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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br (namespace prefix: upn:3Q3U5H8)
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/43JA6PE
Repositorysid.inpe.br/mtc-m21c/2020/11.11.10.05   (restricted access)
Last Update2020:11.11.10.05.02 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2020/11.11.10.05.02
Metadata Last Update2022:01.04.01.35.37 (UTC) administrator
DOI10.1140/epjc/s10052-020-08522-6
ISSN1434-6044
Citation KeyBengalyGonzAlca:2020:ThEvHo
TitleIs there evidence for a hotter Universe?
Year2020
MonthOct.
Access Date2025, Dec. 09
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size628 KiB
2. Context
Author1 Bengaly, Carlos A. P.
2 Gonzalez, Javier E.
3 Alcaniz, Janilson Souza de
Group1
2
3 CRCRN-COCRE-INPE-MCTIC-GOV-BR
Affiliation1 Observatório Nacional (ON)
2 Universidade Federal do Rio Grande do Norte (UFRN)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 carlosbengaly@on.br
2 gonzalezsjavier@gmail.com
3 lcaniz@on.br
JournalEuropean Physical Journal C
Volume80
Number10
Pagese936
Secondary MarkA2_INTERDISCIPLINAR A2_BIOTECNOLOGIA A2_ASTRONOMIA_/_FÍSICA B1_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B1_ENGENHARIAS_IV
Host Collectionurlib.net/www/2017/11.22.19.04 upn:3Q3U5H8
History (UTC)2020-11-11 10:05:55 :: simone -> administrator :: 2020
2022-01-04 01:35:37 :: administrator -> simone :: 2020
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
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Content TypeExternal Contribution
Version Typepublisher
AbstractThe measurement of present-day temperature of the Cosmic Microwave Background (CMB), T0 = 2.72548± 0.00057 K (1σ), made by the Far-InfraRed Absolute Spectrophotometer (FIRAS) as recalibrated by the Wilkinson Microwave Anisotropy Probe (WMAP), is one of the most precise measurements ever made in Cosmology. On the other hand, estimates of the Hubble Constant, H0, obtained from measurements of the CMB temperature fluctuations assuming the standard ΛCDM model exhibit a large (4.1σ) tension when compared with low-redshift, model-independent observations. Recently, some authors argued that a slightly change in T0 could alleviate or solve the H0-tension problem. Here, we investigate evidence for a hotter or colder universe by performing an independent analysis from currently available temperature-redshift T (z) measurements. Our analysis (parametric and non-parametric) shows a good agreement with the FIRAS measurement and a discrepancy of ≥ 1.9σ from the T0 values required to solve the H0 tension. This result reinforces the idea that a solution of the H0-tension problem in fact requires either a better understanding of the systematic errors on the H0 measurements or new physics.
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4. Conditions of access and use
Languageen
Target FileBengaly2020_Article_IsThereEvidenceForAHotterUnive.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/3EUAPES
Citing Item Listsid.inpe.br/bibdigital/2013/10.03.20.46 - 56
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
6. Notes
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