Energy-momentum tensor for scalar fields coupled to the dilaton in two dimensions

dc.contributor.authorLombardo, Fernando C.cat
dc.contributor.authorMazzitelli, Francisco D.cat
dc.contributor.authorRusso, J. G. (Jorge Guillermo)cat
dc.date.accessioned2010-05-06T12:01:04Z
dc.date.available2010-05-06T12:01:04Z
dc.date.issued1999cat
dc.description.abstractWe clarify some issues related to the evaluation of the mean value of the energy-momentum tensor for quantum scalar fields coupled to the dilaton field in two-dimensional gravity. Because of this coupling, the energy-momentum tensor for matter is not conserved and therefore it is not determined by the trace anomaly. We discuss different approximations for the calculation of the energy-momentum tensor and show how to obtain the correct amount of Hawking radiation. We also compute cosmological particle creation and quantum corrections to the Newtonian potential.eng
dc.format.extent8 p.cat
dc.format.mimetypeapplication/pdfeng
dc.identifier.idgrec512100cat
dc.identifier.issn0556-2821cat
dc.identifier.urihttps://hdl.handle.net/2445/12471
dc.language.isoengeng
dc.publisherThe American Physical Societyeng
dc.relation.isformatofReproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.59.064007cat
dc.relation.ispartofPhysical Review D, 1999, vol. 59, núm. 6, p. 064007-1-064007-8cat
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevD.59.064007
dc.rights(c) The American Physical Society, 1999eng
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationRelativitat general (Física)cat
dc.subject.classificationGravitaciócat
dc.subject.otherGeneral relativity (Physics)eng
dc.subject.otherGravitationeng
dc.titleEnergy-momentum tensor for scalar fields coupled to the dilaton in two dimensionseng
dc.typeinfo:eu-repo/semantics/articleeng
dc.typeinfo:eu-repo/semantics/publishedVersion

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