cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Reduction of General One-loop Integrals Using Auxiliary Vector
Creators: name: Feng, Bo
name: Li, Tingfei
name: Wang, Hongbin
name: Zhang, Yaobo
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: As a key method to deal with loop integrals, Integration-By-Parts (IBP) method can be used to do reduction as well as establish the differential equations for master integrals. However, when talking about tensor reduction, the Passarino-Veltman (PV) reduction method is also widely used for one-loop integrals. Recently, we have proposed an improved PV reduction method, i.e., the PV reduction method with auxiliary vector $R$, which can easily give analytical reduction results for any tensor rank. However, our results are only for integrals with propagators with power one. In this paper, we generalize our method to one-loop integrals with general tensor structures and propagators with general powers. Our ideas are simple. We solve the generalised reduction problem by combining differentiation over masses and proper limit of reduction with power-one propagators. Finally, we demonstrate our method with several examples. With the result in this paper, we have shown that our improved PV-reduction method with auxiliary vector is a self-completed reduction method for one-loop integrals.
description: 24 pages,no figures
z~2-9 Galaxies magnified by the Hubble Frontier Field Clusters I: Source Selection and Surface Density-Magnification Constraints from >2500 galaxies
Creators: name: Bouwens, R. J.
name: Illingworth, G.
name: Ellis, R. S.
name: Oesch, P.
name: Paulino-Afonso, A.
name: Ribeiro, B.
name: Stefanon, M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We assemble a large comprehensive sample of 2534 z~2, 3, 4, 5, 6, 7, 8, and 9 galaxies lensed by the six clusters from the Hubble Frontier Fields (HFF) program. Making use of the availability of multiple independent magnification models for each of the HFF clusters and alternatively treating one of the models as the "truth," we show that the median magnification factors from the v4 parametric models are typically reliable to values of 30 to 50, and in one case to 100. Using the median magnification factor from the latest v4 models, we estimate the UV luminosities of the 2534 lensed z~2-9 galaxies, finding sources as faint as -12.4 mag at z~3 and -12.9 mag at z~7. We explicitly demonstrate the power of the surface density-magnification relations Sigma(z) vs. mu in the HFF clusters to constrain both distant galaxy properties and cluster lensing properties. Based on the Sigma(z) vs. mu relations, we show that the median magnification estimates from existing public models must be reliable predictors of the true magnification mu to mu<15 (95% confidence). We also use the observed Sigma(z) vs. mu relations to derive constraints on the evolution of the luminosity function faint-end slope from z~7 to z~2, showing that faint-end slope results can be consistent with blank-field studies if, and only if, the selection efficiency shows no strong dependence on the magnification factor mu. This can only be the case if very low luminosity galaxies are very small, being unresolved in deep lensing probes.
description: 22 pages, 13 figures, 6 tables, accepted for publication in the Astrophysical Journal, updated to be consistent with the proofs
Monte Carlo Calculations of the Extraction of Scintillation Light from Cryogenic N-type GaAs
Creators: name: Derenzo, Stephen
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: The high scintillation luminosity of n-type GaAs at 10K is surprising because (1) with a refractive index of about 3.5, escape is inhibited by total internal reflection and (2) narrow-beam experiments at 90K report infrared absorption coefficients of several per cm. This paper presents Monte Carlo calculations showing that the high luminosity at 10K can be explained if (1) narrow-beam absorption is almost all optical scattering and (2) the absolute absorption coefficient is below 0.1 per cm. Sixteen surface reflector configurations are simulated for a range of internal scattering and absolute absorption coefficients, and these can guide the design of cryogenic scintillating GaAs targets for the direct detection of dark matter. The discussion section presents a possible infrared scattering mechanism based on the metallic nature of n-type GaAs. Appendix A describes the Monte Carlo program steps in detail. Appendix B shows how narrow-beam and integrating sphere experiments can measure the cryogenic optical scattering and absolute absorption coefficients.
description: 12 pages, 7 tables, 2 Appendices. Submitted to Nuclear Instruments and Methods A
sj-docx-2-jtt-10.1177_1357633X211041011 - Supplemental material for Telemedicine use in orthopaedics: Experience during the COVID-19 pandemic
Creators: name: Chin, Brian Z
name: Nashi, Nazrul
name: Lin, Shuxun
name: Yik, Kevin
name: Tan, Gamaliel
name: Kagda, Fareed HY
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 111708 Health and Community Services
subject: FOS: Health sciences
subject: 111799 Public Health and Health Services not elsewhere classified

