X. Garrido, J.C. Hill, Constraints on prerecombination early dark energy from SPT-3G public data, Phys. Rev. D 105 (8) (2022) 083519, arXiv:2112.10754.

[2530] T.L. Smith, M. Lucca, V. Poulin, G.F. Abellan, L. Balkenhol, K. Benabed, S. Galli, R. Murgia, Hints of early dark energy in Planck, SPT, and ACT data: New physics or systematics? Phys. Rev. D 106 (4) (2022) 043526, arXiv:2202.09379.

[2531] J.-Q. Jiang, Y.-S. Piao, Toward early dark energy and ns=1 with Planck, ACT, and SPT observations, Phys. Rev. D 105 (10) (2022) 103514, arXiv: 2022.13379.

[2532] G. Benevento, W. Hu, M. Raveri, Can late dark energy transitions raise the hubble constant? Phys. Rev. D 101 (10) (2020) 103517, arXiv:2002.11707.

[2533] D. Camarena, V. Marra, On the use of the local prior on the absolute magnitude of type Ia supernovae in cosmological inference, Mon. Not. R. Astron. Soc. 504 (2021) 5164-5171, arXiv:2101.08641.

[2534] G. Efstathiou, To H0 or not to H0? Mon. Not. R. Astron. Soc. 505 (3) (2021) 3866-3872, arXiv:2103.08723.

[2535] G. Efstathiou, S. Gratton, A detailed description of the CamSpec likelihood pipeline and a reanalysis of the Planck high frequency maps, 2019, arXiv: 1910.00483.

[2536] Planck Collaboration, Y. Akrami, et al., Planck intermediate results. VII. Joint Planck LFI and HFI data processing, Astron. Astrophys. 643 (2020) A42, arXiv:2007.04997.

[2537] J.-Q. Jiang, G. Ye, Y.-S. Piao, Impact of the Hubble tension on the r-ns contour, Phys. Lett. B 851 (2024) 138588, arXiv:2303.12345.

[2538] W. Liu, H. Zhan, Y. Gong, X. Wang, Can early dark energy be probed by the high-redshift galaxy abundance? Mon. Not. R. Astron. Soc. 533 (1) (2024) 860-871, arXiv:2402.14339.

[2539] M. Boylan-Kolchin, D.R. Weisz, Uncertain times: the redshift-time relation from cosmology and stars, Mon. Not. R. Astron. Soc. 505 (2) (2021) 2764-2783, arXiv:2103.15825.

[2540] P. Diego-Palazuelos, et al., Cosmic birefringence from Planck public release 4, in: 56th Rencontres de Morion on Cosmology, 2022, arXiv:2203.04830.

[2541] K. Murai, F. Naokawa, T. Namikawa, E. Komatsu, Isotropic cosmic birefringence from early dark energy, Phys. Rev. D 107 (4) (2023) L041302, arXiv:2209.07804.

[2542] J.R. Eskilt, L. Herold, E. Komatsu, K. Murai, T. Namikawa, F. Naokawa, Constraints on early dark energy from isotropic cosmic birefringence, Phys. Rev. Lett. 131 (12) (2023) 121001, arXiv:2303.15369.

[2543] L. Yin, J. Kochappan, T. Ghosh, B.-H. Lee, Is cosmic birefringence model-dependent? J. Cosmol. Astropart. Phys. 10 (2023) 007, arXiv:2305. 07937.

[2544] L. Hart, J. Chluba, Using the cosmological recombination radiation to probe early dark energy and fundamental constant variations, Mon. Not. R. Astron. Soc. 519 (3) (2023) 3664-3680, arXiv:2209.12290.

[2545] T. Rudelius, Constraints on early dark energy from the axion weak gravity conjecture, J. Cosmol. Astropart. Phys. 01 (2023) 014, arXiv:2203.05575.

[2546] A. Hebecker, P. Mangat, S. Theisen, L.T. Witkowski, Can gravitational instantons really constrain axion inflation? JHEP 02 (2017) 097, arXiv:1607. 06814.

[2547] B. Heidenreich, M. Reece, T. Rudelius, Sharpening the weak gravity conjecture with dimensional reduction, JHEP 02 (2016) 140, arXiv:1509.06374.

[2548] J.-Q. Jiang, G. Ye, Y.-S. Piao, Return of Harrison-Zeldovich spectrum in light of recent cosmological tensions, Mon. Not. R. Astron. Soc. 527 (1) (2023) L54-L59, arXiv:2210.06125.

[2549] Z.-Y. Peng, Y.-S. Piao, Testing the ns-H0 scaling relation with Planck-independent CMB data, Phys. Rev. D 109 (2) (2024) 023519, arXiv:2308. 01012.

[2550] H. Wang, G. Ye, J.-Q. Jiang, Y.-S. Piao, Towards primordial gravitational waves and ns=1 in light of BICEP/Keck, DESI BAO and Hubble tension, 2024, arXiv:2409.17879.

[2551] R. Kallosh, A. Linde, Hybrid cosmological attractors, Phys. Rev. D 106 (2) (2022) 023522, arXiv:2204.02425.

[2552] G. Ye, J.-Q. Jiang, Y.-S. Piao, Toward inflation with ns=1 in light of the Hubble tension and implications for primordial gravitational waves, Phys. Rev. D 106 (10) (2022) 103528, arXiv:2205.02478.
[2553] F. Niedermann, M.S. Sloth, New early dark energy as a solution to the $H_0$ and $S_8$ tensions, 2023, arXiv:2307.03481.

[2554] F. Niedermann, M.S. Sloth, New early dark energy, Phys. Rev. D 103 (4) (2021) L041303, arXiv:1910.10739.

[2555] K. Freese, M.W. Winkler, Chain early dark energy: A proposal for solving the Hubble tension and explaining today's dark energy, Phys. Rev. D 104 (8) (2021) 083533, arXiv:2102.13655.

[2556] J.S. Cruz, F. Niedermann, M.S. Sloth, Cold new early dark energy pulls the trigger on the $H_0$ and $S_8$ tensions: a simultaneous solution to both tensions without new ingredients, J. Cosmol. Astropart. Phys. 11 (2023) 033, arXiv:2305.08895.

[2557] F. Niedermann, M.S. Sloth, New early dark energy is compatible with current LSS data, Phys. Rev. D 103 (10) (2021) 103537, arXiv:2009.00006.

[2558] B.S. Haridasu, H. Khoraminezhad, M. Viel, Scrutinizing early dark energy models through CMB lensing, 2022, arXiv:2212.09136.

[2559] J.S. Cruz, F. Niedermann, M.S. Sloth, A grounded perspective on new early dark energy using ACT, SPT, and BICEP/Keck, J. Cosmol. Astropart. Phys. 02 (2023) 041, arXiv:2209.02708.

[2560] I.J. Allali, M.P. Hertzberg, F. Rompineve, Dark sector to restore cosmological concordance, Phys. Rev. D 104 (8) (2021) L081303, arXiv:2104.12798.

[2561] D. Aloni, A. Berlin, M. Joseph, M. Schmaltz, N. Weiner, A step in understanding the Hubble tension, Phys. Rev. D 105 (12) (2022) 123516, arXiv:2111.00014.

[2562] F. Niedermann, M.S. Sloth, Hot new early dark energy, Phys. Rev. D 105 (6) (2022) 063509, arXiv:2112.00770.

[2563] F. Niedermann, M.S. Sloth, Hot new early dark energy: Towards a unified dark sector of neutrinos, dark energy and dark matter, Phys. Lett. B 835 (2022) 137555, arXiv:2112.00759.

[2564] M. Garny, F. Niedermann, H. Rubira, M.S. Sloth, Hot new early dark energy bridging cosmic gaps: Supercooled phase transition reconciles stepped dark radiation solutions to the Hubble tension with BBN, Phys. Rev. D 110 (2) (2024) 023531, arXiv:2404.07256.

[2565] N. Schöneberg, G. Franco Abellán, A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension, J. Cosmol. Astropart. Phys. 12 (2022) 001, arXiv:2206.11276.

[2566] A. Berlin, N. Blinov, Thermal dark matter below an MeV, Phys. Rev. Lett. 120 (2) (2018) 021801, arXiv:1706.07046.

[2567] M. Berbig, S. Jana, A. Trautner, The Hubble tension and a renormalizable model of gauged neutrino self-interactions, Phys. Rev. D 102 (11) (2020) 115008, arXiv:2004.13039.

[2568] M. Escudero, T. Schwetz, J. Terol-Calvo, A seesaw model for large neutrino masses in concordance with cosmology, JHEP 02 (2023) 142, arXiv:2211.01729; Addendum., JHEP 06 (2024) 119.

[2569] D. Aloni, M. Joseph, M. Schmaltz, N. Weiner, Dark radiation from neutrino mixing after big bang nucleosynthesis, Phys. Rev. Lett. 131 (22) (2023) 221001, arXiv:2301.10792.

[2570] W. Fischler, J. Meyers, Dark radiation emerging after big bang nucleosynthesis? Phys. Rev. D 83 (2011) 063520, arXiv:1011.3501.

[2571] D. Hooper, F.S. Queiroz, N.Y. Gnedin, Non-thermal dark matter mimicking an additional neutrino species in the early universe, Phys. Rev. D 85 (2012) 063513, arXiv:1111.6599.

[2572] O.E. Bjælde, S. Das, A. Moss, Origin of delta $N_{eff}$ as a result of an interaction between dark radiation and dark matter, J. Cosmol. Astropart. Phys. 10 (2012) 017, arXiv:1205.0553.

[2573] K. Choi, K.-Y. Choi, C.S. Shin, Dark radiation and small-scale structure problems with decaying particles, Phys. Rev. D 86 (2012) 083529, arXiv:1208.2496.

[2574] A. Nygaard, E.B. Holm, T. Tram, S. Hannestad, Decaying dark matter and the hubble tension, 2023, arXiv:2307.00418.

[2575] S. Garciazo, O. Mena, On the dark radiation role in the Hubble constant tension, 2023, arXiv:2306.15067.

[2576] G. Steigman, D.N. Schramm, J.E. Gunn, Cosmological limits to the number of massive leptons, Phys. Lett. B 66 (1977) 202-204.

[2577] M. Archidiacono, E. Giusarma, S. Hannestad, O. Mena, Cosmic dark radiation and neutrinos, Adv. High Energy Phys. 2013 (2013) 191047, arXiv:1307.0637.

[2578] M. Archidiacono, S. Garciazo, Two sides of the same coin: Sterile neutrinos and dark radiation, status and perspectives, Universe 8 (3) (2022) 175, arXiv:2201.10319.

[2579] K. Akita, M. Yamaguchi, A precision calculation of relic neutrino decoupling, J. Cosmol. Astropart. Phys. 08 (2020) 012, arXiv:2005.07047.

[2580] J. Froustey, C. Pitrou, M.C. Volpe, Neutrino decoupling including flavour oscillations and primordial nucleosynthesis, J. Cosmol. Astropart. Phys. 12 (2020) 015, arXiv:2008.01074.

[2581] J.J. Bennett, G. Buldgen, P.F. De Salas, M. Drewes, S. Garciazo, S. Pastor, Y.Y.Y. Wong, Towards a precision calculation of $N_{eff}$ in the standard model II: Neutrino decoupling in the presence of flavour oscillations and finite-temperature QED, J. Cosmol. Astropart. Phys. 04 (2021) 073, arXiv:2012.02726.

[2582] M. Drewes, Y. Georis, M. Klasen, L.P. Wiggering, Y.Y.Y. Wong, Towards a precision calculation of $N_{eff}$ in the standard model. Part III. Improved estimate of NLO contributions to the collision integral, J. Cosmol. Astropart. Phys. 06 (2024) 032, arXiv:2402.18481.

[2583] L. García, J. Tejeiro, L. Castañeda, Primordial nucleosynthesis in the presence of sterile neutrinos, in: A. Bracco, E. Nappi (Eds.), Proc. Int. Sch. Phys. Fermi 178 (2011) 309-316.

[2584] L.A. Anchordoqui, H. Goldberg, Neutrino cosmology after WMAP 7-year data and LHC first Z' bounds, Phys. Rev. Lett. 108 (2012) 081805, arXiv:1111.7264.

[2585] L.A. Anchordoqui, H. Goldberg, G. Steigman, Right-handed neutrinos as the dark radiation: Status and forecasts for the LHC, Phys. Lett. B 718 (2013) 1162-1165, arXiv:1211.0186.

[2586] T.D. Jacques, L.M. Krauss, C. Lunardini, Additional light sterile neutrinos and cosmology, Phys. Rev. D 87 (8) (2013) 083515, arXiv:1301.3119; Erratum; Phys. Rev. D 88 (2013) 109901.

[2587] S. Roy Choudhury, S. Choubey, Constraining light sterile neutrino mass with the BICEP2/Keck array 2014 B-mode polarization data, Eur. Phys. J. C 79 (7) (2019) 557, arXiv:1807.10294.

[2588] S. Weinberg, Goldstone Bosons as fractional cosmic neutrinos, Phys. Rev. Lett. 110 (24) (2013) 241301, arXiv:1305.1971.

[2589] W. Lin, L. Visinelli, D. Xu, T.T. Yanagida, Neutrino astronomy as a probe of physics beyond the standard model: Decay of sub-MeV B-L gauge boson dark matter, Phys. Rev. D 106 (7) (2022) 075011, arXiv:2202.04496.

[2590] P. Arias, D. Cadamuro, M. Goodsell, J. Jaackel, J. Redondo, A. Ringwald, WISPY cold dark matter, J. Cosmol. Astropart. Phys. 06 (2012) 013, arXiv:1201.5902.

[2591] D.J.E. Marsh, Axion cosmology, Phys. Rep. 643 (2016) 1-79, arXiv:1510.07633.

[2592] D. Baumann, D. Green, B. Wallisch, New target for cosmic axion searches, Phys. Rev. Lett. 117 (17) (2016) 171301, arXiv:1604.08614.

[2593] F. D'Eramo, R.Z. Ferreira, A. Notari, J.L. Bernal, Hot axions and the $H_0$ tension, J. Cosmol. Astropart. Phys. 11 (2018) 014, arXiv:1808.07430.

[2594] E.G.M. Ferreira, Ultra-light dark matter, Astron. Astrophys. Rev. 29 (1) (2021) 7, arXiv:2005.03254.

[2595] Y.K. Semertzidis, S. Youn, Axion dark matter: How to see it? Sci. Adv. 8 (8) (2022) abm9928, arXiv:2104.14831.

[2596] F. Chadha-Day, J. Ellis, D.J.E. Marsh, Axion dark matter: What is it and why now? Sci. Adv. 8 (8) (2022) abj3618, arXiv:2105.01406.

[2597] D. Green, Y. Guo, B. Wallisch, Cosmological implications of axion-matter couplings, J. Cosmol. Astropart. Phys. 02 (02) (2022) 019, arXiv:2109.12088.

[2598] C.A.J. O'Hare, Cosmology of axion dark matter, PoS COSMICWISPers (2024) 040, arXiv:2403.17697.

[2599] L. Caloni, M. Gerbino, M. Lattanzi, L. Visinelli, Novel cosmological bounds on thermally-produced axion-like particles, J. Cosmol. Astropart. Phys. 09 (2022) 021, arXiv:2205.01637.

[2600] F. D'Eramo, E. Di Valentino, W. Giarè, F. Hajkarim, A. Melchiorri, O. Mena, F. Renzi, S. Yun, Cosmological bound on the QCD axion mass, redux, J. Cosmol. Astropart. Phys. 09 (2022) 022, arXiv:2205.07849.

