Two Topics concerning Black Holes: Extremality of the Energy, Fractality of the Horizon

dc.creatorSorkin, Rafael D.
dc.date1995-08-02
dc.date.accessioned2026-07-07T03:30:46Z
dc.date.available2026-07-07T03:30:46Z
dc.descriptionWe treat two aspects of the physics of stationary black holes. First we prove that the proportionality, d(energy) ~ d(area) for arbitrary perturbations (``extended first law''), follows directly from an extremality theorem drawn from earlier work. Second we consider quantum fluctuations in the shape of the horizon, concluding heuristically that they exhibit a fractal character, with order lambda fluctuations occurring on all scales lambda below M^{1/3} in natural units.
dc.description18 pages, plainTeX, 2 postscript figures (Figures for automatic inclusion are in a separate file which you should receive with the .tex file. For instructions on decoding and including them (or omitting them to avoid error messages if your system can't handle them) see the box at the beginning of the tex file for this paper.)
dc.identifierhttps://arxiv.org/abs/gr-qc/9508002
dc.identifierhttp://arxiv.org/abs/gr-qc/9508002
dc.identifierin Proceedings of the Conference on Heat Kernel Techniques and Quantum Gravity, held Winnipeg, Canada, August, 1994 (Discourses in Mathematics and its Applications, \#4) edited by S.A. Fulling, pp. 387-407 (University of Texas Press, 1995)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35637
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleTwo Topics concerning Black Holes: Extremality of the Energy, Fractality of the Horizon
dc.typetext

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