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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/47GU5MH
Repositorysid.inpe.br/mtc-m21d/2022/08.29.12.16
Last Update2022:08.29.12.16.34 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/08.29.12.16.34
Metadata Last Update2023:01.03.16.46.14 (UTC) administrator
DOI10.1103/PhysRevD.106.023530
ISSN1550-2368
1550-7998
Citation KeyGariazzoDiVaMenaNune:2022:LaInCo
TitleLate-time interacting cosmologies and the Hubble constant tension
Year2022
MonthJuly
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size1929 KiB
2. Context
Author1 Gariazzo, Stefano
2 Di Valentino, Eleonora
3 Mena, Olga
4 Nunes, Rafael da Costa
ORCID1 0000-0002-4160-6987
Group1
2
3
4 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Istituto Nazionale di Fisica Nucleare (INFN)
2 University of Sheffield
3 Universidad de Valencia-CSIC
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 gariazzo@to.infn.it
2 e.divalentino@sheffield.ac.uk
3 omena@ific.uv.es
4 rafadcnunes@gmail.com
JournalPhysical Review D
Volume106
Number2
Pagese023530
Secondary MarkA2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B2_ENSINO B2_ENGENHARIAS_IV B4_ENGENHARIAS_III C_ASTRONOMIA_/_FÍSICA
History (UTC)2022-08-29 12:16:34 :: simone -> administrator ::
2022-08-29 12:16:35 :: administrator -> simone :: 2022
2022-08-29 12:17:06 :: simone -> administrator :: 2022
2023-01-03 16:46:14 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
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Transferable1
Content TypeExternal Contribution
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AbstractIn this manuscript we reassess the potential of interacting dark matter-dark energy models in solving the Hubble constant tension. These models have been proposed but also questioned as possible solutions to the H0 problem. Here we examine several interacting scenarios against cosmological observations, focusing on the important role played by the calibration of supernovae data. In order to reassess the ability of interacting dark matter-dark energy scenarios in easing the Hubble constant tension, we systematically confront their theoretical predictions using a prior on the supernovae Ia absolute magnitude MB, which has been argued to be more robust and certainly less controversial than using a prior on the Hubble constant H0. While some data combinations do not show any preference for interacting dark sectors and in some of these scenarios the clustering σ8 tension worsens, interacting cosmologies with a dark energy equation of state w<-1 are preferred over the canonical ΛCDM picture even with cosmic microwave background data alone and also provide values of σ8 in perfect agreement with those from weak lensing surveys. Future cosmological surveys will test these exotic dark energy cosmologies by accurately measuring the dark energy equation of state and its putative redshift evolution.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Late-time interacting cosmologies...
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4. Conditions of access and use
data URLhttp://mtc-m21d.sid.inpe.br/ibi/8JMKD3MGP3W34T/47GU5MH
zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/47GU5MH
Languageen
Target FilePhysRevD.106.023530.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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