[2601] J.M. Cline, Z. Liu, W. Xue, Millicharged atomic dark matter, Phys. Rev. D 85 (2012) 101302, arXiv:1201.4858.

[2602] J. Fan, A. Katz, L. Randall, M. Reece, Double-disk dark matter, Phys. Dark Univ. 2 (2013) 139-156, arXiv:1303.1521.

[2603] H. Vogel, J. Redondo, Dark radiation constraints on minicharged particles in models with a hidden photon, J. Cosmol. Astropart. Phys. 02 (2014) 029, arXiv:1311.2600.

[2604] K. Petraki, L. Pearce, A. Kusenko, Self-interacting asymmetric dark matter coupled to a light massive dark photon, J. Cosmol. Astropart. Phys. 07 (2014) 039, arXiv:1403.1077.

[2605] R. Foot, S. Vagnozzi, Dissipative hidden sector dark matter, Phys. Rev. D 91 (2015) 023512, arXiv:1409.7174.

[2606] R. Foot, S. Vagnozzi, Diurnal modulation signal from dissipative hidden sector dark matter, Phys. Lett. B 748 (2015) 61-66, arXiv:1412.0762.

[2607] R. Foot, S. Vagnozzi, Solving the small-scale structure puzzles with dissipative dark matter, J. Cosmol. Astropart. Phys. 07 (2016) 013, arXiv:1602.02467.

[2608] V.V. Flambaum, I.B. Samsonov, Ultralight dark photon as a model for early universe dark matter, Phys. Rev. D 100 (6) (2019) 063541, arXiv:1908.09432.

[2609] L.A. Anchordoqui, S.E. Perez Bergliaffa, Hot thermal universe endowed with massive dark vector fields and the hubble tension, Phys. Rev. D 100 (12) (2019) 123525, arXiv:1910.05860.

[2610] G. Steigman, Equivalent neutrinos, light WIMPs, and the chimera of dark radiation, Phys. Rev. D 87 (10) (2013) 103517, arXiv:1303.0049.

[2611] C. Brust, D.E. Kaplan, M.T. Walters, New light species and the CMB, JHEP 12 (2013) 058, arXiv:1303.5379.

[2612] R.C. Nunes, A. Bonilla, Probing the properties of relic neutrinos using the cosmic microwave background, the Hubble Space Telescope and galaxy clusters, Mon. Not. R. Astron. Soc. 473 (4) (2018) 4404-4409, arXiv:1710.10264.

[2613] A. Bonilla, R.C. Nunes, E.M.C. Abreu, Forecast on lepton asymmetry from future CMB experiments, Mon. Not. R. Astron. Soc. 485 (2) (2019) 2486-2491, arXiv:1810.06356.
[2614] NANOGrav Collaboration, Z. Arzoumanian, et al., The NANOGrav 12.5 yr data set: Search for an isotropic stochastic gravitational-wave background, Astrophys. J. Lett. 905 (2) (2020) L34, arXiv:2009.04496.

[2615] B. Goncharov, et al., On the evidence for a common-spectrum process in the search for the nanohertz gravitational-wave background with the parkes pulsar timing array, Astrophys. J. Lett. 917 (2) (2021) L19, arXiv:2107.12112.

[2616] EPTA Collaboration, S. Chen, et al., Common-red-signal analysis with 24-yr high-precision timing of the European Pulsar Timing Array: inferences in the stochastic gravitational-wave background search, Mon. Not. R. Astron. Soc. 508 (4) (2021) 4970-4993, arXiv:2110.13184.

[2617] J. Antoniadis, et al., The International Pulsar Timing Array second data release: Search for an isotropic gravitational wave background, Mon. Not. R. Astron. Soc. 510 (4) (2022) 4873-4887, arXiv:2201.03980.

[2618] B. Allen, J.D. Romano, Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities, Phys. Rev. D 59 (1999) 102001, arXiv:gr-qc/9710117.

[2619] T.L. Smith, E. Pierpaoli, M. Kamionkowski, A new cosmic microwave background constraint to primordial gravitational waves, Phys. Rev. Lett. 97 (2006) 021301, arXiv:astro-ph/0603144.

[2620] L.A. Boyle, A. Buonanno, Relating gravitational wave constraints from primordial nucleosynthesis, pulsar timing, laser interferometers, and the CMB: Implications for the early Universe, Phys. Rev. D 78 (2008) 043531, arXiv:0708.2279.

[2621] S. Kuroyanagi, T. Takahashi, S. Yokoyama, Blue-tilted tensor spectrum and thermal history of the universe, J. Cosmol. Astropart. Phys. 02 (2015) 003, arXiv:1407.4785.

[2622] G. Cabass, L. Pagano, L. Salvati, M. Gerbino, E. Giusarma, A. Melchiorri, Updated constraints and forecasts on primordial tensor modes, Phys. Rev. D 93 (6) (2016) 063508, arXiv:1511.05146.

[2623] I. Ben-Dayan, B. Keating, D. Leon, I. Wolfson, Constraints on scalar and tensor spectra from $N_{eff}$, J. Cosmol. Astropart. Phys. 06 (2019) 007, arXiv:1903.11843.

[2624] M. Aich, Y.-Z. Ma, W.-M. Dai, J.-Q. Xia, How much primordial tensor mode is allowed? Phys. Rev. D 101 (6) (2020) 063536, arXiv:1912.00995.

[2625] W. Giarè, M. Forconi, E. Di Valentino, A. Melchiorri, Towards a reliable calculation of relic radiation from primordial gravitational waves, Mon. Not. R. Astron. Soc. 520 (2023) 2, arXiv:2210.14159.

[2626] NANOGrav Collaboration, A. Afzal, et al., The NANOGrav 15 yr data set: Search for signals from new physics, Astrophys. J. Lett. 951 (1) (2023) L11, arXiv:2306.16219;

Erratum: Astrophys. J. Lett. 971 (2024) L27;

Erratum: Astrophys. J. 971 (2024) L27.

[2627] M. Benetti, L.L. Graef, S. Vagnozzi, Primordial gravitational waves from NANOGrav: A broken power-law approach, Phys. Rev. D 105 (4) (2022) 043520, arXiv:2111.04758.

[2628] S. Vagnozzi, Inflationary interpretation of the stochastic gravitational wave background signal detected by pulsar timing array experiments, JHEAp 39 (2023) 81-98, arXiv:2306.16912.

[2629] M. Kawasaki, K. Kohri, N. Sugiyama, Cosmological constraints on late time entropy production, Phys. Rev. Lett. 82 (1999) 4168, arXiv:astro-ph/9811437.

[2630] G. Gelmini, S. Palomares-Ruiz, S. Pascoli, Low reheating temperature and the visible sterile neutrino, Phys. Rev. Lett. 93 (2004) 081302, arXiv:astro-ph/0403323.

[2631] P.F. de Salas, M. Lattanzi, G. Mangano, G. Miele, S. Pastor, O. Pisanti, Bounds on very low reheating scenarios after Planck, Phys. Rev. D 92 (12) (2015) 123534, arXiv:1511.00672.

[2632] M. Gerbino, K. Freese, S. Vagnozzi, M. Lattanzi, O. Mena, E. Giusarma, S. Ho, Impact of neutrino properties on the estimation of inflationary parameters from current and future observations, Phys. Rev. D 95 (4) (2017) 043512, arXiv:1610.08830.

[2633] Z. Hou, R. Keisler, L. Knox, M. Millea, C. Reichardt, How massless neutrinos affect the cosmic microwave background damping tail, Phys. Rev. D 87 (2013) 083008, arXiv:1104.2333.

[2634] D. Baumann, Primordial cosmology, PoS TASI2017 (2018) 009, arXiv:1807.03098.

[2635] S. Vagnozzi, Cosmological searches for the neutrino mass scale and mass ordering, 2019, arXiv:1907.08010.

[2636] E. Di Valentino, A. Melchiorri, J. Silk, Reconciling Planck with the local value of $H_0$ in extended parameter space, Phys. Lett. B 761 (2016) 242-246, arXiv:1606.00634.

[2637] S. Vagnozzi, New physics in light of the $H_0$ tension: An alternative view, Phys. Rev. D 102 (2) (2020) 023518, arXiv:1907.07569.

[2638] S. Bashinsky, U. Seljak, Neutrino perturbations in CMB anisotropy and matter clustering, Phys. Rev. D 69 (2004) 083002, arXiv:astro-ph/0310198.

[2639] B. Follin, L. Knox, M. Millea, Z. Pan, First detection of the acoustic oscillation phase shift expected from the cosmic neutrino background, Phys. Rev. Lett. 115 (9) (2015) 091301, arXiv:1503.07863.

[2640] E. Di Valentino, A. Melchiorri, J. Silk, Cosmological constraints in extended parameter space from the Planck 2018 Legacy release, J. Cosmol. Astropart. Phys. 01 (2020) 013, arXiv:1908.01391.

[2641] O. Seto, Y. Toda, Comparing early dark energy and extra radiation solutions to the hubble tension with BBN, Phys. Rev. D 103 (12) (2021) 123501, arXiv:2101.03740.

[2642] S. Hagstotz, P.F. de Salas, S. Garciaio, M. Gerbino, M. Lattanzi, S. Vagnozzi, K. Freese, S. Pastor, Bounds on light sterile neutrino mass and mixing from cosmology and laboratory searches, Phys. Rev. D 104 (12) (2021) 123524, arXiv:2003.02289.

[2643] G. Barenboim, W.H. Kinney, W.-I. Park, Flavor versus mass eigenstates in neutrino asymmetries: implications for cosmology, Eur. Phys. J. C 77 (9) (2017) 590, arXiv:1609.03200.

[2644] O. Seto, Y. Toda, Hubble tension in lepton asymmetric cosmology with an extra radiation, Phys. Rev. D 104 (6) (2021) 063019, arXiv:2104.04381.

[2645] D. Baumann, D. Green, J. Meyers, B. Wallisch, Phases of new physics in the CMB, J. Cosmol. Astropart. Phys. 01 (2016) 007, arXiv:1508.06342.

[2646] N. Blinov, G. Marques-Tavares, Interacting radiation after Planck and its implications for the hubble tension, J. Cosmol. Astropart. Phys. 09 (2020) 029, arXiv:2003.08387.

[2647] D.E. Kaplan, G.Z. Krnjaic, K.R. Rehmann, C.M. Wells, Atomic dark matter, J. Cosmol. Astropart. Phys. 05 (2010) 021, arXiv:0909.0753.

[2648] F.-Y. Cyr-Racine, K. Sigurdson, Cosmology of atomic dark matter, Phys. Rev. D 87 (10) (2013) 103515, arXiv:1209.5752.

[2649] S. Bansal, J. Barron, D. Curtin, Y. Tsai, Precision cosmological constraints on atomic dark matter, JHEP 10 (2023) 095, arXiv:2212.02487.

[2650] Z. Chacko, D. Curtin, M. Geller, Y. Tsai, Cosmological signatures of a mirror twin higgs, JHEP 09 (2018) 163, arXiv:1803.03263.

[2651] F.-Y. Cyr-Racine, K. Sigurdson, Limits on neutrino-neutrino scattering in the early universe, Phys. Rev. D 90 (12) (2014) 123533, arXiv:1306.1536.

[2652] M. Archidiacono, S. Hannestad, Updated constraints on non-standard neutrino interactions from Planck, J. Cosmol. Astropart. Phys. 07 (2014) 046, arXiv:1311.3873.

[2653] L. Lancaster, F.-Y. Cyr-Racine, L. Knox, Z. Pan, A tale of two modes: Neutrino free-streaming in the early universe, J. Cosmol. Astropart. Phys. 07 (2017) 033, arXiv:1704.06657.

[2654] I.M. Oldengott, T. Tram, C. Rampf, Y.Y.Y. Wong, Interacting neutrinos in cosmology: exact description and constraints, J. Cosmol. Astropart. Phys. 11 (2017) 027, arXiv:1706.02123.

[2655] G. Barenboim, P.B. Denton, I.M. Oldengott, Constraints on inflation with an extended neutrino sector, Phys. Rev. D 99 (8) (2019) 083515, arXiv:1903.02036.

[2656] A. Das, S. Ghosh, Flavor-specific interaction favors strong neutrino self-coupling in the early universe, J. Cosmol. Astropart. Phys. 07 (2021) 038, arXiv:2011.12315.

[2657] S. Roy Choudhury, S. Hannestad, T. Tram, Updated constraints on massive neutrino self-interactions from cosmology in light of the $H_0$ tension, J. Cosmol. Astropart. Phys. 03 (2021) 084, arXiv:2012.07519.

[2658] T. Brinckmann, J.H. Chang, M. LoVerde, Self-interacting neutrinos, the Hubble parameter tension, and the cosmic microwave background, Phys. Rev. D 104 (6) (2021) 063523, arXiv:2012.11830.

[2659] S. Roy Choudhury, S. Hannestad, T. Tram, Massive neutrino self-interactions and inflation, J. Cosmol. Astropart. Phys. 10 (2022) 018, arXiv:2207.07142.

[2660] A. Das, S. Ghosh, The magnificent ACT of flavor-specific neutrino self-interaction, J. Cosmol. Astropart. Phys. 09 (2023) 042, arXiv:2303.08843.

[2661] D. Camarena, F.-Y. Cyr-Racine, J. Houghteling, Confronting self-interacting neutrinos with the full shape of the galaxy power spectrum, Phys. Rev. D 108 (10) (2023) 103535, arXiv:2309.03941.

[2662] A. He, R. An, M.M. Ivanov, V. Gluscevic, Self-interacting neutrinos in light of large-scale structure data, Phys. Rev. D 109 (10) (2024) 103527, arXiv:2309.03956.

[2663] N. Bostan, S. Roy Choudhury, First constraints on non-minimally coupled Natural and Coleman-Weinberg inflation and massive neutrino self-interactions with Planck+BICEP/Keck, J. Cosmol. Astropart. Phys. 07 (2024) 032, arXiv:2310.01491.

[2664] N. Blinov, K.J. Kelly, G.Z. Krnjaic, S.D. McDermott, Constraining the self-interacting neutrino interpretation of the hubble tension, Phys. Rev. Lett. 123 (19) (2019) 191102, arXiv:1905.02727.

[2665] S.S. da Costa, D.R. da Silva, Á.S. de Jesus, N. Pinto-Neto, F.S. Queiroz, The H₀ trouble: confronting non-thermal dark matter and phantom cosmology with the CMB, BAO, and type Ia supernovae data, J. Cosmol. Astropart. Phys. 04 (2024) 035, arXiv:2311.07420.

[2666] M. Escudero, S.J. Witte, A CMB search for the neutrino mass mechanism and its relation to the Hubble tension, Eur. Phys. J. C 80 (4) (2020) 294, arXiv:1909.04044.

[2667] G. Barenboim, U. Nierste, Modified majoron model for cosmological anomalies, Phys. Rev. D 104 (2) (2021) 023013, arXiv:2005.13280.

[2668] M. Escudero, S.J. Witte, The hubble tension as a hint of leptogenesis and neutrino mass generation, Eur. Phys. J. C 81 (6) (2021) 515, arXiv:2103.03249.

