Closure in anisotropic cosmological models

Details Closure in anisotropic cosmological models Closure in anisotropic cosmological models

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977jmp....18..250g&link_type=abstract

Journal of Mathematical Physics, Volume 18, Issue 2, pp. 250-252 (1977).

Mathematics

Mathematical Physics

Cosmology

Scientific paper

The closure result of Friedmann cosmology is briefly reviewed. A new closure result is presented for nonrotating, dust filled, but otherwise anisotropic, inhomogeneous cosmological models. The isotropy assumptions are replaced by much milder physical assumptions while the crucial Friedmann condition, 8πκρ-3h2>~0, is replaced by the only slightly stronger 4πκρ-3h2>~0.

Affiliated with

Also associated with

No associations

Rating

Closure in anisotropic cosmological models 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 Closure in anisotropic cosmological models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Closure in anisotropic cosmological models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-800263