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Verfasst von:Meyer, Sven [VerfasserIn]   i
 Pace, Francesco [VerfasserIn]   i
 Bartelmann, Matthias [VerfasserIn]   i
Titel:Relativistic virialization in the spherical collapse model for Einstein-de Sitter and \Lambda CDM cosmologies
Verf.angabe:Sven Meyer, Francesco Pace, Matthias Bartelmann
Fussnoten:Gesehen am 21.09.2017
Titel Quelle:Enthalten in: De.arxiv.org
Jahr Quelle:2012
Band/Heft Quelle:(2012) Artikel-Nummer 1206.0618, 15 Seiten
Abstract:Spherical collapse has turned out to be a successful semi-analytic model to study structure formation in different DE models and theories of gravity. Nevertheless, the process of virialization is commonly studied on the basis of the virial theorem of classical mechanics. In the present paper, a fully generally-relativistic virial theorem based on the Tolman-Oppenheimer-Volkoff (TOV) solution for homogeneous, perfect-fluid spheres is constructed for the Einstein-de Sitter and \Lambda CDM cosmologies. We investigate the accuracy of classical virialization studies on cosmological scales and consider virialization from a more fundamental point of view. Throughout, we remain within general relativity and the class of FLRW models. The virialization equation is set up and solved numerically for the virial radius, y_{vir}, from which the virial overdensity \Delta_{V} is directly obtained. Leading order corrections in the post-Newtonian framework are derived and quantified. In addition, problems in the application of this formalism to dynamical DE models are pointed out and discussed explicitly. We show that, in the weak field limit, the relative contribution of the leading order terms of the post-Newtonian expansion are of the order of 10^{-3}% and the solution of Wang & Steinhardt (1998) is precisely reproduced. Apart from the small corrections, the method could provide insight into the process of virialization from a more fundamental point of view.
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Kostenfrei: Verlag: http://arxiv.org/abs/1206.0618
Datenträger:Online-Ressource
Sprache:eng
K10plus-PPN:1563690586
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