[2669] M. Archidiacono, S. Hannestad, R.S. Hansen, T. Tram, Cosmology with self-interacting sterile neutrinos and dark matter - A pseudoscalar model, Phys. Rev. D 91 (6) (2015) 065021, arXiv:1404.5915.
[2670] F. Forastieri, M. Lattanzi, G. Mangano, A. Mirizzi, P. Natoli, N. Saviano, Cosmic microwave background constraints on secret interactions among sterile neutrinos, J. Cosmol. Astropart. Phys. 07 (2017) 038, arXiv:1704.00626.

[2671] M. Archidiacono, S. Garciao, C. Giunti, S. Hannestad, T. Tram, Sterile neutrino self-interactions: $H_0$ tension and short-baseline anomalies, J. Cosmol. Astropart. Phys. 12 (2020) 029, arXiv:2006.12885.

[2672] M.A. Corona, R. Murgia, M. Cadeddu, M. Archidiacono, S. Garciao, C. Giunti, S. Hannestad, Pseudoscalar sterile neutrino self-interactions in light of Planck, SPT and ACT data, J. Cosmol. Astropart. Phys. 06 (06) (2022) 010, arXiv:2112.00037.

[2673] M. Joseph, D. Aloni, M. Schmaltz, E.N. Sivarajan, N. Weiner, A step in understanding the S8 tension, Phys. Rev. D 108 (2) (2023) 023520, arXiv:2207.03500.

[2674] H. Bagherian, M. Joseph, M. Schmaltz, E.N. Sivarajan, Confronting interacting radiation models for the Hubble tension with Lyman-$\alpha$ data, Phys. Rev. D 111 (4) (2025) 043513, arXiv:2405.17554.

[2675] W. Cho, K.-Y. Choi, S. Mahapatra, Reconciling cosmological tensions with inelastic dark matter and dark radiation in a U(1)D framework, J. Cosmol. Astropart. Phys. 09 (2024) 065, arXiv:2408.03004.

[2676] W. Yang, E. Di Valentino, S. Pan, Y. Wu, J. Lu, Dynamical dark energy after Planck CMB final release and $H_0$ tension, Mon. Not. R. Astron. Soc. 501 (4) (2021) 5845-5858, arXiv:2101.02168.

[2677] F. Dong, C. Park, S.E. Hong, J. Kim, H. Seong Hwang, H. Park, S. Appleby, Tomographic Alcock-Paczynski test with Redshift-space correlation function: Evidence for the dark energy equation-of-state parameter $w > -1$, Astrophys. J. 951 (1) (2023) 98, arXiv:2305.00206.

[2678] M. Najafi, S. Pan, E. Di Valentino, J.T. Firouzjaee, Dynamical dark energy confronted with multiple CMB missions, Phys. Dark Univ. 45 (2024) 101539, arXiv:2407.14939.

[2679] S. Vagnozzi, L. Visinelli, O. Mena, D.F. Mota, Do we have any hope of detecting scattering between dark energy and baryons through cosmology? Mon. Not. R. Astron. Soc. 493 (1) (2020) 1139-1152, arXiv:1911.12374.

[2680] G. Alestas, L. Kazantzidis, L. Perivolaropoulos, $w-M$ phantom transition at $z_i < 0.1$ as a resolution of the Hubble tension, Phys. Rev. D 103 (8) (2021) 083517, arXiv:2012.13932.

[2681] W. Yang, S. Pan, E. Di Valentino, E.N. Saridakis, S. Chakraborty, Observational constraints on one-parameter dynamical dark-energy parametrizations and the $H_0$ tension, Phys. Rev. D 99 (4) (2019) 043543, arXiv:1810.05141.

[2682] V. Marra, L. Perivolaropoulos, Rapid transition of Geff at $z_t \ge 0.01$ as a possible solution of the Hubble and growth tensions, Phys. Rev. D 104 (2) (2021) 0L021303, arXiv:2102.06012.

[2683] G. Alestas, D. Camarena, E. Di Valentino, L. Kazantzidis, V. Marra, S. Nesseris, L. Perivolaropoulos, Late-transition versus smooth $H(z)$-deformation models for the resolution of the Hubble crisis, Phys. Rev. D 105 (6) (2022) 063538, arXiv:2110.04336.

[2684] G. Alestas, L. Perivolaropoulos, Late-time approaches to the Hubble tension deforming $H(z)$, worsen the growth tension, Mon. Not. R. Astron. Soc. 504 (3) (2021) 3956-3962, arXiv:2103.04045.

[2685] L. Heisenberg, H. Villarrubia-Rojo, J. Zosso, Can late-time extensions solve the $H_0$ and $\sigma_8$ tensions? Phys. Rev. D 106 (4) (2022) 043503, arXiv:2202.01202.

[2686] E. Frion, D. Camarena, L. Giani, T. Miranda, D. Bertacca, V. Marra, O.F. Piattella, Bayesian analysis of a Unified Dark Matter model with transition: can it alleviate the $H_0$ tension? Open J. Astrophys. 7 (2024) arXiv:2307.06320.

[2687] S. Kumar, R.C. Nunes, S. Pan, P. Yadav, New late-time constraints on f(R) gravity, Phys. Dark Univ. 42 (2023) 101281, arXiv:2301.07897.

[2688] S. Capozziello, G. Sarracino, G. De Somma, A critical discussion on the $H_0$ tension, Universe 10 (3) (2024) 140, arXiv:2403.12796.

[2689] D. Bousis, L. Perivolaropoulos, Hubble tension tomography: BAO vs SN la distance tension, Phys. Rev. D 110 (10) (2024) 103546, arXiv:2405.07039.

[2690] G. Alestas, L. Kazantzidis, L. Perivolaropoulos, $H_0$ tension, phantom dark energy, and cosmological parameter degeneracies, Phys. Rev. D 101 (12) (2020) 123516, arXiv:2004.08363.

[2691] R. Briffa, C. Escamilla-Rivera, J. Said Levi, J. Mifsud, N.L. Pullicino, Impact of $H_0$ priors on $f(T)$ late time cosmology, Eur. Phys. J. Plus 137 (5) (2022) 532, arXiv:2108.03853.

[2692] J. Levi Said, J. Mifsud, J. Sultana, K.Z. Adami, Reconstructing teleparallel gravity with cosmic structure growth and expansion rate data, J. Cosmol. Astropart. Phys. 06 (2021) 015, arXiv:2103.05021.

[2693] A. Theodoropoulos, L. Perivolaropoulos, The Hubble tension, the M crisis of late time $H(z)$ deformation models and the reconstruction of quintessence Lagrangians, Universe 7 (8) (2021) 300, arXiv:2109.06256.

[2694] G. Alestas, L. Perivolaropoulos, K. Tanidis, Constraining a late time transition of $G_{eff}$ using low-$z$ galaxy survey data, Phys. Rev. D 106 (2) (2022) 023526, arXiv:2201.05846.

[2695] L. Perivolaropoulos, F. Skara, Gravitational transitions via the explicitly broken symmetron screening mechanism, Phys. Rev. D 106 (4) (2022) 043528, arXiv:2203.10374.

[2696] E.A. Paraskevas, A. Cam, L. Perivolaropoulos, O. Akarsu, Transition dynamics in the $\Lambda$SCDM model: Implications for bound cosmic structures, Phys. Rev. D 109 (10) (2024) 103522, arXiv:2402.05908.

[2697] E.A. Paraskevas, L. Perivolaropoulos, Effects of a late gravitational transition on gravitational waves and anticipated constraints, Universe 9 (7) (2023) 317, arXiv:2307.00298.

[2698] L. Perivolaropoulos, F. Skara, A reanalysis of the latest SHOES data for $H_0$: Effects of new degrees of freedom on the Hubble tension, Universe 8 (10) (2022) 502, arXiv:2208.11169.

[2699] L. Perivolaropoulos, Is the Hubble crisis connected with the extinction of dinosaurs? Universe 8 (5) (2022) 263, arXiv:2201.08997.

[2700] Ö. Akarsu, J.D. Barrow, L.A. Escamilla, J.A. Vazquez, Graduated dark energy: Observational hints of a spontaneous sign switch in the cosmological constant, Phys. Rev. D 101 (6) (2020) 063528, arXiv:1912.08751.

[2701] L.A. Anchordoqui, I. Antoniadis, D. Lust, N.T. Noble, J.F. Soriano, From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension, Phys. Dark Univ. 46 (2024) 101715, arXiv:2404.17334.

[2702] A. De Felice, S. Kumar, S. Mukohyama, R.C. Nunes, Observational bounds on extended minimal theories of massive gravity: new limits on the graviton mass, J. Cosmol. Astropart. Phys. 04 (2024) 013, arXiv:2311.10530.

[2703] G. 't Hooft, Dimensional reduction in quantum gravity, Conf. Proc. C 930308 (1993) 284-296, arXiv:gr-qc/9310026.

[2704] L. Susskind, The world as a hologram, J. Math. Phys. 36 (1995) 6377-6396, arXiv:hep-th/9409089.

[2705] R. Bousso, A covariant entropy conjecture, JHEP 07 (1999) 004, arXiv:hep-th/9905177.

[2706] A.G. Cohen, D.B. Kaplan, A.E. Nelson, Effective field theory, black holes, and the cosmological constant, Phys. Rev. Lett. 82 (1999) 4971-4974, arXiv:hep-th/9803132.

[2707] S. Wang, Y. Wang, M. Li, Holographic dark energy, Phys. Rep. 696 (2017) 1-57, arXiv:1612.00345.

[2708] S. Nojiri, S.D. Odintsov, T. Paul, Different faces of generalized holographic dark energy, Symmetry 13 (6) (2021) 928, arXiv:2105.08438.

[2709] S. Nojiri, S.D. Odintsov, V.K. Oikonomou, T. Paul, Unifying holographic inflation with holographic dark energy: a covariant approach, Phys. Rev. D 102 (2) (2020) 023540, arXiv:2007.06829.

[2710] O. Trivedi, M. Khlopov, A.V. Timoshkin, Tsallis holographic dark energy with power law Ansatz approach, Symmetry 16 (4) (2024) 446, arXiv:2402.05784.

[2711] M. Tavayef, A. Sheykhi, K. Bamba, H. Moradpour, Tsallis holographic dark energy, Phys. Lett. B 781 (2018) 195-200, arXiv:1804.02983.

[2712] E.N. Saridakis, Barrow holographic dark energy, Phys. Rev. D 102 (12) (2020) 123525, arXiv:2005.04115.

[2713] H. Moradpour, S.A. Moosavi, I.P. Lobo, J.P. Morais Graça, A. Jawad, I.G. Salako, Thermodynamic approach to holographic dark energy and the Rényi entropy, Eur. Phys. J. C 78 (10) (2018) 829, arXiv:1803.02195.

[2714] N. Drepouan, A. Lymeris, E.N. Saridakis, K. Yesmakhanova, Kaniadakis holographic dark energy and cosmology, Eur. Phys. J. C 82 (5) (2022) 449, arXiv:2109.09181.

[2715] L.N. Granda, A. Oliveros, Infrared cut-off proposal for the Holographic density, Phys. Lett. B 669 (2008) 275-277, arXiv:0810.3149.

[2716] P. Mukherjee, A. Mukherjee, H.K. Jassal, A. Dasgupta, N. Banerjee, Holographic dark energy: constraints on the interaction from diverse observational data sets, Eur. Phys. J. Plus 134 (4) (2019) 147, arXiv:1710.02417.

[2717] P. Adhikary, S. Das, S. Basilakos, E.N. Saridakis, Barrow holographic dark energy in a nonflat universe, Phys. Rev. D 104 (12) (2021) 123519, arXiv:2104.13118.

[2718] H. Moradpour, A.H. Ziaie, M. Kord Zangeneh, Generalized entropies and corresponding holographic dark energy models, Eur. Phys. J. C 80 (8) (2020) 732, arXiv:2005.06271.

[2719] A. Sayahian Jahromi, S.A. Moosavi, H. Moradpour, J.P. Morais Graça, I.P. Lobo, I.G. Salako, A. Jawad, Generalized entropy formalism and a new holographic dark energy model, Phys. Lett. B 780 (2018) 21-24, arXiv:1802.07722.

[2720] O. Trivedi, A. Bidlan, P. Moniz, Fractional holographic dark energy, Phys. Lett. B 858 (2024) 139074, arXiv:2407.16685.

[2721] H. Moradpour, S. Jalalzadeh, U.K. Sharma, On the thermodynamics of reconciling quantum and gravity, Eur. Phys. J. Plus 139 (2) (2024) 170, arXiv:2304.06494.

[2722] R.-Y. Guo, J.-F. Zhang, X. Zhang, Can the $H_0$ tension be resolved in extensions to $\Lambda$CDM cosmology? J. Cosmol. Astropart. Phys. 02 (2019) 054, arXiv:1809.02340.

[2723] T. Jacobson, Thermodynamics of space-time: The Einstein equation of state, Phys. Rev. Lett. 75 (1995) 1260-1263, arXiv:gr-qc/9504004.

[2724] E.P. Verlinde, On the origin of gravity and the laws of Newton, JHEP 04 (2011) 029, arXiv:1001.0785.

[2725] T. Padmanabhan, Gravitational entropy of static space-times and microscopic density of states, Cl. Quant. Grav. 21 (2004) 4485-4494, arXiv:gr-qc/0308070.

[2726] R.-G. Cai, S.P. Kim, First law of thermodynamics and Friedmann equations of Friedmann-Robertson-Walker universe, JHEP 02 (2005) 050, arXiv:hep-th/0501055.

[2727] J.D. Bekenstein, Black holes and entropy, Phys. Rev. D 7 (1973) 2333-2346.

[2728] S.W. Hawking, Black hole explosions, Nature 248 (1974) 30-31.
[2729] G.W. Gibbons, S.W. Hawking, Cosmological event horizons, thermodynamics, and particle creation, Phys. Rev. D 15 (1977) 2738-2751.

[2730] D.A. Easson, P.H. Frampton, G.F. Smoot, Entropic accelerating universe, Phys. Lett. B 696 (2011) 273-277, arXiv:1002.4278.

[2731] H. Gohar, V. Salzano, Generalized mass-to-horizon relation: A new global approach to entropic cosmologies and its connection to ΛCDM, Phys. Rev. D 109 (8) (2024) 084075, arXiv:2307.06239.

[2732] N. Komatsu, S. Kimura, Entropic cosmology for a generalized black-hole entropy, Phys. Rev. D 88 (2013) 083534, arXiv:1307.5949.

[2733] R.C. Nunes, E.M. Barboza Jr., E.M.C. Abreu, J.A. Neto, Probing the cosmological viability of non-gaussian statistics, J. Cosmol. Astropart. Phys. 08 (2016) 051, arXiv:1509.05059.

[2734] H. Moradpour, R.C. Nunes, E.M.C. Abreu, J.A. Neto, A note on the relations between thermodynamics, energy definitions and Friedmann equations, Modern Phys. Lett. A 32 (13) (2017) 1750078, arXiv:1603.01465.

[2735] E.M.C. Abreu, J.A. Neto, E.M. Barboza, R.C. Nunes, Tsallis and Kaniadakis statistics from the viewpoint of entropic gravity formalism, Internat. J. Modern Phys. A 32 (05) (2017) 1750028, arXiv:1701.06898.

[2736] C. Tsallis, L.J.L. Cirto, Black hole thermodynamical entropy, Eur. Phys. J. C 73 (2013) 2487, arXiv:1202.2154.

[2737] J.D. Barrow, The area of a rough black hole, Phys. Lett. B 808 (2020) 135643, arXiv:2004.09444.