description: Supplemental material, sj-docx-2-jtt-10.1177_1357633X211041011 for Telemedicine use in orthopaedics: Experience during the COVID-19 pandemic by Brian Z Chin, Nazrul Nashi, Shuxun Lin, Kevin Yik, Gamaliel Tan and Fareed HY Kagda in Journal of Telemedicine and Telecare
Radio luminosity of GLEAM-X J162759.5-523504.3: does it really exceed the spin-down power of the pulsar?
Creators: name: Erkut, M. Hakan
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The recently discovered radio pulsar GLEAM-X J162759.5-523504.3 with an extremely long spin period was reported to have a radio luminosity that exceeds by orders of magnitude the spin-down power of the pulsar. In this Letter, we rigorously calculate the radio luminosity of the source taking into account the dependence of the opening angle of the pulsar-emission cone first on the spin period alone and then on both the spin parameters and the observing frequency. We also revise the value of the spin-down power reported previously. Our analysis is based on the description of the spectral data in terms of two power-law indices as well as a single power-law index. Even if the pulsar's opening angle is treated as a frequency-independent parameter in line with the usual assumption, the period dependence of this parameter implies relatively small opening angles and therefore radio luminosities well below the spin-down power. Although we estimate higher radio luminosities in the physically more plausible case of a frequency-dependent opening angle, the spin-down power is again not exceeded by the highest possible radio luminosity. The radio efficiency of GLEAM-X J162759.5-523504.3 can therefore not be used in favour of a magnetar hypothesis.
description: 5 pages, 3 figures, updated version, accepted for publication in MNRAS Letters
Linking the properties of accreting white dwarfs with the ionization state of their ambient medium
Creators: name: Souropanis, D.
name: Chiotellis, A.
name: Boumis, P.
name: Chatzikos, M.
name: Akras, S.
name: Piersanti, L.
name: Ruiter, A. J.
name: Ferland, G. J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Steadily accreting white dwarfs (WDs) are efficient sources of ionization and thus, are able to create extended ionized nebulae in their vicinity. These nebulae represent ideal tools for the detection of accreting WDs, given that in most cases the source itself is faint. In this work, we combine radiation transfer simulations with known H and He accreting WD models, providing for the first time the ionization state and the emission line spectra of the formed nebulae as a function of the WD mass, the accretion rate and the chemical composition of the accreted material. We find that the nebular optical line fluxes and radial extent vary strongly with the WD's accretion properties, peaking in systems with WD masses of 0.8 - 1.2 $\rm~M_{\odot}$. Projecting our results on the 'BPT' diagnostic diagrams, we show that accreting WDs nebulae possess characteristics distinct from those of H II-like regions, while they share similar line ratios with the galactic low-ionization emission-line regions. Finally, we compare our results to the relevant constraints imposed by the lack of ionized nebulae in the vicinity of supersoft X-ray sources (SSSs) and Type Ia supernova remnants - sources which are related to steadily accreting WDs. The large discrepancies uncovered by our comparison rule out any steadily accreting WD as a potential progenitor of the studied remnants and additionally require the ambient medium around the SSSs to be less dense than 0.2 $\rm~cm^{-3}$. We discuss possible alternatives that could bridge the incompatibility between the theoretical expectations and the relevant observations.
description: 16 pages, 6 figures, accepted to MNRAS
Can X-ray Observations Improve Optical-UV-based Accretion-Rate Estimates for Quasars?
Creators: name: Marlar, Andrea
name: Shemmer, Ohad
name: Brotherton, Michael S.
name: Richards, Gordon T.
name: Dix, Cooper
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Current estimates of the normalized accretion rates of quasars (L/L_Edd), rely on measuring the velocity widths of broad optical-UV emission lines (e.g., H$β$ and Mg II $\lambda2800$). However, such lines tend to be weak or inaccessible in the most distant quasars, leading to increasing uncertainty in L/L_Edd estimates at $z > 6$. Utilizing a carefully selected sample of 53 radio-quiet quasars that have H$β$ and C IV $\lambda1549$ spectroscopy as well as {\sl Chandra} coverage, we searched for a robust accretion-rate indicator for quasars, particularly at the highest-accessible redshifts ($z \sim 6-7$). Our analysis explored relationships between the H$β$-based L/L_Edd, the equivalent width (EW) of C IV, and the optical-to-X-ray spectral slope (a_ox). Our results show that EW(C IV) is the strongest indicator of the H$β$-based L/L_Edd parameter, consistent with previous studies, although significant scatter persists particularly for sources with weak C IV lines. We do not find evidence for the a_ox parameter improving this relation, and we do not find a significant correlation between a_ox and H$β$-based L/L_Edd. This absence of an improved relationship may reveal a limitation in our sample. X-ray observations of additional luminous sources, found at $z \gtrsim 1$, may allow us to mitigate the biases inherent in our archival sample and test whether X-ray data could improve L/L_Edd estimates. Furthermore, deeper X-ray observations of our sources may provide accurate measurements of the hard-X-ray power-law photon index ($Γ$), which is considered an unbiased L/L_Edd indicator. Correlations between EW(C IV) and a_ox with $Γ$-based L/L_Edd may yield a more robust prediction of a quasar normalized accretion rate.
description: 13 pages (aastex62), 4 figures. Accepted for publication in ApJ
Supplemental Material - Understanding Hesitation to Use Nicotine Replacement Therapy: A Content Analysis of Posts in Online Tobacco-Cessation Support Groups
Creators: name: Phillips, Connor
name: Pechmann, Cornelia
name: Calder, Douglas
name: Prochaska, Judith J
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 111799 Public Health and Health Services not elsewhere classified
subject: FOS: Health sciences

description: Supplemental Material for Understanding Hesitation to Use Nicotine Replacement Therapy: A Content Analysis of Posts in Online Tobacco-Cessation Support Groups by Connor Phillips, Cornelia Pechmann, Douglas Calder, and Judith J Prochaska in American Journal of Health Promotion
Hydrogeologic Investigations of Pavement Subsidence in the Cumberland Gap Tunnel
Creators: name: Dinger, James S.
name: Currens, James C.
name: Zhu, Junfeng
name: Webb, Steven E.
name: Rister, Brad W.
name: Graves, R.C.
name: Allen, David L.
name: Scully, Tim C.
Publisher: name: Kentucky Geological Survey, University of Kentucky
Year: 2014

