Publicação: A test of the standard dark matter density evolution law using galaxy clusters and cosmic chronometers
dc.contributor.author | Bora, Kamal | |
dc.contributor.author | Holanda, R. F.L. | |
dc.contributor.author | Desai, Shantanu | |
dc.contributor.author | Pereira, S. H. [UNESP] | |
dc.contributor.institution | Hyderabad | |
dc.contributor.institution | Universidade Federal do Rio Grande do Norte | |
dc.contributor.institution | Universidade Federal de Campina Grande | |
dc.contributor.institution | Universidade Federal de Sergipe (UFS) | |
dc.contributor.institution | Universidade Estadual Paulista (UNESP) | |
dc.date.accessioned | 2022-04-29T08:38:35Z | |
dc.date.available | 2022-04-29T08:38:35Z | |
dc.date.issued | 2022-01-01 | |
dc.description.abstract | In this paper, we implement a test of the standard law for the dark matter density evolution as a function of redshift. For this purpose, only a flat universe and the validity of the FRW metric are assumed. A deformed dark matter density evolution law is considered, given by ρc(z) ∝ (1 + z) 3+ϵ, and constraints on ϵ are obtained by combining the galaxy cluster gas mass fractions with cosmic chronometers measurements. We find that ϵ= 0 within 2σ c.l., in full agreement with other recent analyses. | en |
dc.description.affiliation | Department of Physics Indian Institute of Technology Hyderabad, Telangana | |
dc.description.affiliation | Departamento de Física Universidade Federal do Rio Grande do Norte, Rio Grande do Norte | |
dc.description.affiliation | Departamento de Física Universidade Federal de Campina Grande, PB | |
dc.description.affiliation | Departamento de Física Universidade Federal de Sergipe, SE | |
dc.description.affiliation | Departamento de Física Faculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista (UNESP), SP | |
dc.description.affiliationUnesp | Departamento de Física Faculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista (UNESP), SP | |
dc.description.sponsorship | Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) | |
dc.description.sponsorshipId | CNPq: 28755/2018-6 | |
dc.identifier | http://dx.doi.org/10.1140/epjc/s10052-022-09987-3 | |
dc.identifier.citation | European Physical Journal C, v. 82, n. 1, 2022. | |
dc.identifier.doi | 10.1140/epjc/s10052-022-09987-3 | |
dc.identifier.issn | 1434-6052 | |
dc.identifier.issn | 1434-6044 | |
dc.identifier.scopus | 2-s2.0-85122766930 | |
dc.identifier.uri | http://hdl.handle.net/11449/230213 | |
dc.language.iso | eng | |
dc.relation.ispartof | European Physical Journal C | |
dc.source | Scopus | |
dc.title | A test of the standard dark matter density evolution law using galaxy clusters and cosmic chronometers | en |
dc.type | Artigo | |
dspace.entity.type | Publication | |
unesp.author.orcid | 0000-0002-0466-3288[3] | |
unesp.department | Física e Química - FEG | pt |