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

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dc.creatorCarter, Brandon
dc.date2002-06-07
dc.date.accessioned2026-07-07T02:03:54Z
dc.date.available2026-07-07T02:03:54Z
dc.descriptionThe 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.
dc.description11 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)
dc.identifierhttps://arxiv.org/abs/astro-ph/0206113
dc.identifierhttp://arxiv.org/abs/astro-ph/0206113
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4554
dc.subjectAstrophysics
dc.titleGeneralised mass variation formula for a stationary axisymmetric star or black hole with surrounding accretion disc
dc.typetext

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