Homogeneous cosmological model in general scalar-tensor theory

Details Homogeneous cosmological model in general scalar-tensor theory Homogeneous cosmological model in general scalar-tensor theory

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981phrvd..23.2111b&link_type=abstract

Physical Review D (Particles and Fields), Volume 23, Issue 10, 15 May 1981, pp.2111-2115

Mathematics

Logic

10

Scientific paper

Some general results on spatially homogeneous cosmological models are obtained in the general scalar-tensor theory proposed by Nordtvedt and Barker. Cosmological equations for a Bianchi type-I empty universe are solved and the behavior of the model is discussed. It is found that the universe expands from the initial singularity of zero volume and then contracts back. There is a significant difference between the nature of the singularity in this model and that in the corresponding Kasner universe in Einstein's theory.

Affiliated with

Also associated with

No associations

Rating

Homogeneous cosmological model in general scalar-tensor theory 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 Homogeneous cosmological model in general scalar-tensor theory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Homogeneous cosmological model in general scalar-tensor theory will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1442911