arXiv Analytics

Sign in

arXiv:gr-qc/0101072AbstractReferencesReviewsResources

Some results on the integrability of Einstein's field equations for axistationary perfect fluids

M. Bradley, G. Fodor, M. Marklund, Z. Perjes

Published 2001-01-17Version 1

Using an orthonormal Lorentz frame approach to axistationary perfect fluid spacetimes, we have formulated the necessary and sufficient equations as a first order system, and investigated the integrability conditions of this set of equations. The integrability conditions are helpful tools when it comes to check the consequences and/or compatibility of certain simplifying assumptions, e.g. Petrov types. Furthermore, using this method, a relation between the fluid shear and vorticity is found for barotropic fluids. We collect some results concerning Petrov types, and it is found that an incompressible axistationary perfect fluid must be of Petrov type I.

Comments: 2 pages, contribution to the 9th Marcel Grossmann meeting (MG9), Rome, July 2000
Categories: gr-qc
Related articles: Most relevant | Search more
arXiv:1306.6204 [gr-qc] (Published 2013-06-26, updated 2014-05-22)
Conformally covariant systems of wave equations and their equivalence to Einstein's field equations
arXiv:gr-qc/0703129 (Published 2007-03-26, updated 2007-04-30)
Improved outer boundary conditions for Einstein's field equations
arXiv:gr-qc/0111008 (Published 2001-11-02, updated 2001-12-11)
An Online Interactive Geometric Database: Including Exact Solutions of Einstein's Field Equations