[2738] I. Cimidiker, M.P. Dabrowski, H. Gohar, Generalized uncertainty principle impact on nonextensive black hole thermodynamics, Cl. Quant. Grav. 40 (14) (2023) 145001, arXiv:2301.00609.

[2739] J.D. Bekenstein, Universal upper bound on the entropy-to-energy ratio for bounded systems, Phys. Rev. D 23 (2) (1981) 287-298.

[2740] M.H.P.M. van Putten, On the hubble expansion in a big bang quantum cosmology, JHEAp 45 (2025) 194-199, arXiv:2403.10865.

[2741] D. Camarena, V. Marra, Local determination of the hubble constant and the deceleration parameter, Phys. Rev. Res. 2 (1) (2020) 013028, arXiv: 1906.11814.

[2742] B. De Simone, M.H.P.M. van Putten, M.G. Dainotti, G. Lambiase, A doublet of cosmological models to challenge the H0 tension in the Pantheon Supernovae Ia catalog, JHEAp 45 (2025) 290-298, arXiv:2411.05744.

[2743] S. Basilakos, A. Lymperis, M. Petronikolou, E.N. Saridakis, Relieving both $H_0$ and $\sigma_k$ tensions in Tsallis cosmology, Eur. Phys. J. C 84 (3) (2024) 297, arXiv:2308.01200.

[2744] M. Asghari, A. Sheykhi, Observational constraints on Tsallis modified gravity, Mon. Not. R. Astron. Soc. 508 (2) (2021) 2855-2861, arXiv:2106.15551.

[2745] H. Gohar, V. Salzano, Cosmological constraints on entropic cosmology with matter creation, Eur. Phys. J. C 81 (4) (2021) 338, arXiv:2008.09635.

[2746] W.J.C. da Silva, R. Silva, Cosmological perturbations in the Tsallis holographic dark energy scenarios, Eur. Phys. J. Plus 136 (5) (2021) 543, arXiv:2011. 09520.

[2747] A. Melchiorri, L. Mersini-Houghton, C.J. Odman, M. Trodden, The state of the dark energy equation of state, Phys. Rev. D 68 (2003) 043509, arXiv:astro-ph/0211522.

[2748] A. Melchiorri, L. Mersini-Houghton, Does the low CMB quadrupole provide a new cosmic coincidence problem?, 2004, arXiv:hep-ph/0403222.

[2749] P.J. Steinhardt, L.-M. Wang, I. Zlatev, Cosmological tracking solutions, Phys. Rev. D 59 (1999) 123504, arXiv:astro-ph/9812313.

[2750] N. Roy, A.X. Gonzalez-Morales, L.A. Urena-Lopez, New general parametrization of quintessence fields and its observational constraints, Phys. Rev. D 98 (6) (2018) 063530, arXiv:1803.09204.

[2751] F.X. Linares Cedeno, N. Roy, L.A. Urena-López, Tracker phantom field and a cosmological constant: Dynamics of a composite dark energy model, Phys. Rev. D 104 (12) (2021) 123502, arXiv:2105.07103.

[2752] N. Roy, S. Goswami, S. Das, Quintessence or phantom: Study of scalar field dark energy models through a general parametrization of the Hubble parameter, Phys. Dark Univ. 36 (2022) 101037, arXiv:2201.09306.

[2753] J.A. Nájera, C. Escamilla-Rivera, Phantom scalar field cosmologies constrained by early cosmic measurements, Universe 10 (6) (2024) 232, arXiv:2403.16562.

[2754] WMAP Collaboration, G. Hinshaw, et al., Nine-year Wilkinson microwave anisotropy probe (WMAP) observations: Cosmological parameter results, Astrophys. J. Suppl. 208 (2013) 19, arXiv:1212.5226.

[2755] B. Feng, X.-L. Wang, X.-M. Zhang, Dark energy constraints from the cosmic age and supernova, Phys. Lett. B 607 (2005) 35-41, arXiv:astro-ph/0404224.

[2756] T. Qiu, Theoretical aspects of quintom models, in: K. Bamba, C.-Q. Geng (Eds.), Modern Phys. Lett. A 25 (2010) 909-921, arXiv:1002.3971.

[2757] M.-J. Zhang, H. Li, Observational constraint on the dark energy scalar field, Chin. Phys. C 45 (4) (2021) 045103, arXiv:1809.08936.

[2758] G. Leon, A. Paliathanasis, J.L. Morales-Martínez, The past and future dynamics of quintom dark energy models, Eur. Phys. J. C 78 (9) (2018) 753, arXiv: 1808.05634.

[2759] S. Panpanich, P. Burikham, S. Spongertskul, L. Tannukij, Resolving Hubble tension with quintom dark energy model, Chin. Phys. C 45 (1) (2021) 015108, arXiv:1908.03324.

[2760] D. Wang, W. Zhang, X.-H. Meng, Searching for the evidence of dynamical dark energy, Eur. Phys. J. C 79 (3) (2019) 211, arXiv:1903.08913.

[2761] L.A. Escamilla, S. Pan, E. Di Valentino, A. Paliathanasis, J.A. Vázquez, W. Yang, Testing an oscillatory behavior of dark energy, Phys. Rev. D 111 (2) (2025) 023531, arXiv:2404.00181.

[2762] J.A. Vázquez, D. Tamayo, A.A. Sen, I. Quiros, Bayesian model selection on scalar $\epsilon$-field dark energy, Phys. Rev. D 103 (4) (2021) 043506, arXiv: 2009.01904.

[2763] J.-Q. Xia, H. Li, X. Zhang, Dark energy constraints after Planck, Phys. Rev. D 88 (2013) 063501, arXiv:1308.0188.

[2764] L. Fu, L. Chen, M. Yang, J. Wang, M.-J. Zhang, A better reconciliation of hubble tension in the dark energy scalar field, Res. Astron. Astrophys. 23 (3) (2023) 035004.

[2765] N. Roy, L.A. Urena-López, Tracker behaviour of quintom dark energy and the Hubble tension, 2023, arXiv:2312.04003.

[2766] M. Cicoli, G. Dibitetto, F.G. Pedro, New accelerating solutions in late-time cosmology, Phys. Rev. D 101 (10) (2020) 103524, arXiv:2002.02695.

[2767] M. Cicoli, G. Dibitetto, F.G. Pedro, Out of the swampland with multifield quintessence? JHEP 10 (2020) 035, arXiv:2007.11011.

[2768] Y. Akrami, M. Sasaki, A.R. Solomon, V. Vardanyan, Multi-field dark energy: Cosmic acceleration on a steep potential, Phys. Lett. B 819 (2021) 136427, arXiv:2008.13660.

[2769] J.R. Eskilt, Y. Akrami, A.R. Solomon, V. Vardanyan, Cosmological dynamics of multifield dark energy, Phys. Rev. D 106 (2) (2022) 023512, arXiv:2201. 08841.

[2770] L. Anguelova, J. Dumancic, R. Gass, L.C.R. Wijewardhana, Dark energy from inspiraling in field space, J. Cosmol. Astropart. Phys. 03 (03) (2022) 018, arXiv:2111.12136.

[2771] L. Anguelova, J. Dumancic, R. Gass, L.C.R. Wijewardhana, Dynamics of inspiraling dark energy, Eur. Phys. J. C 84 (4) (2024) 365, arXiv:2311.07839.

[2772] C. Armendariz-Picon, T. Damour, V.F. Mukhanov, k - inflation, Phys. Lett. B 458 (1999) 209-218, arXiv:hep-th/9904075.

[2773] J. Garriga, V.F. Mukhanov, Perturbations in k-inflation, Phys. Lett. B 458 (1999) 219-225, arXiv:hep-th/9904176.

[2774] R.C. Batista, A short review on clustering dark energy, Universe 8 (1) (2021) 22, arXiv:2204.12341.

[2775] J. Dakin, S. Hannestad, T. Tram, M. Knabenhans, J. Stadel, Dark energy perturbations in N-body simulations, J. Cosmol. Astropart. Phys. 08 (2019) 013, arXiv:1904.05210.

[2776] F. Hassani, J. Adamek, M. Kunz, F. Vernizzi, k-Evolution: a relativistic N-body code for clustering dark energy, J. Cosmol. Astropart. Phys. 12 (2019) 011, arXiv:1910.01104.

[2777] L. Blot, P.S. Corasaniti, F. Schmidt, Non-linear Eulerian hydrodynamics of dark energy: Riemann problem and finite volume schemes, J. Cosmol. Astropart. Phys. 05 (2023) 001, arXiv:2210.04800.

[2778] R.C. Batista, H.P. de Oliveira, L.R.W. Abramo, Spherical collapse of non-top-hat profiles in the presence of dark energy with arbitrary sound speed, J. Cosmol. Astropart. Phys. 02 (2023) 037, arXiv:2210.14769.

[2779] I. Ben-Dayan, U. Kumar, Theoretical priors and the dark energy equation of state, Eur. Phys. J. C 84 (2) (2024) 167, arXiv:2310.03092.

[2780] B.R. Dinda, N. Banerjee, Constraints on the speed of sound in the k-essence model of dark energy, Eur. Phys. J. C 84 (2) (2024) 177, arXiv:2309.10538.

[2781] M. Bastero-Gil, P.H. Frampton, L. Mersini-Houghton, Modified dispersion relations from closed strings in toroidal cosmology, Phys. Rev. D 65 (2002) 106002, arXiv:hep-th/0110167.

[2782] L. Mersini-Houghton, M. Bastero-Gil, P. Kanti, Relic dark energy from transPlanckian regime, Phys. Rev. D 64 (2001) 043508, arXiv:hep-ph/ 0101210.

[2783] L. Mersini-Houghton, M. Bastero-Gil, Dark energy may probe string theory, in: 3rd International Sakharov Conference on Physics, 2002, arXiv:hep-th/ 0212153.

[2784] M. Bastero-Gil, L. Mersini-Houghton, SN1A data and the CMB of modified curvature at short and long distances, Phys. Rev. D 65 (2002) 023502, arXiv:astro-ph/0107256.

[2785] M. Bastero-Gil, L. Mersini-Houghton, Equation of state of the transPlanckian dark energy and the coincidence problem, Phys. Rev. D 67 (2003) 103519, arXiv:hep-th/0205271.

[2786] M. Bastero-Gil, K. Freese, L. Mersini-Houghton, What can WMAP tell us about the very early universe? New physics as an explanation of suppressed large scale power and running spectral index, Phys. Rev. D 68 (2003) 123514, arXiv:hep-ph/0306289.

[2787] I.L. Shapiro, J. Sola, Scaling behavior of the cosmological constant: Interface between quantum field theory and cosmology, JHEP 02 (2002) 006, arXiv: hep-th/0012227.

[2788] J. Sola, Dark energy: A quantum fossil from the inflationary Universe? in: M. Bordag, V.M. Mostepanenko (Eds.), J. Phys. A 41 (2008) 164066, arXiv: 0710.4151.

[2789] I.L. Shapiro, J. Sola, On the possible running of the cosmological 'constant', Phys. Lett. B 682 (2009) 105-113, arXiv:0910.4925.

[2790] C. Moreno-Pulido, J. Sola, Running vacuum in quantum field theory in curved spacetime: renormalizing $\rho_{vac}$ without $\sim m^4$ terms, Eur. Phys. J. C 80 (8) (2020) 692, arXiv:2005.03164.
[2791] C. Moreno-Pulido, J. Sola Peracaula, Renormalizing the vacuum energy in cosmological spacetime: implications for the cosmological constant problem, Eur. Phys. J. C 82 (6) (2022) 551, arXiv:2201.05827.

[2792] C. Moreno-Pulido, J. Sola Peracaula, S. Cheraghchi, Running vacuum in QFT in FLRW spacetime: the dynamics of $\rho_{vac}(H)$ from the quantized matter fields, Eur. Phys. J. C 83 (7) (2023) 637, arXiv:2301.05205.

[2793] J. Sola, Cosmological constant and vacuum energy: old and new ideas, in: T. Papakostas, D.A. Pliakis (Eds.), J. Phys. Conf. Ser. 453 (2013) 012015, arXiv:1306.1527.

[2794] J. Sola Peracaula, The cosmological constant problem and running vacuum in the expanding universe, Phil. Trans. Roy. Soc. Lond. A 380 (2022) 20210182, arXiv:2203.13757.

[2795] S. Basilakos, J.A.S. Lima, J. Sola, From inflation to dark energy through a dynamical Lambda: an attempt at alleviating fundamental cosmic puzzles, Internat. J. Modern Phys. D 22 (2013) 1342008, arXiv:1307.6251.

[2796] S. Basilakos, N.E. Mavromatos, J. Solà Peracaula, Scalar field theory description of the running vacuum model: the vacuumum, J. Cosmol. Astropart. Phys. 12 (2019) 025, arXiv:1901.06638.

[2797] H. Fritzsche, J. Sola, Matter non-conservation in the universe and dynamical dark energy, Cl. Quant. Grav. 29 (2012) 215002, arXiv:1202.5097.

[2798] A. Gomez-Valent, J. Sola, Vacuum models with a linear and a quadratic term in H: structure formation and number counts analysis, Mon. Not. R. Astron. Soc. 448 (2015) 2810-2821, arXiv:1412.3785.

[2799] A. Gomez-Valent, E. Karimkhani, J. Sola, Background history and cosmic perturbations for a general system of self-conserved dynamical dark energy and matter, J. Cosmol. Astropart. Phys. 12 (2015) 048, arXiv:1509.03298.

[2800] H. Fritzsche, J. Sola, Fundamental constants and cosmic vacuum: the micro and macro connection, Modern Phys. Lett. A 30 (22) (2015) 1540034, arXiv:1502.01411.

[2801] H. Fritzsche, J. Solà, R.C. Nunes, Running vacuum in the universe and the time variation of the fundamental constants of nature, Eur. Phys. J. C 77 (3) (2017) 193, arXiv:1605.06104.

[2802] J. Solà Peracaula, The dynamics of vacuum, gravity and matter: Implications on the fundamental constants, Internat. J. Modern Phys. A 39 (09n10) (2024) 2441016, arXiv:2308.13349.

[2803] J. Sola, A. Gomez-Valent, J. de Cruz Pérez, Hints of dynamical vacuum energy in the expanding universe, Astrophys. J. Lett. 811 (2015) L14, arXiv:1506.05793.

[2804] J. Solà, A. Gómez-Valent, J. de Cruz Pérez, First evidence of running cosmic vacuum: challenging the concordance model, Astrophys. J. 836 (1) (2017) 43, arXiv:1602.02103.

[2805] J. Solà Peracaula, J. de Cruz Pérez, A. Gómez-Valent, Dynamical dark energy vs. $\Lambda$=const in light of observations, EPL 121 (3) (2018) 39001, arXiv:1606.00450.

[2806] J. Solà Peracaula, J. de Cruz Pérez, A. Gomez-Valent, Possible signals of vacuum dynamics in the Universe, Mon. Not. R. Astron. Soc. 478 (4) (2018) 4357-4373, arXiv:1703.08218.

[2807] J. Solà, A. Gómez-Valent, J. de Cruz Pérez, The $H_0$ tension in light of vacuum dynamics in the Universe, Phys. Lett. B 774 (2017) 317-324, arXiv:1705.06723.

[2808] A. Gomez-Valent, J. Sola, Relaxing the $\sigma_8$-tension through running vacuum in the universe, EPL 120 (3) (2017) 39001, arXiv:1711.00692.

