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Astron. Astrophys. 325, 439-449


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Non-linear dynamics and mass function of cosmic structures

I. Analytical results

Edouard Audit1, Romain Teyssier2, and Jean-Michel Alimi1

1 Laboratoire d'Astrophysique Extragalactique et de Cosmologie, Observatoire de Paris-Meudon, F-92195 Meudon Cedex, France
2 CEA, DSM/DAPNIA/Service d'Astrophysique CE-SACLAY, F-91191 Gif-sur-Yvette, France

Received 5 February 1997 / Accepted 28 March 1997

Abstract

We investigate some modifications to the Press & Schechter (1974) (PS) prescription resulting from shear and tidal effects. These modifications rely on more realistic treatments of the collapse process than the standard approach based on the spherical model.

First, we show that the mass function resulting from a new approximate Lagrangian dynamic (Audit & Alimi 1996), contains more objects at high mass, than the classical PS mass function and is well fitted by a PS-like function with a threshold density of FORMULA . However, such a Lagrangian description can underestimate the epoch of structure formation since it defines it as the collapse of the first principal axis. We therefore suggest some analytical prescriptions, for computing the collapse time along the second and third principal axes, and we deduce the corresponding mass functions. The collapse along the third axis is delayed by the shear and the number of objects of high mass then decreases.

Finally, we show that the shear also strongly affects the formation of low-mass halos. This dynamical effect implies a modification of the low-mass slope of the mass function and allows the reproduction of the observed luminosity function of field galaxies. In a companion paper, we present results of numerical simulations which complete this work.

Key words: cosmology: theory - gravitation - large-scale structure of universe


© European Southern Observatory (ESO) 1997

Online publication: September 9, 1997
Last change: April 28, 1998
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