Separating expansion from contraction: generalized TOV condition, LTB
models with pressure and $Łambda$CDM
M. Delliou, F. Mena, and J. Mimoso. (2009)cite arxiv:0911.0241
Comment: Proceedings of 'Invisible Universe International Conference', Paris,
June 29- July 3, 2009 ; 5pp, 4 figs.
Abstract
We discuss the existence of a dividing shell separating expanding and
collapsing regions in spherically symmetric solutions with pressure. We obtain
gauge invariant conditions relating not only the intrinsic spatial curvature of
the shells to the ADM mass, but also a function of the pressure which we
introduce that generalises the Tolman-Oppenheimer-Volkoff equilibrium
condition, in the framework of a 3+1 spacetime splitting. We consider the
particular case of a Lemaître-Tolman-Bondi dust models with a cosmological
constant (a $Łambda$-CDM model) as an example of our results.
Description
Separating expansion from contraction: generalized TOV condition, LTB
models with pressure and $\Lambda$CDM
%0 Generic
%1 Delliou2009
%A Delliou, Morgan Le
%A Mena, Filipe C.
%A Mimoso, José Pedro
%D 2009
%K LCDM LTB
%T Separating expansion from contraction: generalized TOV condition, LTB
models with pressure and $Łambda$CDM
%U http://arxiv.org/abs/0911.0241
%X We discuss the existence of a dividing shell separating expanding and
collapsing regions in spherically symmetric solutions with pressure. We obtain
gauge invariant conditions relating not only the intrinsic spatial curvature of
the shells to the ADM mass, but also a function of the pressure which we
introduce that generalises the Tolman-Oppenheimer-Volkoff equilibrium
condition, in the framework of a 3+1 spacetime splitting. We consider the
particular case of a Lemaître-Tolman-Bondi dust models with a cosmological
constant (a $Łambda$-CDM model) as an example of our results.
@misc{Delliou2009,
abstract = { We discuss the existence of a dividing shell separating expanding and
collapsing regions in spherically symmetric solutions with pressure. We obtain
gauge invariant conditions relating not only the intrinsic spatial curvature of
the shells to the ADM mass, but also a function of the pressure which we
introduce that generalises the Tolman-Oppenheimer-Volkoff equilibrium
condition, in the framework of a 3+1 spacetime splitting. We consider the
particular case of a Lema\^itre-Tolman-Bondi dust models with a cosmological
constant (a $\Lambda$-CDM model) as an example of our results.
},
added-at = {2010-04-21T17:24:44.000+0200},
author = {Delliou, Morgan Le and Mena, Filipe C. and Mimoso, José Pedro},
biburl = {https://www.bibsonomy.org/bibtex/2d08454d86a429957268709e66be552f3/ad4},
description = {Separating expansion from contraction: generalized TOV condition, LTB
models with pressure and $\Lambda$CDM},
interhash = {70bdde7c21f5acf3b7174fa58cf7f898},
intrahash = {d08454d86a429957268709e66be552f3},
keywords = {LCDM LTB},
note = {cite arxiv:0911.0241
Comment: Proceedings of 'Invisible Universe International Conference', Paris,
June 29- July 3, 2009 ; 5pp, 4 figs},
timestamp = {2010-04-21T17:24:44.000+0200},
title = {{S}eparating expansion from contraction: generalized {TOV} condition, {LTB}
models with pressure and $\Lambda$CDM},
url = {http://arxiv.org/abs/0911.0241},
year = 2009
}