The imprint of the interaction between dark sectors in galaxy clusters


Autoria(s): HE, Jian-Hua; WANG, Bin; Abdalla, Elcio; PAVON, Diego
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

20/10/2012

20/10/2012

2010

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

http://dx.doi.org/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