Thermodynamics, topology and dimension of initial real tunneling manifolds

dc.creatorRosales, Jose-Luis
dc.date1997-12-12
dc.date.accessioned2026-07-07T03:32:06Z
dc.date.available2026-07-07T03:32:06Z
dc.descriptionWe develop the argument that initial real tunneling in quantum gravity be contemplated as a thermodynamical analogous to a black hole condensate in equilibrium with Hawking's radiation in a box. The total entropy is always maximized in the Lorentzian sector of the manifold, and, in this sense, tunneling is predicted.
dc.identifierhttps://arxiv.org/abs/gr-qc/9712059
dc.identifierhttp://arxiv.org/abs/gr-qc/9712059
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36103
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThermodynamics, topology and dimension of initial real tunneling manifolds
dc.typetext

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