The galaxy halo formation rate

The rate at which galaxy halos form is thought to play a key role in explaining many observable cosmological phenomena such as the initial epoch at which luminous matter forms and the distribution of active galaxies. Here we show how Press-Schechter theory can be used to provide a simple, completely...

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Main Authors: Percival, W, Miller, L
Format: Journal article
Published: 1998
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author Percival, W
Miller, L
author_facet Percival, W
Miller, L
author_sort Percival, W
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description The rate at which galaxy halos form is thought to play a key role in explaining many observable cosmological phenomena such as the initial epoch at which luminous matter forms and the distribution of active galaxies. Here we show how Press-Schechter theory can be used to provide a simple, completely analytic model of the halo formation rate. This model shows good agreement with both Monte-Carlo and N-body simulation results.
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spelling oxford-uuid:c92a4e36-e13d-4683-8758-320d70ef0e422022-03-27T06:57:03ZThe galaxy halo formation rateJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:c92a4e36-e13d-4683-8758-320d70ef0e42Symplectic Elements at Oxford1998Percival, WMiller, LThe rate at which galaxy halos form is thought to play a key role in explaining many observable cosmological phenomena such as the initial epoch at which luminous matter forms and the distribution of active galaxies. Here we show how Press-Schechter theory can be used to provide a simple, completely analytic model of the halo formation rate. This model shows good agreement with both Monte-Carlo and N-body simulation results.
spellingShingle Percival, W
Miller, L
The galaxy halo formation rate
title The galaxy halo formation rate
title_full The galaxy halo formation rate
title_fullStr The galaxy halo formation rate
title_full_unstemmed The galaxy halo formation rate
title_short The galaxy halo formation rate
title_sort galaxy halo formation rate
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