Growth of large-scale structure with a cosmological constant

Details Growth of large-scale structure with a cosmological constant Growth of large-scale structure with a cosmological constant

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.262..717b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 262, no. 3, p. 717-725.

Statistics

Computation

14

Cosmology, Evolution (Development), Universe, Computational Astrophysics, Density Distribution, Inhomogeneity

Scientific paper

Effects of a non-zero cosmological constant, Lambda, upon the growth, collapse, and virialization of spherical and nonspherical density inhomogeneities in the postrecombination universe are calculated. The growth that results is compared with that in the absence of the Lambda term. In the evolution of the velocity field a competition is seen between pure adiabatic decay of the velocity, v varies as a exp -1, and the growth of velocities induced by the growing density perturbations. The formation of flattened 'pancakes' is studied, and the turnaround times together with the density contrast required for the collapse of different axes are derived.

Affiliated with

Also associated with

No associations

Rating

Growth of large-scale structure with a cosmological constant 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 Growth of large-scale structure with a cosmological constant, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Growth of large-scale structure with a cosmological constant will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1334978