description: Abstract:
Cumberland Gap Tunnel was constructed under Cumberland Gap National Historical Park in 1996 to improve transportation on a segment of U.S. 25E, connecting Kentucky and Tennessee and restoring Cumberland Gap to its historical appearance.
The concrete pavement in the tunnel started to subside in 2001. Ground penetrating radar surveys revealed voids in many areas of the limestone roadbed aggregate beneath the pavement. To investigate possible hydrogeologic processes that may have caused favorable conditions for voids to form in the aggregate, we studied geology, groundwater flow, and groundwater chemistry in the tunnel using a variety of methods, including bore drilling, packer test, dye tracing, groundwater- and surface-flow monitoring, water-chemistry modeling, and an aggregate dissolution experiment.
The study revealed that the aggregate receives a large volume of groundwater from much of the bedrock invert, but the flow velocity is too slow to transport small particles out of the aggregate. Calcite saturation indices calculated from water-chemistry data suggest that the groundwater was capable of continuously dissolving calcite, the primary mineral in the limestone aggregate. Water samples taken during different flow conditions indicate that groundwater under low-flow conditions. The dissolution experiment showed that all the limestone aggregate placed beneath the roadbed and in contact with groundwater lost mass; the highest mass loss was 3.4 percent during a 178-day period. The experiment also suggested that water with higher calcite-dissolving potential removed limestone mass quicker than water with low calcite-dissolving potential.
We recommend that the limestone aggregate be replaced with noncarbonate aggregate, such as granite, to prevent dissolution and future road subsidence.
sj-docx-1-scm-10.1177_00369330221112186 - Supplemental material for Design and testing of the safety of the SARUS-CPR hood for novice resuscitators
Creators: name: Wasik, P.
name: McLeod, G. A.
name: Mountain, R.
name: Watts, S.
name: Briggs, H.
name: Maini, N.
name: Belford, I.
name: McGuire, B.
name: Brown, W.
name: Clark, R.
name: Eley, I
name: Richardson, E.
name: Stonebridge, P.
Publisher: name: SAGE Journals
Year: 2022
Subjects: Medicine

description: Supplemental material, sj-docx-1-scm-10.1177_00369330221112186 for Design and testing of the safety of the SARUS-CPR hood for novice resuscitators by P. Wasik, G. A. McLeod, R. Mountain, S. Watts, H. Briggs, N. Maini, I. Belford, B. McGuire, W. Brown, R. Clark, I Eley, E. Richardson and P. Stonebridge in Scottish Medical Journal
Automatic detection of low surface brightness galaxies from SDSS images
Creators: name: Yi, Zhenping
name: Li, Jia
name: Du, Wei
name: Liu, Meng
name: Liang, Zengxu
name: Xing, Yongguang
name: Pan, Jingchang
name: Bu, Yude
name: Kong, Xiaoming
name: Wu, Hong
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Low surface brightness (LSB) galaxies are galaxies with central surface brightness fainter than the night sky. Due to the faint nature of LSB galaxies and the comparable sky background, it is difficult to search LSB galaxies automatically and efficiently from large sky survey. In this study, we established the Low Surface Brightness Galaxies Auto Detect model (LSBG-AD), which is a data-driven model for end-to-end detection of LSB galaxies from Sloan Digital Sky Survey (SDSS) images. Object detection techniques based on deep learning are applied to the SDSS field images to identify LSB galaxies and estimate their coordinates at the same time. Applying LSBG-AD to 1120 SDSS images, we detected 1197 LSB galaxy candidates, of which 1081 samples are already known and 116 samples are newly found candidates. The B-band central surface brightness of the candidates searched by the model ranges from 22 mag arcsec $^ {- 2} $ to 24 mag arcsec $^ {- 2} $, quite consistent with the surface brightness distribution of the standard sample. 96.46\% of LSB galaxy candidates have an axis ratio ($b/a$) greater than 0.3, and 92.04\% of them have $fracDev\_r$\textless 0.4, which is also consistent with the standard sample. The results show that the LSBG-AD model learns the features of LSB galaxies of the training samples well, and can be used to search LSB galaxies without using photometric parameters. Next, this method will be used to develop efficient algorithms to detect LSB galaxies from massive images of the next generation observatories.
description: 11 pages, 9 figures,accepted to be published on MNRAS
sj-docx-2-scm-10.1177_00369330221112186 - Supplemental material for Design and testing of the safety of the SARUS-CPR hood for novice resuscitators
Creators: name: Wasik, P.
name: McLeod, G. A.
name: Mountain, R.
name: Watts, S.
name: Briggs, H.
name: Maini, N.
name: Belford, I.
name: McGuire, B.
name: Brown, W.
name: Clark, R.
name: Eley, I
name: Richardson, E.
name: Stonebridge, P.
Publisher: name: SAGE Journals
Year: 2022
Subjects: Medicine

