Local approach to thermodynamics of black holes

dc.creatorCzuchry, E.
dc.creatorJezierski, J.
dc.creatorKijowski, J.
dc.date2004-05-14
dc.date.accessioned2026-07-07T03:28:41Z
dc.date.available2026-07-07T03:28:41Z
dc.descriptionHamiltonian description of gravitational field contained in a spacetime region with boundary $S$ being a null-like hypersurface (a wave front) is discussed. Complete generating formula for the Hamiltonian dynamics (with no surface integrals neglected) is presented. A quasi-local proof of the 1-st law of black holes thermodynamics is obtained as a consequence, in case when $S$ is a non-expanding horizon. The 0-th law and Penrose inequalities are discussed from this point of view.
dc.description10 pages, to appear in Proceedings of the Seventh Hungarian Relativity Workshop
dc.identifierhttps://arxiv.org/abs/gr-qc/0405073
dc.identifierhttp://arxiv.org/abs/gr-qc/0405073
dc.identifierin Relativity Today (Proc. 7th Hungarian Relativity Workshop, 2003) Ed. I. Racz, (Akadémiai Kiadó, Budapest, 2004)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34927
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleLocal approach to thermodynamics of black holes
dc.typetext

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