Einstein's Field Equations for the Interior of a Uniformly Rotating Stationary Axisymmetric Perfect Fluid
Abstract
We reduce Einstein's field equations for the interior of a uniformly rotating, axisymmetric perfect fluid to a system of six second order partial differential equations for the pressure p the energy density $\mu$ and four dependent variables.Four of these equations do not depend on p and $\mu$ and the other two determine p and $\mu$.
 Publication:

arXiv eprints
 Pub Date:
 February 2001
 arXiv:
 arXiv:grqc/0102005
 Bibcode:
 2001gr.qc.....2005K
 Keywords:

 General Relativity and Quantum Cosmology