description: Supplemental material, sj-docx-2-scm-10.1177_00369330221112186 for Design and testing of the safety of the SARUS-CPR hood for novice resuscitators by P. Wasik, G. A. McLeod, R. Mountain, S. Watts, H. Briggs, N. Maini, I. Belford, B. McGuire, W. Brown, R. Clark, I Eley, E. Richardson and P. Stonebridge in Scottish Medical Journal
Probing the Galactic Halo with RR Lyrae Stars. II. The Substructures of the Milky Way
Creators: name: Wang, F.
name: Zhang, H. -W.
name: Xue, X. -X.
name: Huang, Y.
name: Liu, G. -C.
name: Zhang, L.
name: Yang, C. -Q.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We identify substructures of the Galactic halo using 3,003 type $ab$ RR Lyraes (RRab) with 6D position-velocity information from the SDSS, LAMOST, and Gaia EDR3. Based on the information, we define the separation of any two of the stars in the integrals of motion space and identify substructures by utilizing the friends-of-friends algorithm. We identify members belonging to several known substructures: the Sagittarius stream, the Gaia-Enceladus-Sausage (GES), the Sequoia, and the Helmi streams. In addition to these known substructures, there are three other substructures possibly associated with globular clusters NGC 5272, NGC 6656, and NGC 5024, respectively. Finally, we also find three remaining unknown substructures and one of them has large angular momentum and a mean metallicity $\rm -2.13\,dex$ which may be a new substructure. As for GES, we find that it accounts for a large part of substructures in the inner halo and the range of apocenter distance is from 10 to $34\,\rm kpc$, which suggests that the GES is mainly distributed in the inner halo. The near one-third proportion of the GES and the peak value $20\,\rm kpc$ of the apocenter distances suggest that GES could account for the break in the density profile of the Galactic halo at Galactocentric distance ${\sim}20-25\,\rm kpc$. The similarity of comparing the kinematic properties of Gaia-Enceladus-Sausage with the Hercules-Aquila Cloud and Virgo Overdensity suggests that the three substructures may have similar origins.
description: 14 pages, 14 figures, accepted by MNRAS
Phlugiolopsis montana Wang, Li & Liu 2012
Creators: name: Yao, Yuqing
name: Bian, Xun
name: Zhang, Bin
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Orthoptera
Tettigoniidae
Phlugiolopsis
Phlugiolopsis montana

description: Phlugiolopsis montana Wang, Li & Liu, 2012
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Figure 4
Material examined. 2 males and 1 female, Baihualing, Baoshan, Yunnan, August 6, 2023, coll. by Siyu Pang and Ting Luo; 1 male, Baihualing, Baoshan, Yunnan, August 27, 2024, coll. by Ting Luo and Yanting Qin; 6 males and 3 females, Laifengshan, Tengchong, Yunnan, September 3, 2024, coll. by Ting Luo and Yanting Qin.
Distribution. Yunnan (Baoshan, Tengchong)
description: Published as part of Yao, Yuqing, Bian, Xun & Zhang, Bin, 2025, Four new species of the genus Phlugiolopsis (Orthoptera: Tettigoniidae: Meconematinae) from Western Yunnan, China, pp. 568-578 in Zootaxa 5590 (4) on page 575, DOI: 10.11646/zootaxa.5590.4.7, http://zenodo.org/record/14953625
Photometric redshifts and Galaxy Clusters for DES DR2, DESI DR9, and HSC-SSP PDR3 Data
Creators: name: Zou, Hu
name: Sui, Jipeng
name: Xue, Suijian
name: Zhou, Xu
name: Ma, Jun
name: Zhou, Zhimin
name: Nie, Jundan
name: Zhang, Tianmeng
name: Feng, Lu
name: Shen, Zhixia
name: Wang, Jiali
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Photometric redshift (photo-z) is a fundamental parameter for multi-wavelength photometric surveys, while galaxy clusters are important cosmological probers and ideal objects for exploring the dense environmental impact on galaxy evolution. We extend our previous work on estimating photo-z and detecting galaxy clusters to the latest data releases of the Dark Energy Spectroscopic Instrument (DESI) imaging surveys, Dark Energy Survey (DES), and Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) imaging surveys and make corresponding catalogs publicly available for more extensive scientific applications. The photo-z catalogs include accurate measurements of photo-z and stellar mass for about 320, 293, and 134 million galaxies with $r<23$, $i<24$, and $i<25$ in DESI DR9, DES DR2, and HSC-SSP PDR3 data, respectively. The photo-z accuracy is about 0.017, 0.024, and 0.029 and the general redshift coverage is $z<1$, $z<1.2$, and $z<1.6$, respectively for those three surveys. The uncertainties of the logarithmic stellar mass that is inferred from stellar population synthesis fitting is about 0.2 dex. With the above photo-z catalogs, galaxy clusters are detected using a fast cluster-finding algorithm. A total of 532,810, 86,963, and 36,566 galaxy clusters with the number of members larger than 10 are discovered for DESI, DES, and HSC-SSP, respectively. Their photo-z accuracy is at the level of 0.01. The total mass of our clusters are also estimated by using the calibration relations between the optical richness and the mass measurement from X-ray and radio observations. The photo-z and cluster catalogs are available at ScienceDB (https://www.doi.org/10.11922/sciencedb.o00069.00003) and PaperData Repository (https://doi.org/10.12149/101089).
description: 25 pages, 10 figures, accepted for publication in RAA
sj-docx-4-scm-10.1177_00369330221112186 - Supplemental material for Design and testing of the safety of the SARUS-CPR hood for novice resuscitators
Creators: name: Wasik, P.
name: McLeod, G. A.
name: Mountain, R.
name: Watts, S.
name: Briggs, H.
name: Maini, N.
name: Belford, I.
name: McGuire, B.
name: Brown, W.
name: Clark, R.
name: Eley, I
name: Richardson, E.
name: Stonebridge, P.
Publisher: name: SAGE Journals
Year: 2022
Subjects: Medicine

