Fermion Tunneling from Dynamical Horizons

dc.creatorDi Criscienzo, Roberto
dc.creatorVanzo, Luciano
dc.date2008-03-04
dc.date2008-03-07
dc.date.accessioned2026-07-07T11:48:53Z
dc.date.available2026-07-07T11:48:53Z
dc.descriptionThe instability against emission of fermionic particles by the trapping horizon of an evolving black hole is analyzed using the Hamilton-Jacobi tunneling method. This method automatically selects one special expression for the surface gravity of a changing horizon. The results also apply to point masses embedded in an expanding universe. As a bonus of the tunneling method, we gain the insight that the surface gravity still defines a temperature parameter as long as the evolution is sufficiently slow that the black hole pass through a sequence of quasi-equilibrium states, and that black holes should be semi-classically unstable even in a hypothetical world without bosonic fields.
dc.description8 pages, standard Latex document, few references added
dc.identifierhttps://arxiv.org/abs/0803.0435
dc.identifierhttp://arxiv.org/abs/0803.0435
dc.identifierEurophys.Lett.82:60001,2008
dc.identifierdoi:10.1209/0295-5075/82/60001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203040
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleFermion Tunneling from Dynamical Horizons
dc.typetext

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