Einstein's Field Equations for the Interior of a Uniformly Rotating Stationary Axisymmetric Perfect Fluid

Details Einstein's Field Equations for the Interior of a Uniformly Rotating Stationary Axisymmetric Perfect Fluid Einstein's Field Equations for the Interior of a Uniformly Rotating Stationary Axisymmetric Perfect Fluid

2001-02-02

arxiv.org/abs/gr-qc/0102005v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Scientific paper

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 $\mu$.

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