Nonlocal black-hole thermodynamics and massive remnants

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dc.creatorNikolic, H.
dc.date2006-07-20
dc.date.accessioned2026-07-07T07:16:52Z
dc.date.available2026-07-07T07:16:52Z
dc.descriptionTo alleviate the black-hole (BH) information problem, we study a holographic-principle-inspired nonlocal model of Hawking radiation in which radiated particles created at different times all have the same temperature corresponding to the instantaneous BH mass. Consequently, the black hole loses mass not only by continuously radiating new particles, but also by continuously warming previously radiated particles. The conservation of energy implies that the radiation stops when the mass of the black hole reaches the half of the initial BH mass, leaving a massive BH remnant with a mass much above the Planck scale.
dc.description7 pages, 1 figure included
dc.identifierhttps://arxiv.org/abs/hep-th/0607140
dc.identifierhttp://arxiv.org/abs/hep-th/0607140
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/113741
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNonlocal black-hole thermodynamics and massive remnants
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