From Euclidean to Lorentzian General Relativity: The Real Way

dc.creatorG., J. Fernando Barbero
dc.date1996-05-29
dc.date1996-06-05
dc.date.accessioned2026-07-07T12:01:23Z
dc.date.available2026-07-07T12:01:23Z
dc.descriptionWe study in this paper a new approach to the problem of relating solutions to the Einstein field equations with Riemannian and Lorentzian signatures. The procedure can be thought of as a "real Wick rotation". We give a modified action for general relativity, depending on two real parameters, that can be used to control the signature of the solutions to the field equations. We show how this procedure works for the Schwarzschild metric and discuss some possible applications of the formalism in the context of signature change, the problem of time, black hole thermodynamics...
dc.description20 pages uuencoded gzipped tar format. Accepted in Phys. Rev. D. Some references added
dc.identifierhttps://arxiv.org/abs/gr-qc/9605066
dc.identifierhttp://arxiv.org/abs/gr-qc/9605066
dc.identifierPhys.Rev.D54:1492-1499,1996
dc.identifierdoi:10.1103/PhysRevD.54.1492
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/207081
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleFrom Euclidean to Lorentzian General Relativity: The Real Way
dc.typetext

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