[2809] A. Gómez-Valent, J. Solà Peracaula, Density perturbations for running vacuum: a successful approach to structure formation and to the $\sigma_8$-tension, Mon. Not. R. Astron. Soc. 478 (1) (2018) 126-145, arXiv:1801.08501.

[2810] A. Gómez-Valent, J. Solà, S. Basilakos, Dynamical vacuum energy in the expanding universe confronted with observations: a dedicated study, J. Cosmol. Astropart. Phys. 01 (2015) 004, arXiv:1409.7048.

[2811] C.-Q. Geng, C.-C. Lee, L. Yin, Constraints on running vacuum model with $H(z)$ and $f\sigma_8$, J. Cosmol. Astropart. Phys. 08 (2017) 032, arXiv:1704.02136.

[2812] P. Tsiapi, S. Basilakos, Testing dynamical vacuum models with CMB power spectrum from Planck, Mon. Not. R. Astron. Soc. 485 (2) (2019) 2505-2510, arXiv:1810.12902.

[2813] P. Asimakis, S. Basilakos, N.E. Mavromatos, E.N. Saridakis, Big bang nucleosynthesis constraints on higher-order modified gravities, Phys. Rev. D 105 (8) (2022) 084010, arXiv:2112.10863.

[2814] J. Solà Peracaula, A. Gómez-Valent, J. de Cruz Perez, C. Moreno-Pulido, Running vacuum against the $H_0$ and $\sigma_8$ tensions, EPL 134 (1) (2021) 19001, arXiv:2102.12758.

[2815] J. Sola Peracaula, A. Gomez-Valent, J. de Cruz Perez, C. Moreno-Pulido, Running vacuum in the universe: Phenomenological status in light of the latest observations, and its impact on the $\sigma_8$ and $H_0$ tensions, Universe 9 (6) (2023) 262, arXiv:2304.11157.

[2816] J. de Cruz Perez, J. Sola Peracaula, Running vacuum in Brans & Dicke theory: A possible cure for the $\sigma_8$ and $H_0$ tensions, Phys. Dark Univ. 43 (2024) 101406, arXiv:2302.04807.

[2817] N.E. Mavromatos, Geometrical origins of the universe dark sector: string-inspired torsion and anomalies as seeds for inflation and dark matter, Phil. Trans. A. Math. Phys. Eng. Sci. 380 (2222) (2022) 20210188, arXiv:2108.02152.

[2818] N.E. Mavromatos, Lorentz symmetry violation in string-inspired effective modified gravity theories, Lect. Notes Phys. 1017 (2023) 3-48, arXiv:2205.07044.

[2819] J. Alexandre, N. Houston, N.E. Mavromatos, Starobinsky-type inflation in dynamical supergravity breaking scenarios, Phys. Rev. D 89 (2) (2014) 027703, arXiv:1312.5197.

[2820] W. Yang, E. Di Valentino, S. Pan, A. Shafieloo, X. Li, Generalized emergent dark energy model and the Hubble constant tension, Phys. Rev. D 104 (6) (2021) 063521, arXiv:2103.03815.

[2821] A. Banihashemi, N. Khosravi, A.H. Shirazi, Phase transition in the dark sector as a proposal to lessen cosmological tensions, Phys. Rev. D 101 (12) (2020) 123521, arXiv:1808.02472.

[2822] A. Banihashemi, N. Khosravi, A.H. Shirazi, Ginzburg-Landau theory of dark energy: A framework to study both temporal and spatial cosmological tensions simultaneously, Phys. Rev. D 99 (8) (2019) 083509, arXiv:1810.11007.

[2823] A. Banihashemi, N. Khosravi, A. Shafieloo, Dark energy as a critical phenomenon: a hint from Hubble tension, J. Cosmol. Astropart. Phys. 06 (2021) 003, arXiv:2012.01407.

[2824] V.L. Ginzburg, L.D. Landau, On the theory of superconductivity, in: D. ter Haar (Ed.), Zh. Eksp. Teor. Fiz. 20 (1950) 1064-1082.

[2825] A. Banihashemi, N. Khosravi, Fluctuations in the Ginzburg-Landau theory of dark energy: Internal (in)consistencies in the Planck data set, Astrophys. J. 931 (2) (2022) 148, arXiv:2201.04119.

[2826] M. Rezaei, T. Naderi, M. Malekjani, A. Mehrabi, A Bayesian comparison between $\Lambda$CDM and phenomenologically emergent dark energy models, Eur. Phys. J. C 80 (5) (2020) 374, arXiv:2004.08168.

[2827] S. Pan, W. Yang, E. Di Valentino, A. Shafieloo, S. Chakraborty, Reconciling $H_0$ tension in a six parameter space? J. Cosmol. Astropart. Phys. 06 (06) (2020) 062, arXiv:1907.12551.

[2828] R. Shah, P. Mukherjee, S. Pal, Reconciling S8: insights from interacting dark sectors, Mon. Not. R. Astron. Soc. 536 (3) (2024) 2404-2420, arXiv:2404.06396.

[2829] A. Hernández-Almada, G. Leon, J. Magaña, M.A. García-Aspeitia, V. Motta, Generalized emergent dark energy: observational hubble data constraints and stability analysis, Mon. Not. R. Astron. Soc. 497 (2) (2020) 1590-1602, arXiv:2002.12881.

[2830] W. Yang, E. Di Valentino, S. Pan, O. Mena, Emergent dark energy, neutrinos and cosmological tensions, Phys. Dark Univ. 31 (2021) 100762, arXiv:2007.02927.

[2831] Z. Liu, H. Miao, Update constraints on neutrino mass and mass hierarchy in light of dark energy models, Internat. J. Modern Phys. D 29 (13) (2020) 2050088, arXiv:2002.05563.

[2832] E. Di Valentino, S. Gariazzo, C. Giunti, O. Mena, S. Pan, W. Yang, Minimal dark energy: Key to sterile neutrino and Hubble constant tensions? Phys. Rev. D 105 (10) (2022) 103511, arXiv:2110.03990.

[2833] M.A. García-Aspeitia, G. Fernandez-Anaya, A. Hernández-Almada, G. Leon, J. Magaña, Cosmology under the fractional calculus approach, Mon. Not. R. Astron. Soc. 517 (4) (2022) 4813-4826, arXiv:2207.00878.

[2834] L. Pizzuti, I.D. Saltas, L. Amendola, Mg-mampost: a code to test modifications of gravity with internal kinematics and lensing analyses of galaxy clusters, Mon. Not. R. Astron. Soc. 506 (1) (2021) 595-612, arXiv:2011.15089.

[2835] H.B. Benaoum, W. Yang, S. Pan, E. Di Valentino, Modified emergent dark energy and its astronomical constraints, Internat. J. Modern Phys. D 31 (03) (2022) 2250015, arXiv:2008.09098.

[2836] L. Parker, A. Raval, New quantum aspects of a vacuum dominated universe, Phys. Rev. D 62 (2000) 083503, arXiv:gr-qc/0003103; Erratum; Phys. Rev. D 67 (2003) 029903.

[2837] L. Parker, D.A.T. Vanzella, Acceleration of the universe, vacuum metamorphosis, and the large time asymptotic form of the heat kernel, Phys. Rev. D 69 (2004) 104009, arXiv:gr-qc/0312108.

[2838] R.R. Caldwell, W. Komp, L. Parker, D.A.T. Vanzella, A sudden gravitational transition, Phys. Rev. D 73 (2006) 023513, arXiv:astro-ph/0507622.

[2839] E. Di Valentino, E.V. Linder, A. Melchiorri, $H_0$ ex machina: Vacuum metamorphosis and beyond $H_0$, Phys. Dark Univ. 30 (2020) 100733, arXiv:2006.16291.

[2840] G. Lambiase, S. Mohanty, A. Narang, P. Parashari, Testing dark energy models in the light of $\sigma_8$ tension, Eur. Phys. J. C 79 (2) (2019) 141, arXiv:1804.07154.

[2841] R.A. Battye, A. Moss, Evidence for massive neutrinos from cosmic microwave background and lensing observations, Phys. Rev. Lett. 112 (5) (2014) 051303, arXiv:1308.5870.

[2842] Y. Wang, K. Freese, P. Gondolo, M. Lewis, Future type IA supernova data as tests of dark energy from modified Friedmann equations, Astrophys. J. 594 (2003) 25-32, arXiv:astro-ph/0302064.

[2843] R. Lazkoz, V. Salzano, L. Fernandez-Jambrina, M. Bouhmadi-López, Ripped $\Lambda$CDM: An observational contender to the consensus cosmological model, Phys. Dark Univ. 45 (2024) 101511, arXiv:2311.14156.

[2844] L. Huang, S.-J. Wang, W.-W. Yu, No-go guide for the Hubble tension: Late-time or local-scale new physics, Sci. China Phys. Mech. Astron. 68 (2) (2025) 220413, arXiv:2401.14170.

[2845] N. Kitazawa, Late-time data require smaller sound horizon at recombination, 2023, arXiv:2310.10017.
[2846] Ruchika, 2D BAO vs 3D BAO: Hints for new physics?, 2024, arXiv:2406.05453.

[2847] R.E. Keeley, A. Shafieloo, Ruling out new physics at low redshift as a solution to the H0 tension, Phys. Rev. Lett. 131 (11) (2023) 111002, arXiv:2206.08440.

[2848] M.W. Hossain, A. Maqsood, Comparison between axionlike and power law potentials in a cosmological background, Phys. Rev. D 109 (10) (2024) 103512, arXiv:2311.17825.

[2849] C.G. Boiza, M. Bouhmadi-López, Speeding up the Universe with a generalised axion-like potential, 2024, arXiv:2409.18184.

[2850] C.G. Boiza, M. Bouhmadi-López, Cosmological perturbations in a generalised axion-like dark energy model, Phys. Dark Univ. 48 (2025) 101845, arXiv: 2410.22467.

[2851] M.W. Hossain, A. Maqsood, Cosmological implications of tracker scalar fields as dynamical dark energy, 2025, arXiv:2502.19274.

[2852] H.-W. Chiang, C.G. Boiza, M. Bouhmadi-López, Observational constraints on generalised axion-like potentials for the late universe, 2025, arXiv:2503.04898.

[2853] H. Benaoum, Accelerated universe from modified Chaplygin gas and tachyonic fluid, Universe 8 (7) (2022) 340, arXiv:hep-th/0205140.

[2854] H. Stefancic, Expansion around the vacuum equation of state - Sudden future singularities and asymptotic behavior, Phys. Rev. D 71 (2005) 084024, arXiv: astro-ph/0411630.

[2855] M. Bouhmadi-López, M. Brilenkov, R. Brilenkov, J. Morais, A. Zhuk, Scalar perturbations in the late Universe: viability of the Chaplygin gas models, J. Cosmol. Astropart. Phys. 12 (2015) 037, arXiv:1509.06963.

[2856] W. Yang, S. Pan, S. Vagnozzi, E. Di Valentino, D.F. Mota, S. Capozziello, Dawn of the dark: unified dark sectors and the EDGES Cosmic Dawn 21-cm signal, J. Cosmol. Astropart. Phys. 11 (2019) 044, arXiv:1907.05344.

[2857] I. Albarran, M. Bouhmadi-López, J. Morais, Cosmological perturbations in an effective and genuinely phantom dark energy Universe, Phys. Dark Univ. 16 (2017) 94-108, arXiv:1611.00392.

[2858] K.R. Dienes, L. Heurtier, F. Huang, D. Kim, T.M.P. Tait, B. Thomas, Stasis in an expanding universe: A recipe for stable mixed-component cosmological eras, Phys. Rev. D 105 (2) (2022) 023530, arXiv:2111.04753.

[2859] K.R. Dienes, L. Heurtier, F. Huang, T.M.P. Tait, B. Thomas, Stasis, stasis, triple stasis, Phys. Rev. D 109 (8) (2024) 083508, arXiv:2309.10345.

[2860] K.R. Dienes, L. Heurtier, F. Huang, T.M.P. Tait, B. Thomas, Cosmological stasis from dynamical scalars: Tracking solutions and the possibility of a stasis-induced inflation, Phys. Rev. D 110 (12) (2024) 123514, arXiv:2406. 06830.

[2861] L.R.W. Abramo, R.H. Brandenberger, V.F. Mukhanov, The energy - momentum tensor for cosmological perturbations, Phys. Rev. D 56 (1997) 3248-3257, arXiv:gr-qc/9704037.

[2862] R.H. Brandenberger, Back reaction of cosmological perturbations, in: 3rd International Conference on Particle Physics and the Early Universe, 2000, pp. 198-206, arXiv:hep-th/0004016.

[2863] M.A.C. Alvarez, L. Graef, R. Brandenberger, Back-reaction of super-hubble fluctuations, late time tracking and recent observational results, 2025, arXiv: 2502.17395.

[2864] L.A. Escamilla, E. Özülker, Ö. Akarsu, E. Di Valentino, J.A. Vázquez, Do we need wavelets in the late universe?, 2024, arXiv:2408.12516.

[2865] Ö. Akarsu, A. Çam, E.A. Paraskevas, L. Perivolaropoulos, Linear matter density perturbations in the ΛCDM model: Examining growth dynamics and addressing the $S_8$ tension, 2025, arXiv:2502.20384.

[2866] M. Biagetti, G. Francolini, A. Riotto, Enhancing massive galaxy formation at high redshift in non-standard cosmologies, Astrophys. J. 944 (2) (2023) 113, arXiv:2210.04812.

[2867] D. Wang, Y. Liu, JWST high redshift galaxy observations have a strong tension with Planck CMB measurements, 2022, arXiv:2301.00347.

[2868] K. Dutta, Ruchika, A. Roy, A.A. Sen, M.M. Sheikh-Jabbari, Beyond ΛCDM with low and high redshift data: implications for dark energy, Gen. Relativity Gravitation 52 (2) (2020) 15, arXiv:1808.06623.

[2869] G. Acquaviva, Ö. Akarsu, N. Katirci, J.A. Vazquez, Simple-graduated dark energy and spatial curvature, Phys. Rev. D 104 (2) (2021) 023505, arXiv: 2104.02623.

[2870] Ö. Akarsu, L. Perivolaropoulos, A. Tsikoundoura, A.E. Yükselci, A. Zhuk, Dynamical dark energy with AdS-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension, 2025, arXiv:2502.14667.

[2871] E. Ozulker, Is the dark energy equation of state parameter singular? Phys. Rev. D 106 (6) (2022) 063509, arXiv:2203.04167.

[2872] O. Akarsu, A. De Felice, E. Di Valentino, S. Kumar, R.C. Nunes, E. Ozulker, J.A. Vazquez, A. Yadav, ΛCDM cosmology from a type-II minimally modified gravity, 2024, arXiv:2402.07716.

[2873] D. Green, J. Meyers, Cosmological preference for a negative neutrino mass, Phys. Rev. D 111 (8) (2025) 083507, arXiv:2407.07878.

[2874] W. Elbers, C.S. Frenk, A. Jenkins, B. Li, S. Pascoli, Negative neutrino masses as a mirage of dark energy, Phys. Rev. D 111 (6) (2025) 063534, arXiv: 2407.10965.

[2875] S.-F. Ge, L. Tan, Identifying neutrino mass ordering with cosmic gravitational focusing, Phys. Rev. D 111 (8) (2025) 083539, arXiv:2409.11115.

