The imprint of the interaction between dark sectors in galaxy clusters
Contribuinte(s) |
UNIVERSIDADE DE SÃO PAULO |
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Data(s) |
20/10/2012
20/10/2012
2010
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Resumo |
Based on perturbation theory, we study the dynamics of how dark matter and dark energy in the collapsing system approach dynamical equilibrium when they are in interaction. We find that the interaction between dark sectors cannot ensure the dark energy to fully cluster along with dark matter. When dark energy does not trace dark matter, we present a new treatment on studying the structure formation in the spherical collapsing system. Furthermore we examine the cluster number counts dependence on the interaction between dark sectors and analyze how dark energy inhomogeneities affect cluster abundances. It is shown that cluster number counts can provide specific signature of dark sectors interaction and dark energy inhomogeneities. Natural Science Foundation of China (NSFC) NNSF Natural Science Foundation of China National Basic Research Program of China National Basic Research Program of China[2010CB833000] brazilian foundation CNPq Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) brazilian foundation FAPESP |
Identificador |
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, n.12, 2010 1475-7516 http://producao.usp.br/handle/BDPI/29254 10.1088/1475-7516/2010/12/022 |
Idioma(s) |
eng |
Publicador |
IOP PUBLISHING LTD |
Relação |
Journal of Cosmology and Astroparticle Physics |
Direitos |
restrictedAccess Copyright IOP PUBLISHING LTD |
Palavras-Chave | #cluster counts #dark energy theory #HUBBLE-SPACE-TELESCOPE #LARGE-SCALE STRUCTURE #OBSERVATIONAL CONSTRAINTS #COSMOLOGICAL PARAMETERS #NUMBER COUNTS #ENERGY MODELS #MATTER #SUPERNOVAE #DISCOVERIES #PRINCIPLE #Astronomy & Astrophysics #Physics, Particles & Fields |
Tipo |
article original article publishedVersion |