description: Supplemental material, sj-docx-4-scm-10.1177_00369330221112186 for Design and testing of the safety of the SARUS-CPR hood for novice resuscitators by P. Wasik, G. A. McLeod, R. Mountain, S. Watts, H. Briggs, N. Maini, I. Belford, B. McGuire, W. Brown, R. Clark, I Eley, E. Richardson and P. Stonebridge in Scottish Medical Journal
Additional file 1 of Ethical issues in vaccine trial participation by adolescents: qualitative insights on family decision making from a human papillomavirus vaccine trial in Tanzania
Creators: name: Frost, Lucy
name: Erio, Ms Tusajigwe
name: Whitworth, Hilary
name: Marwerwe, Ms Graca
name: Hayes, Richard
name: Baisley, Kathy
name: de SanJosé, Silvia
name: Watson-Jones, Deborah
name: Mitchell, Kirstin
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Biotechnology
Biological Sciences not elsewhere classified
Cancer
Science Policy

description: Supplementary Material 1
Additional file 1 of Associations of epigenetic age acceleration at birth and age 12 years with adolescent cardiometabolic risk: the HOME study
Creators: name: Arzu, Jennifer L.
name: Kelsey, Karl T.
name: Papandonatos, George D.
name: Cecil, Kim M.
name: Chen, Aimin
name: Langevin, Scott M.
name: Lanphear, Bruce P.
name: Yolton, Kimberly
name: Buckley, Jessie P.
name: Braun, Joseph M.
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: Physiology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Mental Health

description: Additional file1.
Many-quark interactions: Large-$N$ scaling and contribution to baryon masses
Creators: name: Buisseret, F.
name: Semay, C.
name: Willemyns, C. T.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Starting from an effective Hamiltonian modelling a baryon made of $N$ identical quarks in the large-$N$ approach of QCD, we obtain analytical formulas allowing to estimate the contributions of multiquark interactions to the baryon mass. The cases of vanishing (mass spectrum) and non-vanishing (baryon melting) temperatures are treated.
sj-docx-1-psp-10.1177_01461672221105958 – Supplemental material for The Effect of Counterfactual Potency on Behavioral Intentions
Creators: name: Kim, Woo J.
name: Summerville, Amy
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 170199 Psychology not elsewhere classified
subject: FOS: Psychology

description: Supplemental material, sj-docx-1-psp-10.1177_01461672221105958 for The Effect of Counterfactual Potency on Behavioral Intentions by Woo J. Kim and Amy Summerville in Personality and Social Psychology Bulletin
Phenomenology of diphoton photoproduction at next-to-leading order
Creators: name: Grocholski, Oskar
name: Pire, Bernard
name: Sznajder, Paweł
name: Szymanowski, Lech
name: Wagner, Jakub
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We develop the analysis of diphoton exclusive photoproduction in the kinematics where a collinear QCD factorization framework applies, namely nearly forward large invariant mass diphoton production. We work at the leading twist level and at the next-to-leading order (NLO) in the strong coupling constant $α_S$. We compare our predictions for cross-sections with Born order calculations for the experimental conditions accessible to JLab experiments and show the interesting sensitivity of our results to various models of generalized parton distributions (GPDs). The NLO corrections are rather large and negative but do not prevent the studied reaction from being a promising tool for the extraction of C-dd GPDs, which do not contribute to either spacelike or timelike deeply virtual Compton scattering amplitudes.
Supplemental Material - Exploration of the molecular mechanisms, shared gene signatures, and MicroRNAs between systemic lupus erythematosus and diffuse large B cell lymphoma by bioinformatics analysis
Creators: name: Peng, Zhishen
name: Liang, Xiaofeng
name: Lin, Xiaobing
name: Lin, Weiyi
name: Lin, Zien
name: Wei, Shanshan
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 111702 Aged Health Care
subject: FOS: Health sciences

description: Supplemental Material for Exploration of the molecular mechanisms, shared gene signatures, and MicroRNAs between systemic lupus erythematosus and diffuse large B cell lymphoma by bioinformatics analysis by Zhishen Peng, Xiaofeng Liang, Xiaobing Lin, Weiyi Lin, Zien Lin and Shanshan Wei in Lupus
Passive Laser Power Stabilization via an Optical Spring
Creators: name: Cullen, Torrey
name: Aronson, Scott
name: Pagano, Ron
name: Nery, Marina Trad
name: Cain, Henry
name: Cripe, Jonathon
name: Cole, Garret D.
name: Sharifi, Safura
name: Aggarwal, Nancy
name: Wilke, Benno
name: Corbitt, Thomas
Publisher: name: arXiv
Year: 2022
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Metrology experiments can be limited by the noise produced by the laser involved via small fluctuations in the laser's power or frequency. Typically, active power stabilization schemes consisting of an in-loop sensor and a feedback control loop are employed. Those schemes are fundamentally limited by shot noise coupling at the in-loop sensor. In this letter we propose to use the optical spring effect to passively stabilize the classical power fluctuations of a laser beam. In a proof of principle experiment, we show that the relative power noise of the laser is stabilized from approximately $2 \times 10^{-5}$ Hz$^{-1/2}$ to a minimum value of $1.6 \times 10^{-7}$ Hz$^{-1/2}$, corresponding to the power noise reduction by a factor of $125$. The bandwidth at which stabilization occurs ranges from $400$ Hz to $100$ kHz. The work reported in this letter further paves the way for high power laser stability techniques which could be implemented in optomechanical experiments and in gravitational wave detectors.
Influence des attitudes associées aux comportements sur l'intention entrepreneuriale des étudiants maliens : Cas de la FSEG /USSGB
Creators: name: Boubacar Soungalo DEMBÉLÉ
name: Kanidiala KEÏTA
name: Souaïbou Samba Lamine TRAORÉ
name: Soumaïla FANÉ
Publisher: name: Zenodo
Year: 2025

