Reconsidering the black hole final state in Dirac fields

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dc.creatorGe, Xian-Hui
dc.creatorShen, You-Gen
dc.date2005-01-18
dc.date.accessioned2026-07-07T10:50:30Z
dc.date.available2026-07-07T10:50:30Z
dc.descriptionWe extend Horowitz and Maldacena's proposal about black hole final state to Dirac fields and find that if annihilation of the infalling positrons and the collapsed electrons inside the horizon is considered, then the nonlinear evolution of collapsing quantum state will be avoided. We further propose that annihilation also plays the central role in the process of black hole information escaping in both Dirac and scalar fields. The computation speed of a black hole is also briefly discussed.
dc.description7pages; Phys. Lett. B 2005 (in press)
dc.identifierhttps://arxiv.org/abs/hep-th/0501131
dc.identifierhttp://arxiv.org/abs/hep-th/0501131
dc.identifierPhys.Lett.B612:61-64,2005
dc.identifierdoi:10.1016/j.physletb.2005.02.050
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/184555
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleReconsidering the black hole final state in Dirac fields
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