Generalized Laplace Method for Simple Determination of Kerr-Newman Black Hole Horizon Radius

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dc.creatorPankovic, Vladan
dc.creatorCiganovic, Sima
dc.creatorIvanovic, Jovan
dc.date2008-11-26
dc.date.accessioned2026-07-07T12:04:45Z
dc.date.available2026-07-07T12:04:45Z
dc.descriptionIn this work we present a generalized Laplace method for a formal, simple, quasi-classical, determination of the outer and inner horizon radius of Kerr-Newman black hole. We consider classical gravitational interaction between a thin, with homogeneously distributed mass and electric charge, spherical (black) shell and a probe particle. Also, we use relativistic equivalence principle. Finally we suppose that probe particle propagates radially to shell with speed of light while tangentially it rotates in common with shell, so that total energy of a probe particle equals zero.
dc.description4 pages, no figures
dc.identifierhttps://arxiv.org/abs/0811.4297
dc.identifierhttp://arxiv.org/abs/0811.4297
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/208194
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGeneralized Laplace Method for Simple Determination of Kerr-Newman Black Hole Horizon Radius
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