LiteBIRD Science Goals and Forecasts. A Case Study of the Origin of Primordial Gravitational Waves using Large-Scale CMB Polarization
Creators: name: Campeti, P.
name: Komatsu, E.
name: Baccigalupi, C.
name: Ballardini, M.
name: Bartolo, N.
name: Carones, A.
name: Errard, J.
name: Finelli, F.
name: Flauger, R.
name: Galli, S.
name: Galloni, G.
name: Giardiello, S.
name: Hazumi, M.
name: Henrot-Versillé, S.
name: Hergt, L. T.
name: Kohri, K.
name: Leloup, C.
name: Lesgourgues, J.
name: Macias-Perez, J.
name: Martínez-González, E.
name: Matarrese, S.
name: Matsumura, T.
name: Montier, L.
name: Namikawa, T.
name: Paoletti, D.
name: Poletti, D.
name: Remazeilles, M.
name: Shiraishi, M.
name: van Tent, B.
name: Tristram, M.
name: Vacher, L.
name: Vittorio, N.
name: Weymann-Despres, G.
name: Anand, A.
name: Aumont, J.
name: Aurlien, R.
name: Banday, A. J.
name: Barreiro, R. B.
name: Basyrov, A.
name: Bersanelli, M.
name: Blinov, D.
name: Bortolami, M.
name: Brinckmann, T.
name: Calabrese, E.
name: Carralot, F.
name: Casas, F. J.
name: Clermont, L.
name: Columbro, F.
name: Conenna, G.
name: Coppolecchia, A.
name: Cuttaia, F.
name: D'Alessandro, G.
name: de Bernardis, P.
name: De Petris, M.
name: Della Torre, S.
name: Di Giorgi, E.
name: Diego-Palazuelos, P.
name: Eriksen, H. K.
name: Franceschet, C.
name: Fuskeland, U.
name: Galloway, M.
name: Georges, M.
name: Gerbino, M.
name: Gervasi, M.
name: Ghigna, T.
name: Gimeno-Amo, C.
name: Gjerløw, E.
name: Gruppuso, A.
name: Gudmundsson, J.
name: Krachmalnicoff, N.
name: Lamagna, L.
name: Lattanzi, M.
name: Lembo, M.
name: Lonappan, A. I.
name: Masi, S.
name: Massa, M.
name: Micheli, S.
name: Moggi, A.
name: Monelli, M.
name: Morgante, G.
name: Mot, B.
name: Mousset, L.
name: Nagata, R.
name: Natoli, P.
name: Novelli, A.
name: Obata, I.
name: Pagano, L.
name: Paiella, A.
name: Pavlidou, V.
name: Piacentini, F.
name: Pinchera, M.
name: Pisano, G.
name: Puglisi, G.
name: Raffuzzi, N.
name: Ritacco, A.
name: Rizzieri, A.
name: Ruiz-Granda, M.
name: Savini, G.
name: Scott, D.
name: Signorelli, G.
name: Stever, S. L.
name: Stutzer, N.
name: Sullivan, R. M.
name: Tartari, A.
name: Tassis, K.
name: Terenzi, L.
name: Thompson, K. L.
name: Vielva, P.
name: Wehus, I. K.
name: Zhou, Y.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: We study the possibility of using the $LiteBIRD$ satellite $B$-mode survey to constrain models of inflation producing specific features in CMB angular power spectra. We explore a particular model example, i.e. spectator axion-SU(2) gauge field inflation. This model can source parity-violating gravitational waves from the amplification of gauge field fluctuations driven by a pseudoscalar "axionlike" field, rolling for a few e-folds during inflation. The sourced gravitational waves can exceed the vacuum contribution at reionization bump scales by about an order of magnitude and can be comparable to the vacuum contribution at recombination bump scales. We argue that a satellite mission with full sky coverage and access to the reionization bump scales is necessary to understand the origin of the primordial gravitational wave signal and distinguish among two production mechanisms: quantum vacuum fluctuations of spacetime and matter sources during inflation. We present the expected constraints on model parameters from $LiteBIRD$ satellite simulations, which complement and expand previous studies in the literature. We find that $LiteBIRD$ will be able to exclude with high significance standard single-field slow-roll models, such as the Starobinsky model, if the true model is the axion-SU(2) model with a feature at CMB scales. We further investigate the possibility of using the parity-violating signature of the model, such as the $TB$ and $EB$ angular power spectra, to disentangle it from the standard single-field slow-roll scenario. We find that most of the discriminating power of $LiteBIRD$ will reside in $BB$ angular power spectra rather than in $TB$ and $EB$ correlations.
description: 22 pages, 13 figures. Published in JCAP 06 (2024) 008. Added comments at end of Sec. 6 reframing conclusions in more general way. Updated references