Generalised mass variation formula for a stationary axisymmetric star or black hole with surrounding accretion disc
Abstract
Description
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.
11 pages, Tex version of manuscript originally distributed with restricted circulation in Journees Relativistes, 1979, ed. I. Moret-Bailly, C. Latremoliere, pp 166-182 (Faculte des Sciences, Angers, 1979)
11 pages, Tex version of manuscript originally distributed with restricted circulation in Journees Relativistes, 1979, ed. I. Moret-Bailly, C. Latremoliere, pp 166-182 (Faculte des Sciences, Angers, 1979)