A Cosmological Mass Function with Broken Hierarchy

dc.creatorLee, Jounghun
dc.date2006-05-29
dc.date.accessioned2026-07-07T07:08:35Z
dc.date.available2026-07-07T07:08:35Z
dc.descriptionWe construct an analytic formalism for the mass function of cold dark matter halos, assuming that there is a break in the hierarchical merging process. According to this {\it broken-hierarchy} scenario, due to the inherent nature of the gravitational tidal field the formation of massive pancakes precedes that of dark halos of low-mass. In the framework of the Zel'dovich approximation which generically predicts the presence of pancakes, we first derive analytically the conditional probability that a low-mass halo observed at present epoch was embedded in an isolated pancake at some earlier epoch. Then, we follow the standard Press-Schechter approach to count analytically the number density of low-mass halos that formed through anti-hierarchical fragmentation of the massive pancakes. Our mass function is well approximated by a power-law dN/dM = M^{-l} in the mass range 10^{6}M_{sun}/h < M < 10^{10}M_{sun}/h with the slope l=1.86 shallower than that of the currently popular Sheth-Tormen mass function l = 2.1. It is expected that our mass function will provide a useful analytic tool for investigating the effect of broken hierarchy on the structure formation.
dc.descriptionsubmitted to ApJL, 11 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0605697
dc.identifierhttp://arxiv.org/abs/astro-ph/0605697
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/110763
dc.subjectAstrophysics
dc.titleA Cosmological Mass Function with Broken Hierarchy
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