Generalised mass variation formula for a stationary axisymmetric star or black hole with surrounding accretion disc

Details Generalised mass variation formula for a stationary axisymmetric star or black hole with surrounding accretion disc Generalised mass variation formula for a stationary axisymmetric star or black hole with surrounding accretion disc

2002-06-07

arxiv.org/abs/astro-ph/0206113v1

Astronomy and Astrophysics

Astrophysics

11 pages, Tex version of manuscript originally distributed with restricted circulation in Journees Relativistes, 1979, ed. I.

Scientific paper

The general relativistic mass-energy variation formula for axisymmetric
equilibrium states of a selfgravitating system is developed in the particular
case for which the relevant matter consists of a perfectly conducting
multiconstituent fluid (or superfluid) with stationary circular or convective
motion.

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