Evolution of spherical non-uniform perturbations in the universe
| Contribuinte(s) |
Universidade Estadual Paulista (UNESP) |
|---|---|
| Data(s) |
30/09/2013
20/05/2014
30/09/2013
20/05/2014
01/11/2010
|
| Resumo |
Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES) Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) We study the evolution of inhomogeneous spherical perturbations in the universe in a way that generalizes the spherical top-hat collapse in a straightforward manner. For that purpose we will derive a dynamical equation for the density contrast in the context of a Lemaitre-Tolman-Bondi metric and construct solutions with and without a cosmological constant for the evolution of a spherical perturbation with a given initial radial profile. Copyright (C) EPLA, 2010 |
| Formato |
6 |
| Identificador |
http://dx.doi.org/10.1209/0295-5075/92/39001 Epl. Mulhouse: Epl Association, European Physical Society, v. 92, n. 3, p. 6, 2010. 0295-5075 http://hdl.handle.net/11449/24297 10.1209/0295-5075/92/39001 WOS:000284996700040 |
| Idioma(s) |
eng |
| Publicador |
Epl Association, European Physical Society |
| Relação |
EPL |
| Direitos |
closedAccess |
| Tipo |
info:eu-repo/semantics/conferenceObject |
