Galaxy Formation in Anisotropic Cosmologies

Details Galaxy Formation in Anisotropic Cosmologies Galaxy Formation in Anisotropic Cosmologies

Aug 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972phrvd...6..969p&link_type=abstract

Physical Review D, vol. 6, Issue 4, pp. 969-983

Other

34

Scientific paper

We analyze the growth rates of perturbations of the generic dust-filled Bianchi type-I cosmology (which exhibits anisotropy but not rotation). Anisotropy induces coupling between gravitational wave and density modes and can enhance the power-law rate of growth of the density perturbations. A maximum growth rate for pregalaxy perturbations is t83 (where t is cosmic time), so that no conclusive solution to the galaxy formation problem is found. The detailed structure of the flow of energy between gravitational wave and density modes and of the growth of rotational modes (decoupled from other perturbations) is presented. We also give a detailed discussion of the gauge-invariance properties of these perturbations.

Affiliated with

Also associated with

No associations

Rating

Galaxy Formation in Anisotropic 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 Galaxy Formation in Anisotropic Cosmologies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Galaxy Formation in Anisotropic Cosmologies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-873025