Structure formation in the quasispherical Szekeres model

Details Structure formation in the quasispherical Szekeres model Structure formation in the quasispherical Szekeres model

2006-04-24

arxiv.org/abs/astro-ph/0604490v2

Phys.Rev.D73:123508,2006

Astronomy and Astrophysics

Astrophysics

11 pages, 14 figures; changes after referee comments; accepted for publication in Physical Review D15

Scientific paper

10.1103/PhysRevD.73.123508

Structure formation in the Szekeres model is investigated. Since the Szekeres model is an inhomogeneous model with no symmetries, it is possible to examine the interaction of neighboring structures and its impact on the growth of a density contrast. It has been found that the mass flow from voids to clusters enhances the growth of the density contrast. In the model presented here, the growth of the density contrast is almost 8 times faster than in the linear approach.

Affiliated with

Also associated with

No associations

Rating

Structure formation in the quasispherical Szekeres model does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Structure formation in the quasispherical Szekeres model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure formation in the quasispherical Szekeres model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-582688