COBE- and Cluster-Normalized CDM Simulations

Simple item page
dc.creatorPiran, Tsvi
dc.creatorEl-Ad, Hagai
dc.creatorMartel, Hugo
dc.creatorLecar, Myron
dc.date2000-07-05
dc.date.accessioned2026-07-07T01:54:16Z
dc.date.available2026-07-07T01:54:16Z
dc.descriptionWe introduce a set of four new publicly available N-body simulations, the most recent additions to the Texas P^3M Database. Our models probe the less studied parameter space region of moderate volume (100/h Mpc box) combined with fine mass resolution (~10^12 M_Sol, roughly comparable to a L_* galaxy), making these simulations especially suitable for study of major large-scale structure features such as voids, and for comparison with the largest three-dimensional redshift surveys currently available. Our cosmological models (LCDM, TOCDM, OCDM, TCDM) are all COBE-normalized, and when possible (LCDM and TOCDM) also cluster-normalized, based on the X-ray cluster M--T relation. The COBE- and cluster-normalized LCDM model reiterates the attractiveness of this currently favored model which does not require the introduction of tilt in order to fit the constraints imposed by observations of other cosmological parameters.
dc.descriptionProceedings of the XXXVth Rencontres de Moriond, Energy Densities in the Universe, Editions Frontieres; 4 pages, moriond LaTeX file using epsfig, 2 tables, 2 PS figures. Complete gzipped version is available at http://merger.fiz.huji.ac.il/~eladh
dc.identifierhttps://arxiv.org/abs/astro-ph/0007060
dc.identifierhttp://arxiv.org/abs/astro-ph/0007060
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1281
dc.subjectAstrophysics
dc.titleCOBE- and Cluster-Normalized CDM Simulations
dc.typetext

Files

Collections

arXiv