Stationary circularly symmetric 2+1 rigidly rotating perfect fluids

Details Stationary circularly symmetric 2+1 rigidly rotating perfect fluids Stationary circularly symmetric 2+1 rigidly rotating perfect fluids

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004phrvd..69l4024g&link_type=abstract

Physical Review D, vol. 69, Issue 12, id. 124024

Mathematics

Logic

1

Exact Solutions, Gravity In More Than Four Dimensions, Kaluza-Klein Theory, Unified Field Theories, Alternative Theories Of Gravity

Scientific paper

The general solution for a stationary circularly symmetric metric ds2=-N(r)2dt2+dr2/F(r)2+r2[dφ-J/(2r2)dt]2, coupled to a rigidly rotating perfect fluid and a cosmological constant, is determined through an arbitrarily given function N(r), which allows the evaluation of the structural function F(r), the energy density, and the isotropic pressure. The interior solution with a constant energy density can be matched to the BTZ black hole.

Affiliated with

Also associated with

No associations

Rating

Stationary circularly symmetric 2+1 rigidly rotating perfect 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 Stationary circularly symmetric 2+1 rigidly rotating perfect fluids, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stationary circularly symmetric 2+1 rigidly rotating perfect fluids will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1394409