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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3UGD4E2
Repositorysid.inpe.br/mtc-m21c/2019/12.03.15.09
Last Update2019:12.03.15.09.15 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2019/12.03.15.09.15
Metadata Last Update2020:01.06.11.42.24 (UTC) administrator
DOI10.1093/mnras/stz2676
ISSN0035-8711
1365-2966
Citation KeyKumarNuneYada:2019:TeWaDa
TitleTesting the warmness of dark matter
Year2019
MonthNov.
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size1088 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
JournalMonthly Notices of the Royal Astronomical Society
Volume490
Number1
Pages1406-1414
Secondary MarkA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A2_ASTRONOMIA_/_FÍSICA B2_ENSINO B5_ENGENHARIAS_IV
History (UTC)2019-12-03 15:09:15 :: simone -> administrator ::
2019-12-03 15:09:16 :: administrator -> simone :: 2019
2019-12-03 15:10:03 :: simone -> administrator :: 2019
2020-01-06 11:42:24 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordscosmological parameters
dark energy
dark matter
cosmology: observations
AbstractDark matter (DM) as a pressureless perfect fluid provides a good fit of the standard Lambda cold dark matter (Lambda CDM) model to the astrophysical and cosmological data. In this paper, we investigate two extended properties of DM: a possible time dependence of the equation of state of DM via Chevallier-Polarski-Linder parametrization, w(dm) = w(dm0) + w(dm1)(1 - a), and the constant non-null sound speed (c) over cap (2)(s,dm). We analyse these DM properties on top of the base Lambda CDM model by using the data from Planck cosmic microwave background (CMB) temperature and polarization anisotropy, baryonic acoustic oscillations (BAOs), and the local value of the Hubble constant from the Hubble Space Telescope (HST). We find new and robust constraints on the extended free parameters of DM. The most tight constraints are imposed by CMB+BAO data, where the three parameters w(dm0), w(dm1), and (c) over cap (2)(s,dm) are, respectively, constrained to be less than 1.43 x 10(-3), 1.44 x 10(-3), and 1.79 x 10(-6) at 95 per cent CL. All the extended parameters of DM show consistency with zero at 95 per cent CL, indicating no evidence beyond the CDM paradigm. We notice that the extended properties of DM significantly affect several parameters of the base Lambda CDM model. In particular, in all the analyses performed here, we find significantly larger mean values of H-0 and lower mean values of sigma(8) in comparison to the base Lambda CDM model. Thus, the well-known H-0 and sigma(8) tensions might be reconciled in the presence of extended DM parameters within the Lambda CDM framework. Also, we estimate the warmness of DM particles as well as its mass scale, and find a lower bound: similar to 500 eV from our analyses.
AreaCEA
ArrangementTesting the warmness...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3UGD4E2
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3UGD4E2
Languageen
Target Filekumar_testing.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.00.07 4
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
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