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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3TP7UN8
Repositorysid.inpe.br/mtc-m21c/2019/08.01.10.49   (restricted access)
Last Update2019:08.01.10.49.52 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2019/08.01.10.49.53
Metadata Last Update2020:01.06.11.42.17 (UTC) administrator
DOI10.1140/epjc/s10052-019-7087-7
ISSN1434-6044
Citation KeyKumarNuneYada:2019:ReTeCM
TitleDark sector interaction: a remedy of the tensions between CMB and LSS data
Year2019
MonthJuly
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size517 KiB
2. Context
Author1 Kumar, Suresh
2 Nunes, Rafael da Costa
3 Yadav, Santosh Kumar
Group1
2 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 BITS Pilani
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 BITS Pilani
Author e-Mail Address1 suresh.kumar@pilani.bits-pilani.ac.in
2 rafadcnunes@gmail.com
3 sky91bbaulko@gmail.com
JournalEuropean Physical Journal C
Volume79
Number7
Pagese576
Secondary MarkA2_INTERDISCIPLINAR A2_BIOTECNOLOGIA A2_ASTRONOMIA_/_FÍSICA B1_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B1_ENGENHARIAS_IV
History (UTC)2019-08-01 10:50:25 :: simone -> administrator :: 2019
2020-01-06 11:42:17 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractThe well-known tensions on the cosmological parameters H0 and sigma 8 within the Lambda CDM cosmology shown by the Planck-CMB and LSS data are possibly due to the systematics in the data or our ignorance of some new physics beyond the Lambda CDM model. In this letter, we focus on the second possibility, and investigate a minimal extension of the Lambda CDM model by allowing a coupling between its dark sector components (dark energy and dark matter). We analyze this scenario with Planck-CMB, KiDS and HST data, and find that the H0 and sigma 8 tensions disappear. In the joint analyses with Planck, HST and KiDS data, we find non-zero coupling in the dark sector up to 99% CL. Thus, we find a strong statistical support from the observational data for an interaction in the dark sector of the Universe while solving the H0 and sigma 8 tensions simultaneously.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Dark sector interaction:...
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4. Conditions of access and use
Languageen
Target Filekumar_dark.pdf
User Groupsimone
Reader Groupadministrator
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Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.00.07 2
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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