description: L’objectif principal de ce papier était d’examiner l’influence des attitudes associées au comportement sur l’intention entrepreneuriale des étudiants de la FSEG/USSGB. Dans la présente recherche, nous nous sommes appuyés sur la théorie du modèle de Tounès (2003) qui s’appuie sur le modèle de la formation de l’événement entrepreneurial de Sokol et Shapero (1982) qui mobilise la théorie du comportement planifié d’Ajzen (1991), nous sommes parvenus à nos objectifs.  La validation du modèle s’appuie sur nos visites dans ladite Faculté afin d’y interroger les animateurs des formations, à travers une enquête exploratoire de type qualitative auprès de 25 jeunes étudiant(e)s de la Faculté des Sciences Economiques et de Gestion de Bamako et l’étude empirique (étude quantitative) est conduite auprès de 250 étudiants(e)s de fin de cycle Licence (L3) toutes filières confondues pour l’étude confirmatoire. Les résultats obtenus nous révèlent que les attitudes associées au comportement à un effet positif et significatif sur l’intention entrepreneuriale avec β=0,048 et un t de Student significatif (t=8,269 et p-value <0,001).
Additional file 1 of Tsunami waveform inversion using Green’s functions with advection effects: application to the 2003 Tokachi–Oki earthquake
Creators: name: Yamanaka, Yusuke
name: Tanioka, Yuichiro
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: Physiology
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Plant Biology

description: Additional file 1.Supplementary Information
sj-docx-1-jic-10.1177_08850666211046175 - Supplemental material for CVP and echo Measurements are Associated with Improved Outcomes in Patients with Gastrointestinal (GI) Hemorrhage: A Retrospective Analysis of the MIMIC- IV Database
Creators: name: Song, Wenye
name: Mobli, Keyan
name: Jupiter, Daniel C.
name: Radhakrishnan, Ravi S.
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 110305 Emergency Medicine
subject: FOS: Clinical medicine
subject: 111702 Aged Health Care
subject: FOS: Health sciences
subject: 110203 Respiratory Diseases

description: Supplemental material, sj-docx-1-jic-10.1177_08850666211046175 for CVP and echo Measurements are Associated with Improved Outcomes in Patients with Gastrointestinal (GI) Hemorrhage: A Retrospective Analysis of the MIMIC- IV Database by Wenye Song, Keyan Mobli, Daniel C. Jupiter and Ravi S. Radhakrishnan in Journal of Intensive Care Medicine
Magnetic order and exchange couplings in the frustrated diamond lattice antiferromagnet MnSc$_2$Se$_4$
Creators: name: Guratinder, K.
name: Tsurkan, V.
name: Prodan, L.
name: Keller, L.
name: Embs, J. P.
name: Juranyi, F.
name: Medarde, M.
name: Rüegg, Ch.
name: Zaharko, O.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report the magnetic properties of $A$-site spinel compound MnSc$_2$Se$_4$. The macroscopic magnetic measurements uncovers successive magnetic transitions at $T_{\rm{N1}}$= 2.04 K, followed by two further transitions at $T_{\rm{N2}}$=1.8 K and $T_{\rm{N3}}$=1.6 K. Neutron powder diffraction reveals that both, $T_{\rm{N2}} < T < T_{\rm{N1}}$ and $T
description: Accepted in Phys. Rev. B
Additional file 1 of Development and application of the Meal and Snack Assessment (MESA) quality scale for children and adolescents using item response theory
Creators: name: Lemke, Stella
name: de Andrade, Dalton Francisco
name: de Fragas Hinnig, Patrícia
name: da Silva, Silvio Aparecido
name: Vincenzi, Silvana Ligia
name: Roberto, Denise Miguel Teixeira
name: Lobo, Adriana Soares
name: Vieira, Francilene Gracieli Kunradi
name: Di Pietro, Patricia Faria
name: de Assis, Maria Alice Altenburg
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Biological Sciences not elsewhere classified
Science Policy

description: Supplementary Material 1.
Additional file 1 of Iron deficiency anemia and its association with cognitive function among adolescents in the Ashanti Region - Ghana
Creators: name: Yeboah, Francis Agyemang
name: Bioh, Joyce
name: Amoani, Benjamin
name: Effah, Alfred
name: Senu, Ebenezer
name: Mensah, Oscar Simon Olympio
name: Agyei, Alex
name: Kwarteng, Samuel
name: Agomuo, Samuel Kwame Sopuruchi
name: Opoku, Stephen
name: Agordzo, Samuel Kekeli
name: Aidoo, Ebenezer Krampah
name: Sakyi, Samuel Asamoah
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Neuroscience
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Mental Health

