Relativistic perfect fluid models

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

10 pages, Presented at the Journees Relativistes 1999, Weimar (September 12-17)

Scientific paper

10.1002/(SICI)1521-3889(200005)9

The various schemes for studying rigidly rotating perfect fluids in general relativity are reviewed. General conclusions one may draw from these are: (i) There is a need to restrict the scope of the possible ansatze, and (ii) the angular behaviour is a valuable commodity. This latter observation follows from a large number of analytic models exhibiting a NUT-like behaviour. A method of getting around problem (ii) is presented on a simple example. To alleviate problem (i) for rigidly rotating perfect fluids, approximation schemes based on a series expansion in the angular velocity are suggested. A pioneering work, due to Hartle, explores the global properties of matched space-times to quadratic order in the angular velocity. As a first example of the applications, it is shown that the rigidly rotating incompressible fluid cannot be Petrov type D.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Relativistic perfect fluid models 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 Relativistic perfect fluid models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Relativistic perfect fluid models will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-97303

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.