Mass function of gravitationally bounded objects in the inhomogeneous Universe

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dc.creatorArhipova, N. A.
dc.creatorLukash, V. N.
dc.creatorKomberg, B. V.
dc.creatorMikheeva, E. V.
dc.date2003-03-26
dc.date.accessioned2026-07-07T02:08:06Z
dc.date.available2026-07-07T02:08:06Z
dc.descriptionWe modify the Press-Schechter formalism to calculate the mass function of gravitationally bounded objects in a local Universe with size $L> 10h^{-1}$Mpc, i.e. separately in voids ($Ω_{m,L}<Ω_m$) and superclusters ($Ω_{m,L}>Ω_m$). The dependence of the abundance of gravitationally bounded objects on local matter density is analyzed.
dc.description6 pages, 3 figures, proceedings of the 6rd International Conference on Cosmoparticle Physics "Cosmion-2001", oral report
dc.identifierhttps://arxiv.org/abs/astro-ph/0303572
dc.identifierhttp://arxiv.org/abs/astro-ph/0303572
dc.identifierGrav.Cosmol.Suppl. 8 (2002) 66-71
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5916
dc.subjectAstrophysics
dc.titleMass function of gravitationally bounded objects in the inhomogeneous Universe
dc.typetext

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