description: Supplementary Material 1
sj-docx-3-pie-10.1177_09544089231159780 - Supplemental material for Effect of deep cryogenic treatment, tempering temperature and time on hardness of Nimonic-90
Creators: name: Singh, Gurkirat
name: Pandey, Kailash Nath
Publisher: name: SAGE Journals
Year: 2023
Subjects: subject: 99999 Engineering not elsewhere classified
subject: FOS: Other engineering and technologies
subject: 91299 Materials Engineering not elsewhere classified
subject: FOS: Materials engineering

description: Supplemental material, sj-docx-3-pie-10.1177_09544089231159780 for Effect of deep cryogenic treatment, tempering temperature and time on hardness of Nimonic-90 by Gurkirat Singh and Kailash Nath Pandey in Proceedings of the Institution of Mechanical Engineers, Part E: Journal of Process Mechanical Engineering
Alignment of the central galaxies with the environment
Creators: name: Rodriguez, Facundo
name: Merchán, Manuel
name: Artale, M. Celeste
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In this work, we combine ellipticity and major axis position angle measurements from the Sloan Digital Sky Server Data Release 16 (SDSS DR16) with the group finder algorithm of Rodriguez \& Merchán to determine the alignment of the central galaxies with the surrounding structures and satellite galaxies lying in their group. We use two independent methods: A modified version of the two-point cross-correlation function and the angle between the central galaxy orientation and the satellite galaxies relative position. The first method allows us to study the inner and outer regions of the cluster, while the second method provides information within the halos. Our results show that central galaxies present anysotropy in the correlation function up to $\sim 10 h^{-1}Mpc$, which becomes $\sim$10\% stronger for the brightest ones ($^{0.1}M_{r}
description: 11 pages, 10 figures, Approved for publication in MNRAS
Gravitational-Wave Signatures of Chiral-Symmetric Technicolor
Creators: name: Yang, Hao
name: Freitas, Felipe F.
name: Marciano, Antonino
name: Morais, António P.
name: Pasechnik, Roman
name: Viana, João
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: A chiral-symmetric technicolor model successfully reconciles the tension between electroweak precision tests and traditional technicolor models. Focusing on its simplest realization preserving the conventional Higgs mechanism, we study its primordial gravitational wave signatures originating from first order phase transitions in the early Universe. We found that abundant phase transition patterns arise from a physically viable parameter space. Besides, we have also found gravitational wave signals possibly visible by future experiments, such as LISA, BBO and u-DECIGO. Our results stress the importance of gravitational wave detectors in exploring new physics complementary to ground colliders in the multi-messenger astronomy era.
description: 9 pages, 6 figures, 3 tables; accepted for publication in Phys. Lett. B
Additional file 2 of Ethical issues in vaccine trial participation by adolescents: qualitative insights on family decision making from a human papillomavirus vaccine trial in Tanzania
Creators: name: Frost, Lucy
name: Erio, Ms Tusajigwe
name: Whitworth, Hilary
name: Marwerwe, Ms Graca
name: Hayes, Richard
name: Baisley, Kathy
name: de SanJosé, Silvia
name: Watson-Jones, Deborah
name: Mitchell, Kirstin
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Biotechnology
Biological Sciences not elsewhere classified
Cancer
Science Policy

description: Supplementary Material 2
An Alternative Framework for E-Model Inflation in Supergravity
Creators: name: Pallis, C.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We present novel realizations of E-model inflation within Supergravity which are largely associated with the existence of a pole of order one in the kinetic term of the (gauge-singlet) inflaton superfield. This pole arises due to the selected logarithmic Kahler potentials K1 and ~K1, which parameterize the same hyperbolic manifold with scalar curvature R=-2/N, where N>0 is the coefficient of a logarithmic term. The associated superpotential W exhibits the same R charge with the inflaton-accompanying superfield and includes all the allowed renormalizable terms. For K=K1, inflation can be attained for N=2 at the cost of some tuning regarding the coefficients of the W terms and predicts a tensor-to-scalar ratio r at the level of 0.001. The tuning can be totally eluded for K=~K1, which allows for quadratic- and quartic-like models with N values increasing with r and spectral index ns close or even equal to its present central observational value.
description: To appear in EPJC
Harvesting Entanglement by non-identical detectors with different energy gaps
Creators: name: Hu, Hui
name: Zhang, Jialin
name: Yu, Hongwei
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: It has been shown that the vacuum state of a free quantum field is entangled and such vacuum entanglement can be harvested by a pair of initially uncorrelated detectors interacting locally with the vacuum field for a finite time. In this paper, we examine the entanglement harvesting phenomenon of two non-identical inertial detectors with different energy gaps locally interacting with massless scalar fields via a Gaussian switching function. We focus on how entanglement harvesting depends on the energy gap difference from two perspectives: the amount of entanglement harvested and the harvesting-achievable separation between the two detectors. In the sense of the amount of entanglement, we find that as long as the inter-detector separation is not too small with respect to the interaction duration parameter, two non-identical detectors could extract more entanglement from the vacuum state than the identical detectors. There exists an optimal value of the energy gap difference when the inter-detector separation is sufficiently large that renders the harvested entanglement to peak. Regarding the harvesting-achievable separation, we further find that the presence of an energy gap difference generally enlarges the harvesting-achievable separation range. Our results suggest that the non-identical detectors may be advantageous to extracting entanglement from vacuum in certain circumstances as compared to identical detectors.
description: 16 pages,5 figures
sj-docx-5-cpc-10.1177_10556656231163725 - Supplemental material for Bone Density of the Condyle of Children with Craniofacial Microsomia and its Correlation with Condylar Resorption After Mandible Distraction Osteogenesis
Creators: name: Li, Xiyuan
name: Zhang, Zhiyong
name: Tang, Xiaojun
name: Li, Chuan
name: Liu, Wei
Publisher: name: SAGE Journals
Year: 2023
Subjects: Surgery

