2002A&A...387..759D


Query : 2002A&A...387..759D

2002A&A...387..759D - Astronomy and Astrophysics, volume 387759-777 (2002/6-1)

On the evolution of aspherical perturbations in the universe: An analytical model.

DEL POPOLO A.

Abstract (from CDS):

I study the role of shear fields on the evolution of density perturbations by using an analytical approximate solution for the equations of motion of homogeneous ellipsoids embedded in a homogeneous background. The equations of motion of a homogeneous ellipsoid (Icke, 1973A&A....27....1I; White & Silk, 1979ApJ...231....1W, hereafter WS) are modified in order to take account of the tidal field, as done in Watanabe (1993PASJ...45..393W) and then are integrated analytically, similar to what was done in WS. The comparison of the analytical solution with numerical simulations shows that it is a good approximation of the numerical one. This solution is used to study the evolution of the configuration of the ellipsoids, to calculate the evolution of the density contrast and that of the axial peculiar velocity of the ellipsoids for several values of the amplitude of the external tidal field, and is compared again with numerical simulations. In order to calculate the evolution of the density contrast at turn-around and collapse velocity at the epoch of collapse, as a function of the ratio of the initial value of the semi-axes, I use the previously-obtained approximate solution to modify the analytical model proposed by Barrow & Silk (1981ApJ...250..432B) for the ellipsoid evolution in the non-linear regime. The density contrast at turn-around and the collapse velocity are found to be reduced with respect to that found by means of the spherical model. The reduction increases with increasing strength of the external tidal field and with increasing initial asymmetry of the ellipsoids. These last calculations are also compared with numerical solutions and they are again in good agreement with the numerical ones.

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Journal keyword(s): cosmology: theory - large-scale structure of Universe - galaxies: formation

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Local Supercluster SCG 12 31 +12.4           ~ 566 0

Query : 2002A&A...387..759D

Basic data :
NAME Local Supercluster -- Supercluster of Galaxies
Other object types:
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SCG ()
ICRS coord. (ep=J2000) :
12 31 00.0 +12 24 00 [ ] E ~
FK4 coord. (ep=B1950 eq=1950) :
12 28 28.2 +12 40 34 [ ]
Gal coord. (ep=J2000) :
283.9216 +74.5125 [ ]
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Hierarchy : number of linked objects
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Identifiers (6) :
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NAME LOCAL SUPERCL NAME VIRGO SUPERCL NAME Vir Supercluster
NAME LSC NAME Local Supercluster NAME Virgo Supercluster

References (566 between 1850 and 2026) (Total 566)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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