[2876] J.D. Barrow, Sudden future singularities, Cl. Quant. Grav. 21 (2004) L79-L82, arXiv:gr-qc/0403084.

[2877] A. De Felice, A. Doll, S. Mukohyama, A theory of type-II minimally modified gravity, J. Cosmol. Astropart. Phys. 09 (2020) 034, arXiv:2004.12549.

[2878] A. De Felice, S. Mukohyama, M.C. Pookkillath, Addressing $H_0$ tension by means of VCDM, Phys. Lett. B 816 (2021) 136201, arXiv:2009.08718; Erratum; Phys. Lett. B 818 (2021) 136364.

[2879] J.A. Vazquez, S. Hee, M.P. Hobson, A.N. Lasenby, M. Ibison, M. Bridges, Observational constraints on conformal time symmetry, missing matter and double dark energy, J. Cosmol. Astropart. Phys. 07 (2018) 062, arXiv:1208. 2542.

[2880] BOSS Collaboration, T. Delubac, et al., Baryon acoustic oscillations in the $\Lambda$α forest of BOSS DR11 quasars, Astron. Astrophys. 574 (2015) A59, arXiv: 1404.1801.

[2881] V. Sahni, Y. Shtanov, Brane world models of dark energy, J. Cosmol. Astropart. Phys. 11 (2003) 014, arXiv:astro-ph/0202346.

[2882] S. Bag, V. Sahni, A. Shafieloo, Y. Shtanov, Phantom braneworld and the Hubble tension, Astrophys. J. 923 (2) (2021) 212, arXiv:2107.03271.

[2883] E. Di Valentino, E.V. Linder, A. Melchiorri, Vacuum phase transition solves the $H_0$ tension, Phys. Rev. D 97 (4) (2018) 043528, arXiv:1710.02153.

[2884] E. Mörtsell, S. Dhawan, Does the hubble constant tension call for new physics? J. Cosmol. Astropart. Phys. 09 (2018) 025, arXiv:1801.07260.

[2885] V. Poulin, K.K. Boddy, S. Bird, M. Kamionkowski, Implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions, Phys. Rev. D 97 (12) (2018) 123504, arXiv:1803.02474.

[2886] S. Capozziello, Ruchika, A.A. Sen, Model independent constraints on dark energy evolution from low-redshift observations, Mon. Not. R. Astron. Soc. 484 (2019) 4484, arXiv:1806.03943.

[2887] Ö. Akarsu, J.D. Barrow, C.V.R. Board, N.M. Uzun, J.A. Vazquez, Screening $\Lambda$ in a new modified gravity model, Eur. Phys. J. C 79 (10) (2019) 846, arXiv:1903.11519.

[2888] L. Visinelli, S. Vagnozzi, U. Danielsson, Revisiting a negative cosmological constant from low-redshift data, Symmetry 11 (8) (2019) 1035, arXiv:1907. 07953.

[2889] A. Perez, D. Sudarsky, E. Wilson-Ewing, Resolving the $H_0$ tension with diffusion, Gen. Relativity Gravitation 53 (1) (2021) 7, arXiv:2001.07536.

[2890] Ö. Akarsu, N. Katirci, S. Kumar, R.C. Nunes, B. Özürk, S. Sharma, Rastall gravity extension of the standard ΛCDM model: theoretical features and observational constraints, Eur. Phys. J. C 80 (11) (2020) 1050, arXiv:2004. 04074.

[2891] R. Calderón, R. Gannouji, B. L'Huillier, D. Polarski, Negative cosmological constant in the dark sector? Phys. Rev. D 103 (2) (2021) 023526, arXiv: 2008.10237.

[2892] G. Ye, Y.-S. Piao, $T_0$ censorship of early dark energy and AdS vacua, Phys. Rev. D 102 (8) (2020) 083523, arXiv:2008.10832.

[2893] A. Paliathanasis, G. Leon, Dynamics of a two scalar field cosmological model with phantom terms, Cl. Quant. Grav. 38 (7) (2021) 075013, arXiv:2009. 12874.

[2894] O. Akarsu, E.O. Colgain, E. Özulker, S. Thakur, L. Yin, Inevitable manifestation of wiggles in the expansion of the late universe, Phys. Rev. D 107 (12) (2023) 123526, arXiv:2207.10609.

[2895] S. Di Gennaro, Y.C. Ong, Sign switching dark energy from a running barrow entropy, Universe 8 (10) (2022) 541, arXiv:2205.09311.

[2896] Y.C. Ong, An effective sign switching dark energy: Lotka-Volterra model of two interacting fluids, Universe 9 (10) (2023) 437, arXiv:2212.04429.

[2897] B. Alexandre, S. Gielen, J. Magueijo, Overall signature of the metric and the cosmological constant, J. Cosmol. Astropart. Phys. 02 (2024) 036, arXiv: 2306.11502.

[2898] Y. Tiwari, B. Ghosh, R.K. Jain, Towards a possible solution to the Hubble tension with Horndeski gravity, Eur. Phys. J. C 84 (3) (2024) 220, arXiv: 2301.09382.

[2899] L.A. Anchordoqui, I. Antoniadis, D. Lust, Anti-de Sitter → de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters, Phys. Lett. B 855 (2024) 138775, arXiv:2312.12352.

[2900] L.A. Anchordoqui, I. Antoniadis, D. Bielli, A. Chatrabhuti, H. Isono, Thin-wall vacuum decay in the presence of a compact dimension meets the $H_0$ and $S_8$ tensions, 2024, arXiv:2410.18649.

[2901] H. Wang, Z.-Y. Peng, Y.-S. Piao, Can recent DESI BAO measurements accommodate a negative cosmological constant? Phys. Rev. D 111 (6) (2025) L061306, arXiv:2406.03395.

[2902] Y. Toda, W. Giarè, E. Özülker, E. Di Valentino, S. Vagnozzi, Combining pre- and post-recombination new physics to address cosmological tensions: Case study with varying electron mass and sign-switching cosmological constant, Phys. Dark Univ. 46 (2024) 101676, arXiv:2407.01173.

[2903] O. Akarsu, B. Bulduk, A. De Felice, N. Katirci, N.M. Uzun, Unexplored regions in teleparallel $f(T)$ gravity: Sign-changing dark energy density, 2024, arXiv: 2410.23068.

[2904] M.S. Souza, A.M. Barcelos, R.C. Nunes, Ö. Akarsu, S. Kumar, Mapping the ΛCDM scenario to $f(T)$ modified gravity: Effects on structure growth rate, Universe 11 (1) (2025) 2, arXiv:2501.18031.

[2905] P. Mukherjee, D. Kumar, A.A. Sen, Quintessential implications of the presence of AdS in the dark energy sector, 2025, arXiv:2501.18335.
[2906] U.K. Tyagi, S. Haridasu, S. Basak, Holographic and gravity-thermodynamic approaches in entropic cosmology: Bayesian assessment using late-time data, Phys. Rev. D 110 (6) (2024) 063503, arXiv:2406.07446.

[2907] M.T. Manoharan, Insights on Granda-Oliveros holographic dark energy: possibility of negative dark energy at $z \ge 2$, Eur. Phys. J. C 84 (5) (2024) 552.

[2908] A. Gómez-Valent, J. Solà Peracaula, Composite dark energy and the cosmological tensions, Phys. Lett. B 864 (2025) 139391, arXiv:2412.15124.

[2909] S. Dwivedi, M. Högås, 2D BAO vs. 3D BAO: Solving the Hubble tension with bimetric cosmology, Universe 10 (11) (2024) 406, arXiv:2407.04322.

[2910] R.E. Keeley, K.N. Abazajian, M. Kaplinghat, A. Shafieloo, The preference for evolving dark energy from cosmological distance measurements and possible signatures in the growth rate of perturbations, 2025, arXiv:2502.12667.

[2911] E. Di Valentino, A. Mukherjee, A.A. Sen, Dark energy with phantom crossing and the $H_0$ tension, Entropy 23 (4) (2021) 404, arXiv:2005.12587.

[2912] S. Kumar, R.C. Nunes, Echo of interactions in the dark sector, Phys. Rev. D 96 (10) (2017) 103511, arXiv:1702.02143.

[2913] E. Di Valentino, A. Melchiorri, O. Mena, Can interacting dark energy solve the $H_0$ tension? Phys. Rev. D 96 (4) (2017) 043503, arXiv:1704.08342.

[2914] W. Yang, A. Mukherjee, E. Di Valentino, S. Pan, Interacting dark energy with time varying equation of state and the $H_0$ tension, Phys. Rev. D 98 (12) (2018) 123527, arXiv:1809.06883.

[2915] S. Pan, W. Yang, E. Di Valentino, E.N. Saridakis, S. Chakraborty, Interacting scenarios with dynamical dark energy: Observational constraints and alleviation of the $H_0$ tension, Phys. Rev. D 100 (10) (2019) 103520, arXiv:1907.07540.

[2916] S. Kumar, R.C. Nunes, S.K. Yadav, Dark sector interaction: a remedy of the tensions between CMB and LSS data, Eur. Phys. J. C 79 (7) (2019) 576, arXiv:1903.04865.

[2917] E. Di Valentino, A. Melchiorri, O. Mena, S. Vagnozzi, Nonminimal dark sector physics and cosmological tensions, Phys. Rev. D 101 (6) (2020) 063502, arXiv:1910.09853.

[2918] E. Di Valentino, A. Melchiorri, O. Mena, S. Vagnozzi, Interacting dark energy in the early 2020s: A promising solution to the $H_0$ and cosmic shear tensions, Phys. Dark Univ. 30 (2020) 100666, arXiv:1908.04281.

[2919] M. Lucca, D.C. Hooper, Shedding light on dark matter-dark energy interactions, Phys. Rev. D 102 (12) (2020) 123502, arXiv:2002.06127.

[2920] S. Kumar, Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy, Phys. Dark Univ. 33 (2021) 100862, arXiv:2102.12902.

[2921] R.C. Nunes, S. Vagnozzi, S. Kumar, E. Di Valentino, O. Mena, New tests of dark sector interactions from the full-shape galaxy power spectrum, Phys. Rev. D 105 (12) (2022) 123506, arXiv:2203.08093.

[2922] M.A. Sabogal, E. Silva, R.C. Nunes, S. Kumar, E. Di Valentino, Sign switching in dark sector coupling interactions as a candidate for resolving cosmological tensions, Phys. Rev. D 111 (4) (2025) 043531, arXiv:2501.10323.

[2923] M. Montero, C. Vafa, I. Valenzuela, The dark dimension and the Swampland, JHEP 02 (2023) 022, arXiv:2205.12293.

[2924] L.A. Anchordoqui, I. Antoniadis, Large extra dimensions from higher-dimensional inflation, Phys. Rev. D 109 (10) (2024) 103508, arXiv:2310.20828.

[2925] N. Arkani-Hamed, S. Dubovsky, A. Nicolis, G. Villadoro, Quantum horizons of the standard model landscape, JHEP 06 (2007) 078, arXiv:hep-th/0703067.

[2926] J.F. Soriano, S. Wohlberg, L.A. Anchordoqui, New insights on a sign-switching $\Lambda$, Phys. Dark Univ. 48 (2025) 101911, arXiv:2502.19239.

[2927] A. Awad, W. El Hanafy, G.G.L. Nashed, E.N. Saridakis, Phase portraits of general f(T) cosmology, J. Cosmol. Astropart. Phys. 02 (2018) 052, arXiv:1710.10194.

[2928] M. Hashim, W. El Hanafy, A. Golovnev, A.A. El-Zant, Toward a concordance teleparallel cosmology. Part I. Background dynamics, J. Cosmol. Astropart. Phys. 07 (2021) 052, arXiv:2010.14964.

[2929] M. Hashim, A.A. El-Zant, W. El Hanafy, A. Golovnev, Toward a concordance teleparallel cosmology. Part II. Linear perturbation, J. Cosmol. Astropart. Phys. 07 (2021) 053, arXiv:2104.08311.

[2930] M. Cicoli, S. De Alwis, A. Maharana, F. Muia, F. Quevedo, De Sitter vs Quintessence in string theory, Fortsch. Phys. 67 (1-2) (2019) 1800079, arXiv:1808.08967.

[2931] Ruchika, S.A. Adil, K. Dutta, A. Mukherjee, A.A. Sen, Observational constraints on axion(s) dark energy with a cosmological constant, Phys. Dark Univ. 40 (2023) 101199, arXiv:2005.08813.

[2932] J. Grande, J. Solà, H. Stefancic, LXCDM: A cosmon model solution to the cosmological coincidence problem? J. Cosmol. Astropart. Phys. 08 (2006) 011, arXiv:gr-qc/0604057.

[2933] A.A. Sen, Deviation from LambdaCDM: Pressure parametrization, Phys. Rev. D 77 (2008) 043508, arXiv:0708.1072.

[2934] S. Kumar, A. Nautiyal, A.A. Sen, Deviation from ΛCDM with cosmic strings networks, Eur. Phys. J. C 73 (9) (2013) 2562, arXiv:1207.4024.

[2935] R.Y. Wen, L.T. Hergt, N. Afshordi, D. Scott, A cosmic glitch in gravity, J. Cosmol. Astropart. Phys. 03 (2024) 045, arXiv:2311.03028.

[2936] J.M. Maldacena, The Large N limit of superconformal field theories and supergravity, Adv. Theor. Math. Phys. 2 (1998) 231-252, arXiv:hep-th/9711200.

[2937] R. Bousso, J. Polchinski, Quantization of four form fluxes and dynamical neutralization of the cosmological constant, JHEP 06 (2000) 006, arXiv:hep-th/0004134.

[2938] M. Demirtas, M. Kim, L. McAllister, J. Moritz, A. Rios-Tascon, Exponentially small cosmological constant in string theory, Phys. Rev. Lett. 128 (1) (2022) 011602, arXiv:2107.09065.

[2939] A.A. Sen, S.A. Adil, S. Sen, Do cosmological observations allow a negative $\Lambda$? Mon. Not. R. Astron. Soc. 518 (1) (2022) 1098-1105, arXiv:2112.10641.

[2940] C.B.V. Dash, T.G. Sarkar, A.A. Sen, Post-reionization Hi 21-cm signal: a probe of negative cosmological constant, M Mon. Not. R. Astron. Soc. 527 (4) (2023) 11694-11706, arXiv:2309.01623.

[2941] C. Andrei, A. Iijas, P.J. Steinhardt, Rapidly descending dark energy and the end of cosmic expansion, Proc. Nat. Acad. Sci. 119 (15) (2022) e2200539119, arXiv:2201.07704.

[2942] S. Vagnozzi, Seven hints that early-time new physics alone is not sufficient to solve the hubble tension, Universe 9 (9) (2023) 393, arXiv:2308.16628.

[2943] Y.L. Bolotin, A. Kostenko, O.A. Lemets, D.A. Yerokhin, Cosmological evolution with interaction between dark energy and dark matter, Internat. J. Modern Phys. D 24 (03) (2014) 1530007, arXiv:1310.0085.

[2944] B. Wang, E. Abdalla, F. Atrio-Barandela, D. Pavón, Further understanding the interaction between dark energy and dark matter: current status and future directions, Rep. Prog. Phys. 87 (3) (2024) 036901, arXiv:2402.00819.

[2945] M.A. van der Westhuizen, A. Abebe, Interacting dark energy: clarifying the cosmological implications and viability conditions, J. Cosmol. Astropart. Phys. 01 (2024) 048, arXiv:2302.11949.