description: Supplemental material, sj-docx-5-cpc-10.1177_10556656231163725 for Bone Density of the Condyle of Children with Craniofacial Microsomia and its Correlation with Condylar Resorption After Mandible Distraction Osteogenesis by Xiyuan Li, Zhiyong Zhang, Xiaojun Tang, Chuan Li and Wei Liu in The Cleft Palate Craniofacial Journal
Additional file 1 of Behavioral skills training for teaching safety skills to mental health service providers compared to training-as-usual: a pragmatic randomized control trial
Creators: name: Lin, Elizabeth
name: Malhas, Mais
name: Bratsalis, Emmanuel
name: Thomson, Kendra
name: Hargreaves, Fabienne
name: Donner, Kayle
name: Baig, Heba
name: Boateng, Rhonda
name: Swain, Rajlaxmi
name: Benadict, Mary Benisha
name: Busch, Louis
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology
subject: Mental Health

description: Additional file 1.
Additional file 3 of Ethical issues in vaccine trial participation by adolescents: qualitative insights on family decision making from a human papillomavirus vaccine trial in Tanzania
Creators: name: Frost, Lucy
name: Erio, Ms Tusajigwe
name: Whitworth, Hilary
name: Marwerwe, Ms Graca
name: Hayes, Richard
name: Baisley, Kathy
name: de SanJosé, Silvia
name: Watson-Jones, Deborah
name: Mitchell, Kirstin
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Biotechnology
Biological Sciences not elsewhere classified
Cancer
Science Policy

description: Supplementary Material 3
Dark Matter-Induced Multi-Phase Dynamical Symmetry Breaking
Creators: name: Kannike, Kristjan
name: Koivunen, Niko
name: Kubarski, Aleksei
name: Marzola, Luca
name: Raidal, Martti
name: Strumia, Alessandro
name: Vipp, Venno
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We consider the classically scale invariant Higgs-dilaton model of dynamical symmetry breaking extended with an extra scalar field that plays the role of dark matter. The Higgs boson is light near a critical boundary between different symmetry breaking phases, where quantum corrections beyond the usual Gildener-Weinberg approximation become relevant. This implies a tighter connection between dark matter and Higgs phenomenology. The model has only three free parameters, yet it allows for the observed relic abundance of dark matter while respecting all constraints. The direct detection cross section mediated by the Higgs boson is determined by the dark matter mass alone and is testable at future experiments.
description: 9 pages, 4 figures; for a webinar presentation of the paper see https://www.youtube.com/watch?v=ZTIdhPiI7hk
Constructing Teachers Identity: A Narrative Analysis of Chinese Teachers' Strategies in Managing Unruly Students
Creators: name: Mengyan Ma, Zhijia Feng
Publisher: name: Zenodo
Year: 2025
Subjects: Narrative Analysis, Chinese-English Teacher, Identity Construction, English Teaching, Unruly Students

description: The development of teacher identity and its evolution in various contexts is an increasingly focused area of research. This study examines How teachers construct their identity in discourse when dealing with unruly students. The beliefs, identities, and emotions of teachers, which are central to their professional activities, stem from their work experiences, teaching practices, and learning histories. By employing convenience sampling method, four participants offered valuable experience in dealing with unruly students. These aspects play a crucial role in shaping their classroom management strategies and decision-making processes. Through the lens of narrative analysis, the findings indicate that while teachers have diverse attitudes and strategies towards managing disruptive behaviors, they commonly utilize interpersonal skills to build rapport and foster understanding. Considering the Chinese educational context, there is a notable deficiency in research employing narrative analysis to investigate the identity construction of Chinese-English teachers faced with student misbehavior. This study aims to address this research gap by providing insights into the dynamic nature of teacher identity in challenging classroom situations.
Moving structures in ultraviolet bright points: observations from Solar Orbiter/EUI
Creators: name: Li, Dong
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Moving structures have been detected in coronal bright points and in a solar flare in active regions, which were bi-directional, symmetrical, simultaneous, and quasi-periodic (Ning & Guo 2014; Ning 2016; Li et al. 2016a). They could be regarded as observational evidence of plasma outflows via magnetic reconnection. In this article, we explored pairs of moving structures in fifteen ultraviolet bright points (UBPs), which were observed in the quiet Sun or inside a small active region on 19 November 2020, and measured by the High Resolution (HRI) Telescopes of the Extreme Ultraviolet Imager (EUI) on board the Solar Orbiter (SolO) in two passbands, HRIEUV 174 Å and HRILyα 1216 Å. Moving structures observed in ten UBPs as starting from their bright cores and propagating toward two ends, are interpreted as diverging motions of bi-directional moving structures. These moving structures are also characterized by simultaneity and symmetry and in the case of seven UBPs they exhibit quasi-periodicity. They could be generated by outflows after magnetic reconnections. Moving structures seen in another five UBPs as originating from double ends and moving closer, and merging together, are manifested as converging motions, which might be caused by inflows through the magnetic reconnection, or might be interpreted as upflows driven by the chromospheric evaporation.
description: Accepted for publication in Astronomy & Astrophysics