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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/477SHFS
Repositorysid.inpe.br/mtc-m21d/2022/07.04.19.07
Last Update2022:07.04.19.07.05 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/07.04.19.07.05
Metadata Last Update2023:01.03.16.46.09 (UTC) administrator
DOI10.1103/PhysRevD.105.123506
ISSN1550-2368
1550-7998
Citation KeyNunesVagKumDiVMen:2022:NeTeDa
TitleNew tests of dark sector interactions from the full-shape galaxy power spectrum
Year2022
MonthJune
Access Date2024, May 13
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size662 KiB
2. Context
Author1 Nunes, Rafael da Costa
2 Vagnozzi, Sunny
3 Kumar, Suresh
4 Di Valentino, Eleonora
5 Mena, Olga
ORCID1 0000-0002-8432-5616
2 0000-0002-7614-6677
3 0000-0002-1638-2264
4 0000-0001-8408-6961
Group1 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 University of Cambridge
3
4 University of Sheffield
5 University of Valencia
Author e-Mail Address1 rafadcnunes@gmail.com
2 sunny.vagnozzi@ast.cam.ac.uk
3 suresh.math@igu.ac.in
4 e.divalentino@sheffield.ac.uk
5 omena@ific.uv.es
JournalPhysical Review D
Volume105
Number12
Pagese123506
Secondary MarkA2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B2_ENSINO B2_ENGENHARIAS_IV B4_ENGENHARIAS_III C_ASTRONOMIA_/_FÍSICA
History (UTC)2022-07-04 19:07:05 :: simone -> administrator ::
2022-07-04 19:07:06 :: administrator -> simone :: 2022
2022-07-04 19:07:49 :: simone -> administrator :: 2022
2023-01-03 16:46:09 :: administrator -> simone :: 2022
3. Content and structure
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Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractWe explore the role of redshift-space galaxy clustering data in constraining nongravitational interactions between dark energy (DE) and dark matter (DM), for which state-of-the-art limits have so far been obtained from late-time background measurements. We use the joint likelihood for prereconstruction full-shape (FS) galaxy power spectrum and postreconstruction Baryon Acoustic Oscillation (BAO) measurements from the BOSS DR12 sample, alongside Cosmic Microwave Background (CMB) data from Planck: from this dataset combination we infer H0 1/4 68.02+0.49 and the 2?? lower limit ?? > ???0.12, among the strongest limits ever reported on the DM-DE coupling strength ?? for the particular model considered. Contrary to what has been observed for the ??CDM model and simple extensions thereof, we find that the CMB + FS combination returns tighter constraints compared to the CMB + BAO one, suggesting that there is valuable additional information contained in the broadband of the power spectrum. We test this finding by running additional CMB-free analyses and removing sound horizon information, and discuss the important role of the equality scale in setting constraints on DM-DE interactions. Our results reinforce the critical role played by redshift-space galaxy clustering measurements in the epoch of precision cosmology, particularly in relation to tests of nonminimal dark sector extensions of the ??CDM model.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > New tests of...
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4. Conditions of access and use
data URLhttp://mtc-m21d.sid.inpe.br/ibi/8JMKD3MGP3W34T/477SHFS
zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/477SHFS
Languageen
Target FilePhysRevD.105.123506.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/bibdigital/2022/04.03.17.52 1
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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