Near-Extreme Black Holes and the Universal Relaxation Bound

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dc.creatorHod, Shahar
dc.date2007-05-16
dc.date.accessioned2026-07-07T10:35:53Z
dc.date.available2026-07-07T10:35:53Z
dc.descriptionA fundamental bound on the relaxation time τof a perturbed thermodynamical system has recently been derived, τ\geq \hbar/πT, where $T$ is the system's temperature. We demonstrate analytically that black holes saturate this bound in the extremal limit and for large values of the azimuthal number m of the perturbation field.
dc.description2 Pages. Submitted to PRD on 5/12/2007
dc.identifierhttps://arxiv.org/abs/0705.2306
dc.identifierhttp://arxiv.org/abs/0705.2306
dc.identifierClass.Quant.Grav.24:4235-4238,2007
dc.identifierdoi:10.1088/0264-9381/24/16/N01
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179872
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleNear-Extreme Black Holes and the Universal Relaxation Bound
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