[2946] J.S. Alcaniz, J.A.S. Lima, Interpreting cosmological vacuum decay, Phys. Rev. D 72 (2005) 063516, arXiv:astro-ph/0507372.

[2947] D. Pavon, B. Wang, Le Chatelier-Braun principle in cosmological physics, Gen. Relativity Gravitation 41 (2009) 1-5, arXiv:0712.0565.

[2948] V. da Fonseca, T. Barreiro, N.J. Nunes, A simple parametrisation for coupled dark energy, Phys. Dark Univ. 35 (2023) 100940, arXiv:2104.14889.

[2949] M. Carrillo González, M. Trodden, Field theories and fluids for an interacting dark sector, Phys. Rev. D 97 (4) (2018) 043508, arXiv:1705.04737; Erratum-, Phys. Rev. D 101 (2020) 089901.

[2950] M. Zumalacarregui, T.S. Koivisto, D.F. Mota, P. Ruiz-Lapuente, Disformal scalar fields and the dark sector of the universe, J. Cosmol. Astropart. Phys. 05 (2010) 038, arXiv:1004.2684.

[2951] C. van de Bruck, J. Morrice, Disformal couplings and the dark sector of the universe, J. Cosmol. Astropart. Phys. 04 (2015) 036, arXiv:1501.03073.

[2952] E.M. Teixeira, A. Nunes, N.J. Nunes, Disformally coupled quintessence, Phys. Rev. D 101 (8) (2020) 083506, arXiv:1912.13348.

[2953] C. van de Bruck, E.M. Teixeira, Dark D-Brane Cosmology: from background evolution to cosmological perturbations, Phys. Rev. D 102 (10) (2020) 103503, arXiv:2007.15414.

[2954] C. Van De Bruck, J. Mifsud, Searching for dark matter - dark energy interactions: going beyond the conformal case, Phys. Rev. D 97 (2) (2018) 023506, arXiv:1709.04882.

[2955] J. Valiviita, E. Majerotto, R. Maartens, Instability in interacting dark energy and dark matter fluids, J. Cosmol. Astropart. Phys. 07 (2008) 020, arXiv:0804.0232.

[2956] M.B. Gavela, D. Hernandez, L. Lopez Honorez, O. Mena, S. Rigolin, Dark coupling, J. Cosmol. Astropart. Phys. 07 (2009) 034, arXiv:0901.1611; Erratum; JCAP 05 (2010) E01.

[2957] Y. Zhai, W. Giarbè, C. van de Bruck, E. Di Valentino, O. Mena, R.C. Nunes, A consistent view of interacting dark energy from multiple CMB probes, J. Cosmol. Astropart. Phys. 07 (2023) 032, arXiv:2303.08201.

[2958] W. Giarbè, Y. Zhai, S. Pan, E. Di Valentino, R.C. Nunes, C. van de Bruck, Tightening the reins on nonminimal dark sector physics: Interacting dark energy with dynamical and nondynamical equation of state, Phys. Rev. D 110 (6) (2024) 063527, arXiv:2404.02110.

[2959] A. Paliathanasis, S. Pan, W. Yang, Dynamics of nonlinear interacting dark energy models, Internat. J. Modern Phys. D 28 (12) (2019) 1950161, arXiv:1903.02370.

[2960] J. De-Santiago, I.E. Sánchez G., D. Tamayo, Non-linear coupling in the dark sector as a running vacuum model, Gen. Relativity Gravitation 50 (8) (2018) 101, arXiv:1612.02836.

[2961] F. Arevalo, A.P.R. Bacalhau, W. Zimdahl, Cosmological dynamics with non-linear interactions, Cl. Quant. Grav. 29 (2012) 235001, arXiv:1112.5095.

[2962] E. Ebrahimi, H. Golchin, A. Mehrabi, S.M.S. Movahed, Consistency of nonlinear interacting ghost dark energy with recent observations, Internat. J. Modern Phys. D 26 (11) (2017) 1750124, arXiv:1611.06551.

[2963] M. Khurshudyan, A. Khurshudyan, On cosmology of interacting varying polytropic dark fluids, Modern Phys. Lett. A 34 (17) (2019) 1950133, arXiv:1707.04116.

[2964] G. Cheng, Y.-Z. Ma, F. Wu, J. Zhang, X. Chen, Testing interacting dark matter and dark energy model with cosmological data, Phys. Rev. D 102 (4) (2020) 043517, arXiv:1911.04520.
[2965] W. Yang, S. Pan, A. Paliathanasis, Cosmological constraints on an exponential interaction in the dark sector, Mon. Not. R. Astron. Soc. 482 (1) (2019) 1007–1016, arXiv:1804.08558.

[2966] M. Khurshudyan, A. Khurshudyan, Some interacting dark energy models, Symmetry 10 (11) (2018) 577, arXiv:1708.02293.

[2967] S. Pan, W. Yang, A. Paliathanasis, Non-linear interacting cosmological models after Planck 2018 legacy release and the $H_0$ tension, Mon. Not. R. Astron. Soc. 493 (3) (2020) 3114–3131, arXiv:2002.03408.

[2968] Z. Haba, A. Stachowski, M. Szydłowski, Dynamics of the diffusive DM-DE interaction – dynamical system approach, J. Cosmol. Astropart. Phys. 07 (2016) 024, arXiv:1603.07620.

[2969] G. Koutsoumbas, K. Ntrekis, E. Papantonopoulos, E.N. Saridakis, Unification of dark matter - dark energy in generalized Galilean theories, J. Cosmol. Astropart. Phys. 02 (2018) 003, arXiv:1704.08640.

[2970] S. Calogero, H. Velten, Cosmology with matter diffusion, J. Cosmol. Astropart. Phys. 11 (2013) 025, arXiv:1308.3393.

[2971] E.F. Piratova Moreno, L.Á. García, Late accelerated expansion of the universe in diffusive scenarios, Rev. Mex. Astron. Astrofis. 59 (2) (2023) 389–399.

[2972] T. Josset, A. Perez, D. Sudarsky, Dark energy from violation of energy conservation, Phys. Rev. Lett. 118 (2) (2017) 021102, arXiv:1604.04183.

[2973] A. Perez, D. Sudarsky, Dark energy from quantum gravity discreteness, Phys. Rev. Lett. 122 (22) (2019) 221302, arXiv:1711.05183.

[2974] A. Perez, D. Sudarsky, Black holes, Planckian granularity, and the changing cosmological ‘constant’, Gen. Relativity Gravitation 53 (4) (2021) 40, arXiv:1911.06059.

[2975] C. Corral, N. Cruz, E. González, Diffusion in unimodular gravity: Analytical solutions, late-time acceleration, and cosmological constraints, Phys. Rev. D 102 (2) (2020) 023508, arXiv:2005.06052.

[2976] F.X. Linares Cedeño, U. Nucamendi, Revisiting cosmological diffusion models in unimodular gravity and the $H_0$ tension, Phys. Dark Univ. 32 (2021) 100807, arXiv:2009.10268.

[2977] S.J. Landau, M. Benetti, A. Perez, D. Sudarsky, Cosmological constraints on unimodular gravity models with diffusion, Phys. Rev. D 108 (4) (2023) 043524, arXiv:2211.07424.

[2978] D. Wands, J. De-Santiago, Y. Wang, Inhomogeneous vacuum energy, Cl. Quant. Grav. 29 (2012) 145017, arXiv:1203.6776.

[2979] M. Sebastianutti, N.B. Hogg, M. Bruni, The interacting vacuum and tensions: A comparison of theoretical models, Phys. Dark Univ. 46 (2024) 101546, arXiv:2312.14123.

[2980] S. Weinberg, The cosmological constant problem, in: J.-P. Hsu, D. Fine (Eds.), Rev. Modern Phys. 61 (1989) 1–23.

[2981] G.F.R. Ellis, H. van Elst, J. Murugan, J.-P. Uzan, On the trace-free Einstein equations as a viable alternative to general relativity, Cl. Quant. Grav. 28 (2011) 225007, arXiv:1008.1196.

[2982] M. de Cesare, E. Wilson-Ewing, Interacting dark sector from the trace-free Einstein equations: Cosmological perturbations with no instability, Phys. Rev. D 106 (2) (2022) 023527, arXiv:2112.12701.

[2983] A. Shafieloo, D.K. Hazra, V. Sahni, A.A. Starobinsky, Metastable dark energy with radioactive-like decay, Mon. Not. R. Astron. Soc. 473 (2) (2018) 2760–2770, arXiv:1610.05192.

[2984] J.S.T. de Souza, G. S. Vicente, L.L. Graef, Constraints on metastable dark energy decaying into dark matter, Universe 10 (9) (2024) 371, arXiv:2403.04970.

[2985] X. Li, A. Shafieloo, V. Sahni, A.A. Starobinsky, Revisiting metastable dark energy and tensions in the estimation of cosmological parameters, Astrophys. J. 887 (1999) 153, arXiv:1904.03790.

[2986] W. Yang, E. Di Valentino, S. Pan, S. Basilakos, A. Paliathanasis, Metastable dark energy models in light of Planck 2018 data: Alleviating the $H_0$ tension, Phys. Rev. D 102 (6) (2020) 063503, arXiv:2001.04307.

[2987] K. Urbanowski, Cosmological “constant” in a universe born in the metastable false vacuum state, Eur. Phys. J. C 82 (3) (2022) 242, arXiv:2110.11957.

[2988] K. Urbanowski, A universe born in a metastable false vacuum state needs not die, Eur. Phys. J. C 83 (1) (2023) 55, arXiv:2207.10965.

[2989] E. Abdalla, L.L. Graef, B. Wang, A model for dark energy decay, Phys. Lett. B 726 (2013) 786–790, arXiv:1202.0499.

[2990] R.G. Landim, E. Abdalla, Metastable dark energy, Phys. Lett. B 764 (2017) 271–276, arXiv:1611.00428.

[2991] R.G. Landim, R.J.F. Marcondes, F.F. Bernardi, E. Abdalla, Interacting dark energy in the dark $SU(2)_R$ model, Braz. J. Phys. 48 (4) (2018) 364–369, arXiv:1711.07282.

[2992] D. Stojkovic, G.D. Starkman, R. Matsuo, Dark energy, the colored anti-de Sitter vacuum, and LHC phenomenology, Phys. Rev. D 77 (2008) 063006, arXiv:hep-ph/0703246.

[2993] E. Greenwood, E. Halstead, R. Poltis, D. Stojkovic, Dark energy, the electroweak vacua and collider phenomenology, Phys. Rev. D 79 (2009) 103003, arXiv:0810.5343.

[2994] F. Simpson, Scattering of dark matter and dark energy, Phys. Rev. D 82 (2010) 083505, arXiv:1007.1034.

[2995] A. Pourtsidou, C. Skordis, E.J. Copeland, Models of dark matter coupled to dark energy, Phys. Rev. D 88 (8) (2013) 083505, arXiv:1307.0458.

[2996] M. Asghari, J. Beltrán Jiménez, S. Khosravi, D.F. Mota, On structure formation from a small-scales-interacting dark sector, J. Cosmol. Astropart. Phys. 04 (2019) 042, arXiv:1902.05532.

[2997] D. Figueruelo, et al., J-PAS: Forecasts for dark matter - dark energy elastic couplings, J. Cosmol. Astropart. Phys. 07 (2021) 022, arXiv:2103.01571.

[2998] J. Beltrán Jiménez, D. Bettoni, D. Figueruelo, F.A. Teppa Pannia, S. Tsujikawa, Probing elastic interactions in the dark sector and the role of S8, Phys. Rev. D 104 (10) (2021) 103503, arXiv:2106.11222.

[2999] V. Poulin, J.L. Bernal, E.D. Kovetz, M. Kamionkowski, Sigma-8 tension is a drag, Phys. Rev. D 107 (12) (2023) 123538, arXiv:2209.06217.

[3000] J.B. Jiménez, D. Bettoni, D. Figueruelo, F.A. Teppa Pannia, On evidence for elastic interactions in the dark sector, Phys. Dark Univ. 47 (2025) 101761, arXiv:2410.18645.

[3001] J. Beltrán Jiménez, E. Di Dio, D. Figueruelo, A smoking gun from the power spectrum dipole for elastic interactions in the dark sector, J. Cosmol. Astropart. Phys. 11 (2023) 088, arXiv:2212.08617 [astro-ph.CO].

[3002] J. Beltrán Jiménez, D. Figueruelo, F.A. Teppa Pannia, Nondegeneracy of massive neutrinos and elastic interactions in the dark sector, Phys. Rev. D 110 (2) (2024) 023527, arXiv:2403.03216 [astro-ph.CO].

[3003] M. Baldi, F. Simpson, Structure formation simulations with momentum exchange: alleviating tensions between high-redshift and low-redshift cosmological probes, Mon. Not. R. Astron. Soc. 465 (1) (2017) 653–666, arXiv:1605.05623 [astro-ph.CO].

[3004] A. Pourtsidou, T. Tram, Reconciling CMB and structure growth measurements with dark energy interactions, Phys. Rev. D 94 (4) (2016) 043518, arXiv:1604.04222 [astro-ph.CO].

[3005] P. Agrawal, G. Obied, P.J. Steinhardt, C. Vafa, On the cosmological implications of the String Swampland, Phys. Lett. B 784 (2018) 271–276, arXiv:1806.09718 [hep-th].

[3006] W.H. Kinney, S. Vagnozzi, L. Visinelli, The zoo plot meets the swampland: mutual (in)consistency of single-field inflation, string conjectures, and cosmological data, Cl. Quant. Grav. 36 (11) (2019) 117001, arXiv:1808.06424 [astro-ph.CO].

[3007] P. Agrawal, G. Obied, C. Vafa, $H_0$ tension, swampland conjectures, and the epoch of fading dark matter, Phys. Rev. D 103 (4) (2021) 043523, arXiv:1906.08261 [astro-ph.CO].

[3008] A. Salam, E. Sezgin, Chiral compactification on Minkowski $\times S^{*2}$ of $N=2$ Einstein–Maxwell supergravity in six-dimensions, Phys. Lett. B 147 (1984) 47.

[3009] M. Cvetic, G.W. Gibbons, C.N. Pope, A string and M theory origin for the Salam–Sezgin model, Nuclear Phys. B 677 (2004) 164–180, arXiv:hep-th/0308026.

[3010] L.A. Anchordoqui, I. Antoniadis, D. Lüst, J.F. Soriano, T.R. Taylor, $H_0$ tension and the String Swampland, Phys. Rev. D 101 (2020) 083532, arXiv:1912.00242 [hep-th].

[3011] L.A. Anchordoqui, I. Antoniadis, D. Lüst, J.F. Soriano, Dark energy, Ricci-nonflat spaces, and the Swampland, Phys. Lett. B 816 (2021) 136199, arXiv:2005.10075 [hep-th].

[3012] D. Benisty, S. Pan, D. Staicova, E. Di Valentino, R.C. Nunes, Late-time constraints on interacting dark energy: Analysis independent of $H_0$, rd, and MB, Astron. Astrophys. 688 (2024) A156, arXiv:2403.00056 [astro-ph.CO].

[3013] G.A. Hoerning, R.G. Landim, L.O. Ponte, R.P. Rolim, F.B. Abdalla, E. Abdalla, Constraints on interacting dark energy revisited: implications for the hubble tension, 2023, arXiv:2308.05807 [astro-ph.CO].

