Cavity evolution in relativistic self-gravitating fluids

Details Cavity evolution in relativistic self-gravitating fluids Cavity evolution in relativistic self-gravitating fluids

2010-04-09

arxiv.org/abs/1004.1490v1

Class.Quantum.Grav.27:135017,2010

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

10 pages Revtex. To appear in Class. Quantum Grav.

Scientific paper

We consider the evolution of cavities within spherically symmetric relativistic fluids, under the assumption that proper radial distance between neighboring fluid elements remains constant during their evolution (purely areal evolution condition). The general formalism is deployed and solutions are presented. Some of them satisfy Darmois conditions whereas others present shells and must satisfy Israel conditions, on either one or both boundary surfaces. Prospective applications of these results to some astrophysical scenarios is suggested.

Affiliated with

Also associated with

No associations

Rating

Cavity evolution in relativistic self-gravitating fluids 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 Cavity evolution in relativistic self-gravitating fluids, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cavity evolution in relativistic self-gravitating fluids will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-220867