Stationary axisymmetric perfect fluid solutions in general relativity.

Details Stationary axisymmetric perfect fluid solutions in general relativity. Stationary axisymmetric perfect fluid solutions in general relativity.

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988gregr..20..635h&link_type=abstract

General Relativity and Gravitation, Volume 20, Issue 7, pp.635-646

Physics

18

General Relativity, Relativistic Fluids

Scientific paper

A new class of exact solutions of Einstein's field equations with the energy-momentum tensor of a perfect fluid is given. The class of solutions is invariantly characterized by means of the following properties: (i) The energy-momentum tensor describes a perfect fluid. (ii) There are two commuting Killing vectors ξ andη which form an abelian groupG 2 of motion. (iii) There is a timelike Killing vector parallel to the four-velocity of the fluid (rigid rotation of the fluid). (iv) The four-vector of the angular velocity of the fluid is a gradient ? i=-(1/4c)ɛirklUl (Ur:k-Uk:r)=χ' i. The last assumption is the reason that all solutions of this class can be found by solving an ordinary differential equation of the second order.

Affiliated with

Also associated with

No associations

Rating

Stationary axisymmetric perfect fluid solutions in general relativity. 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 axisymmetric perfect fluid solutions in general relativity., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stationary axisymmetric perfect fluid solutions in general relativity. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1423146