[3014] S. Pan, W. Yang, On the interacting dark energy scenarios – the case for Hubble constant tension, 2023, arXiv:2310.07260 [astro-ph.CO].

[3015] W. Yang, S. Pan, E. Di Valentino, R.C. Nunes, S. Vagnozzi, D.F. Mota, Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension, J. Cosmol. Astropart. Phys. 09 (2018) 019, arXiv:1805.08252 [astro-ph.CO].

[3016] A. Bhattacharyya, U. Alam, K.L. Pandey, S. Das, S. Pal, Are $H_0$ and $\sigma_8$ tensions generic to present cosmological data? Astrophys. J. 876 (2) (1999) 143, arXiv:1805.04716 [astro-ph.CO].

[3017] E. Di Valentino, R.Z. Ferreira, L. Visinelli, U. Danielsson, Late time transitions in the quintessence field and the $H_0$ tension, Phys. Dark Univ. 26 (2019) 100385, arXiv:1906.11255 [astro-ph.CO].

[3018] Y.-H. Yao, X.-H. Meng, Can interacting dark energy with dynamical coupling resolve the Hubble tension, 2022, arXiv:2207.05955 [astro-ph.CO].

[3019] S. Gariazzo, E. Di Valentino, O. Mena, R.C. Nunes, Late-time interacting cosmologies and the Hubble constant tension, Phys. Rev. D 106 (2) (2022) 023530, arXiv:2111.03152 [astro-ph.CO].

[3020] R.-Y. Guo, L. Feng, T.-Y. Yao, X.-Y. Chen, Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension, J. Cosmol. Astropart. Phys. 12 (12) (2021) 036, arXiv:2110.02536 [gr-qc].

[3021] R.C. Nunes, E. Di Valentino, Dark sector interaction and the supernova absolute magnitude tension, Phys. Rev. D 104 (6) (2021) 063529, arXiv:2107.09151 [astro-ph.CO].

[3022] Y. Zhao, Y. Liu, S. Liao, J. Zhang, X. Liu, W. Du, Constraining interacting dark energy models with the halo concentration–mass relation, Mon. Not. R. Astron. Soc. 523 (4) (2023) 5962–5971, arXiv:2212.02050 [astro-ph.CO].
[3023] L.-Y. Gao, Z.-W. Zhao, S.-S. Xue, X. Zhang, Relieving the H 0 tension with a new interacting dark energy model, J. Cosmol. Astropart. Phys. 07 (2021) 005, arXiv:2101.10714 [astro-ph.CO].

[3024] H. Amirhashchi, A.K. Yadav, N. Ahmad, V. Yadav, Interacting dark sectors in anisotropic universe: Observational constraints and H0 tension, Phys. Dark Univ. 36 (2022) 101043, arXiv:2001.03775 [astro-ph.CO].

[3025] S. Pan, W. Yang, C. Singha, E.N. Saridakis, Observational constraints on sign-
changeable interaction models and alleviation of the H₀ tension, Phys. Rev.
D 100 (8) (2019) 083539, arXiv:1903.10969 [astro-ph.CO].

[3026] L.-Y. Gao, S.-S. Xue, X. Zhang, Dark energy and matter interacting scenario to relieve H₀ and S₈ tensions*, Chin. Phys. C 48 (5) (2024) 051001, arXiv:2212.13146 [astro-ph.CO].

[3027] W. Yang, S. Pan, E. Di Valentino, O. Mena, A. Melchiorri, 2021-H0
odyssey: closed, phantom and interacting dark energy cosmologies, J. Cosmol.
Astropart. Phys. 10 (2021) 008, arXiv:2101.03129 [astro-ph.CO].

[3028] W. Yang, S. Pan, R.C. Nunes, D.F. Mota, Dark calling Dark: Interaction in the dark sector in presence of neutrino properties after Planck CMB final release, J. Cosmol. Astropart. Phys. 04 (2020) 008, arXiv:1910.08821 [astro-ph.CO].

[3029] M. Lucca, Dark energy–dark matter interactions as a solution to the S8 tension, Phys. Dark Univ. 34 (2021) 100899, arXiv:2105.09249 [astro-ph.CO].

[3030] R. An, C. Feng, B. Wang, Relieving the tension between weak lensing and cosmic microwave background with interacting dark matter and dark energy models, J. Cosmol. Astropart. Phys. 02 (2018) 038, arXiv:1711.06799 [astro-ph.CO].

[3031] S. Sinha, N. Banerjee, Density perturbation in an interacting holographic dark energy model, Eur. Phys. J. Plus 135 (10) (2020) 779, arXiv:1911.06520 [gr-qc].

[3032] S. Sinha, Differentiating dark interactions with perturbation, Phys. Rev. D 103 (12) (2021) 123547, arXiv:2101.08959 [astro-ph.CO].

[3033] S. Sinha, M. Banerjee, S. Das, Perturbation in an interacting dark universe, Phys. Dark Univ. 42 (2023) 101273, arXiv:2204.05174 [gr-qc].

[3034] B.J. Barros, D. Castelão, V. da Fonseca, T. Barreiro, N.J. Nunes, I. Tereno, Is there evidence for CIDER in the Universe? J. Cosmol. Astropart. Phys. 01 (2023) 013, arXiv:2209.04468 [astro-ph.CO].

[3035] O. Trivedi, Recent advances in cosmological singularities, Symmetry 16 (3) (2024) 298, arXiv:2309.08954 [gr-qc].

[3036] J. de Haro, S. Nojiri, S.D. Odintsov, V.K. Oikonomou, S. Pan, Finite-time cosmological singularities and the possible fate of the universe, Phys. Rep. 1034 (2023) 1–114, arXiv:2309.07465 [gr-qc].

[3037] S. Nojiri, S.D. Odintsov, S. Tsujikawa, Properties of singularities in (phantom) dark energy universe, Phys. Rev. D 71 (2005) 063004, arXiv:hep-th/0501025.

[3038] S. Nojiri, S.D. Odintsov, V.K. Oikonomou, Modified gravity theories on a Nutshell: Inflation, bounce and late-time evolution, Phys. Rep. 692 (2017) 1–104, arXiv:1705.11098 [gr-qc].

[3039] S. Nojiri, S.D. Odintsov, Inhomogeneous equation of state of the universe: Phantom era, future singularity and crossing the phantom barrier, Phys. Rev. D 72 (2005) 023003, arXiv:hep-th/0505215.

[3040] K. Bamba, S. Nojiri, S.D. Odintsov, The Universe future in modified gravity theories: Approaching the finite-time future singularity, J. Cosmol. Astropart. Phys. 10 (2008) 045, arXiv:0807.2575 [hep-th].

[3041] S. Nojiri, S.D. Odintsov, Quantum escape of sudden future singularity, Phys. Lett. B 595 (2004) 1–8, arXiv:hep-th/0405078.

[3042] S. Castello, N. Grimm, C. Bonvin, Rescuing constraints on modified gravity using gravitational redshift in large-scale structure, Phys. Rev. D 106 (8) (2022) 083511, arXiv:2204.11507 [astro-ph.CO].

[3043] S. Castello, M. Mancarella, N. Grimm, D. Sobral-Blanco, I. Tutusaus, C. Bonvin, Gravitational redshift constraints on the effective theory of interacting dark energy, J. Cosmol. Astropart. Phys. 05 (2024) 003, arXiv:2311.14425 [astro-ph.CO].

[3044] C. Bonvin, L.E. Pogosian, Can cosmology distinguish a dark force from a modification of gravity? Nat. Astron. 7 (9) (2023) 1023–1024.

[3045] S. Castello, Z. Wang, L. Dam, C. Bonvin, L. Pogosian, Disentangling modified gravity from a dark force with gravitational redshift, Phys. Rev. D 110 (2024) 103523, arXiv:2404.09379 [astro-ph.CO].

[3046] D. Sobral-Blanco, C. Bonvin, Measuring anisotropic stress with relativistic effects, Phys. Rev. D 104 (6) (2021) 063516, arXiv:2102.05086 [astro-ph.CO].

[3047] D. Sobral-Blanco, C. Bonvin, Measuring the distortion of time with relativistic effects in large-scale structure, Mon. Not. R. Astron. Soc. 519 (1) (2022) L39–L44, arXiv:2205.02567 [astro-ph.CO].

[3048] Y.-H. Li, J.-F. Zhang, X. Zhang, Testing models of vacuum energy interacting with cold dark matter, Phys. Rev. D 93 (2) (2016) 023002, arXiv:1506.06349 [astro-ph.CO].

[3049] L. Feng, H.-L. Li, J.-F. Zhang, X. Zhang, Exploring neutrino mass and mass hierarchy in interacting dark energy models, Sci. China Phys. Mech. Astron. 63 (2) (2020) 220401, arXiv:1903.08848 [astro-ph.CO].

[3050] Y.-H. Li, X. Zhang, Large-scale stable interacting dark energy model: cosmological perturbations and observational constraints, Phys. Rev. D 89 (8) (2014) 083009, arXiv:1312.6328 [astro-ph.CO].

[3051] L. Feng, X. Zhang, Revisit of the interacting holographic dark energy model after Planck 2015, J. Cosmol. Astropart. Phys. 08 (2016) 072, arXiv:1607.05567 [astro-ph.CO].

[3052] M.-M. Zhao, D.-Z. He, J.-F. Zhang, X. Zhang, Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant, Phys. Rev. D 96 (4) (2017) 043520, arXiv:1703.08456 [astro-ph.CO].

[3053] Y.-H. Li, J.-F. Zhang, X. Zhang, Exploring the full parameter space for an interacting dark energy model with recent observations including redshift-space distortions: Application of the parametrized post-Friedmann approach, Phys. Rev. D 90 (12) (2014) 123007, arXiv:1409.7205 [astro-ph.CO].

[3054] Y.-H. Li, J.-F. Zhang, X. Zhang, Parametrized post-Friedmann framework for interacting dark energy, Phys. Rev. D 90 (6) (2014) 063005, arXiv:1404.5220 [astro-ph.CO].

[3055] R.-Y. Guo, Y.-H. Li, J.-F. Zhang, X. Zhang, Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach, J. Cosmol. Astropart. Phys. 05 (2017) 040, arXiv:1702.04189 [astro-ph.CO].

[3056] X. Zhang, Probing the interaction between dark energy and dark matter with the parametrized post-Friedmann approach, Sci. China Phys. Mech. Astron. 60 (5) (2017) 050431, arXiv:1702.04564 [astro-ph.CO].

[3057] L. Feng, Y.-H. Li, F. Yu, J.-F. Zhang, X. Zhang, Exploring interacting holographic dark energy in a perturbed universe with parameterized post-Friedmann approach, Eur. Phys. J. C 78 (10) (2018) 865, arXiv:1807.03022 [astro-ph.CO].

[3058] Y.-H. Li, X. Zhang, IDECAM: an implementation of interacting dark energy cosmology in CAMB, J. Cosmol. Astropart. Phys. 09 (2023) 046, arXiv:2306.01593 [astro-ph.CO].

[3059] J.-J. Guo, J.-F. Zhang, Y.-H. Li, D.-Z. He, X. Zhang, Probing the sign-
changeable interaction between dark energy and dark matter with current
observations, Sci. China Phys. Mech. Astron. 61 (3) (2018) 030011, arXiv:
1710.03068 [astro-ph.CO].

[3060] H.-L. Li, J.-F. Zhang, L. Feng, X. Zhang, Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter, Eur. Phys. J. C 77 (12) (2017) 907, arXiv:1711.06159 [astro-ph.CO].

[3061] L. Feng, D.-Z. He, H.-L. Li, J.-F. Zhang, X. Zhang, Constraints on active and sterile neutrinos in an interacting dark energy cosmology, Sci. China Phys. Mech. Astron. 63 (9) (2020) 290404, arXiv:1910.03872 [astro-ph.CO].

[3062] M. Zhang, B. Wang, P.-J. Wu, J.-Z. Qi, Y. Xu, J.-F. Zhang, X. Zhang, Prospects for constraining interacting dark energy models with 21 cm intensity mapping experiments, Astrophys. J. 918 (2) (2021) 56, arXiv:2102.03979 [astro-ph.CO].

[3063] T.-N. Li, P.-J. Wu, G.-H. Du, S.-J. Jin, H.-L. Li, J.-F. Zhang, X. Zhang, Constraints on interacting dark energy models from the desi baryon acoustic oscillation and des supernovae data, Astrophys. J. 976 (1) (2024) 1, arXiv: 2407.14934 [astro-ph.CO].

[3064] J. Gleyzes, D. Langlois, M. Mancarella, F. Vernizzi, Effective theory of interacting dark energy, J. Cosmol. Astropart. Phys. 08 (2015) 054, arXiv:1504.05481 [astro-ph.CO].

[3065] J. Gleyzes, D. Langlois, M. Mancarella, F. Vernizzi, Effective theory of dark energy at redshift survey scales, J. Cosmol. Astropart. Phys. 02 (2016) 056, arXiv:1509.02191 [astro-ph.CO].

[3066] C.M. Will, The confrontation between general relativity and experiment, Living Rev. Rel. 17 (2014) 4, arXiv:1403.7377 [gr-qc].

[3067] A. Addazi, et al., Quantum gravity phenomenology at the dawn of the multi-
messenger era—A review, Prog. Part. Nucl. Phys. 125 (2022) 103948, arXiv:
2111.05659 [hep-ph].

[3068] R. Alves Batista, et al., White paper and roadmap for quantum gravity phenomenology in the multi-messenger era, Cl. Quant. Grav. 42 (3) (2025) 032001, arXiv:2312.00409 [gr-qc].

[3069] M.H. Goroff, A. Sagnotti, The ultraviolet behavior of einstein gravity, Nuclear Phys. B 266 (1986) 709–736.

[3070] L. Barack, et al., Black holes, gravitational waves and fundamental physics: a roadmap, Cl. Quant. Grav. 36 (14) (2019) 143001, arXiv:1806.05195 [gr-qc].

[3071] S.M. Carroll, The cosmological constant, Living Rev. Rel. 4 (2001) 1, arXiv:astro-ph/0004075.

[3072] Supernova Search Team Collaboration, A.G. Riess, et al., Observational evidence from supernovae for an accelerating universe and a cosmological constant, Astron. J. 116 (1998) 1009–1038, arXiv:astro-ph/9805201.

[3073] Supernova Cosmology Project Collaboration, S. Perlmutter, et al., Measurements of Ω and Λ from 42 high redshift supernovae, Astrophys. J. 517 (1999) 565–586, arXiv:astro-ph/9812133.

[3074] M. Davis, G. Efstathiou, C.S. Frenk, S.D.M. White, The evolution of large scale structure in a universe dominated by cold dark matter, Astrophys. J. 292 (1985) 371–394.

[3075] G. Bertone, D. Hooper, History of dark matter, Rev. Modern Phys. 90 (4) (2018) 045002, arXiv:1605.04909 [astro-ph.CO].

[3076] E. Aprile, T. Doke, Liquid xenon detectors for particle physics and astrophysics, Rev. Modern Phys. 82 (2010) 2053–2097, arXiv:0910.4956 [physics.ins-det].

[3077] M. Misiaszek, N. Rossi, Direct detection of dark matter: A critical review, Symmetry 16 (2) (2024) 201, arXiv:2310.20472 [hep-ph].

[3078] F. Bajardi, S. Capozziello, Noether Symmetries in Theories of Gravity, in: Cambridge Monographs on Mathematical Physics, Cambridge University Press, 2022.