Quantum Black Hole

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dc.creatorChao, Wu Zhong
dc.date1998-08-13
dc.date.accessioned2026-07-07T03:32:36Z
dc.date.available2026-07-07T03:32:36Z
dc.descriptionCreation of a black hole in quantum cosmology is the third way of black hole formation. In contrast to the gravitational collapse from a massive body in astrophysics or from the quantum fluctuation of matter fields in the very early universe, in quantum cosmology scenario the black hole is essentially created from nothing. The black hole originates from a constrained gravitational instanton. The probability of creation for all kinds of single black holes in the Kerr- Newman-de Sitter family, at the semi-classical level, is the exponential of the total entropy of the universe, or one quarter of the sum of both the black hole and the cosmological horizon areas. The de Sitter spacetime is the most probable evolution at the Planckian era.
dc.description8 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/9808038
dc.identifierhttp://arxiv.org/abs/gr-qc/9808038
dc.identifierGen.Rel.Grav. 30 (1998) 115
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36293
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleQuantum Black Hole
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