Evolution of density and velocity inhomogeneities in Friedmann cosmologies

Details Evolution of density and velocity inhomogeneities in Friedmann cosmologies Evolution of density and velocity inhomogeneities in Friedmann cosmologies

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.205..543p&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 205, Nov. 1983, p. 543-558. Research supported by the B

Astronomy and Astrophysics

Astronomy

16

Big Bang Cosmology, Space Density, Universe, Density Distribution, Evolution (Development), Inhomogeneity, Milky Way Galaxy, Velocity Distribution, Voids

Scientific paper

The authors treat the evolution of density and velocity perturbations in a Friedmann universe, on the assumption of spherical symmetry. The initial density and velocity profiles are left arbitrary, and the various characteristics of the evolution are examined. In particular the authors examine the formation and evolution of large empty regions of the universe; and compare with the recently discovered voids in the galaxy distribution. An observational method for measuring the initial profiles is outlined.

Affiliated with

Also associated with

No associations

Rating

Evolution of density and velocity inhomogeneities in Friedmann cosmologies 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 Evolution of density and velocity inhomogeneities in Friedmann cosmologies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of density and velocity inhomogeneities in Friedmann cosmologies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1487389