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Record W3166868049 · doi:10.1103/physrevd.103.123528

Constraints on dark matter to dark radiation conversion in the late universe with DES-Y1 and external data

2021· article· en· W3166868049 on OpenAlexaff
Angela Chen, Dragan Huterer, S. Lee, A. Ferté, N. Weaverdyck, O. Alves, C. Danielle Leonard, N. MacCrann, Marco Raveri, A. Porredon, Eleonora Di Valentino, J. Muir, Pablo Lemos, Andrew R. Liddle, J. Blazek, A. Campos, R. Cawthon, A. Choi, Scott Dodelson, J. Elvin-Poole, D. Gruen, Ashley J. Ross, L F Secco, I. Sevilla-Noarbe, E. Sheldon, M. A. Troxel, J. Zuntz, T. M. C. Abbott, M. Aguena, S. Allam, J. Annis, S. Àvila, E. Bertin, S Bhargava, Sarah Bridle, D. Brooks, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, M. Costanzi, M. Crocce, L. N. da Costa, M. E. S. Pereira, T. M. Davis, P. Doel, T. F. Eifler, I. Ferrero, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztañaga, D. W. Gerdes, R. A. Gruendl, J. Gschwend, G. Gutiérrez, S. R. Hinton, K. Honscheid, B. Hoyle, D. J. James, Mike Jarvis, K. Kuehn, O. Lahav, M. A. G. Maia, J. L. Marshall, F. Menanteau, R. Miquel, R. Morgan, A. Palmese, F. Paz-Chinchón, A. Roodman, E. Sánchez, V. Scarpine, M. Schubnell, S. Serrano, M. Smith, E. Suchyta, G. Tarlé, D. Thomas, C. To, T N Varga, J. Weller, R. D. Wilkinson

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicCosmology and Gravitation Theories
Canadian institutionsPerimeter Institute
FundersSLAC National Accelerator LaboratoryH2020 European Research CouncilIntegrated Electronics Engineering Center, Binghamton UniversityEuropean Regional Development FundScience and Technology Facilities CouncilKavli Institute for Cosmological Physics, University of ChicagoSeventh Framework ProgrammeUniversity of Illinois at Urbana-ChampaignLudwig-Maximilians-Universität MünchenFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroCentro de Investigaciones Energéticas, Medioambientales y TecnológicasConselho Nacional de Desenvolvimento Científico e TecnológicoGeneralitat de CatalunyaOffice of ScienceUniversity of EdinburghCenter for Cosmology and Astroparticle Physics, Ohio State UniversityUniversity of SussexUniversity of CambridgeHigh Energy PhysicsDeutsche ForschungsgemeinschaftArgonne National LaboratoryCentres de Recerca de CatalunyaUniversity of PortsmouthUniversity of ChicagoTexas A and M UniversityInstitut de Física d'Altes EnergiesNational Centre for Supercomputing ApplicationsEidgenössische Technische Hochschule ZürichUniversity College LondonUniversity of MichiganUniversity of California, Santa CruzInstituto Nacional de Ciência e Tecnologia de Fármacos e MedicamentosOhio State UniversityMinistério da Ciência, Tecnologia e InovaçãoHigher Education Funding Council for EnglandLawrence Berkeley National LaboratoryFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaMinisterio de Ciencia e InnovaciónEuropean CommissionU.S. Department of EnergyUniversity of NottinghamStanford UniversityFermilabNational Science Foundation
KeywordsPhysicsDark radiationPlanckCosmic microwave backgroundDark energyBaryon acoustic oscillationsAstrophysicsDark matterHot dark matterScalar field dark matterRedshiftUniverseCosmologyGalaxyQuantum mechanics

Abstract

fetched live from OpenAlex

We study a phenomenological class of models where dark matter converts to dark radiation in the low redshift epoch. This class of models, dubbed DMDR, characterizes the evolution of comoving dark-matter density with two extra parameters, and may be able to help alleviate the observed discrepancies between early and late-time probes of the Universe. We investigate how the conversion affects key cosmological observables such as the cosmic microwave background (CMB) temperature and matter power spectra. Combining 3x2pt data from Year 1 of the Dark Energy Survey, Planck-2018 CMB temperature and polarization data, supernovae (SN) Type Ia data from Pantheon, and baryon acoustic oscillation (BAO) data from BOSS DR12, MGS and 6dFGS, we place new constraints on the amount of dark matter that has converted to dark radiation and the rate of this conversion. The fraction of the dark matter that has converted since the beginning of the Universe in units of the current amount of dark matter, $\ensuremath{\zeta}$, is constrained at 68% confidence level to be $<0.32$ for DES-Y1 3x2pt data, $<0.030$ for $\mathrm{CMB}+\mathrm{SN}+\mathrm{BAO}$ data, and $<0.037$ for the combined dataset. The probability that the DES and CMB+SN+BAO datasets are concordant increases from 4% for the $\mathrm{\ensuremath{\Lambda}}\mathrm{CDM}$ model to 8% (less tension) for DMDR. The tension in ${S}_{8}={\ensuremath{\sigma}}_{8}\sqrt{{\mathrm{\ensuremath{\Omega}}}_{m}/0.3}$ between DES-Y1 3x2pt and $\mathrm{CMB}+\mathrm{SN}+\mathrm{BAO}$ is slightly reduced from $2.3\ensuremath{\sigma}$ to $1.9\ensuremath{\sigma}$. We find no reduction in the Hubble tension when the combined data is compared to distance-ladder measurements in the DMDR model. The maximum-posterior goodness-of-fit statistics of DMDR and $\mathrm{\ensuremath{\Lambda}}\mathrm{CDM}$ model are comparable, indicating no preference for the DMDR cosmology over $\mathrm{\ensuremath{\Lambda}}\mathrm{CDM}$.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.004
metaresearch head score (Gemma)0.010
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.018
Threshold uncertainty score0.037

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0040.010
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.002
Science and technology studies0.0010.001
Scholarly communication0.0020.001
Open science0.0010.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0040.001

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.016
GPT teacher head0.375
Teacher spread0.359 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations38
Published2021
Admission routes1
Has abstractyes

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