You are in the accessibility menu

Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/65552
Full metadata record
DC FieldValueLanguage
dc.contributor.authorHiguchi, Atsushi-
dc.contributor.authorMatsas, George E. A.-
dc.contributor.authorSudarsky, Daniel-
dc.date.accessioned2014-05-27T11:19:38Z-
dc.date.accessioned2016-10-25T18:15:19Z-
dc.date.available2014-05-27T11:19:38Z-
dc.date.available2016-10-25T18:15:19Z-
dc.date.issued1998-11-15-
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.58.104021-
dc.identifier.citationPhysical Review D - Particles, Fields, Gravitation and Cosmology, v. 58, n. 10, p. 1040211-10402110, 1998.-
dc.identifier.issn0556-2821-
dc.identifier.urihttp://hdl.handle.net/11449/65552-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/65552-
dc.description.abstractWe show that the response rate of (i) a static source interacting with Hawking radiation of a massless scalar field in Schwarzschild spacetime (with the Unruh vacuum) and that of (ii) a uniformly accelerated source with the same proper acceleration in Minkowski spacetime (with the Minkowski vacuum) are equal. We show that this equality will not hold if the Unruh vacuum is replaced by the Hartle-Hawking vacuum. It is verified that the source responds to the Hawking radiation near the horizon as if it were at rest in a thermal bath in Minkowski spacetime with the same temperature. It is also verified that the response rate in the Hartle-Hawking vacuum approaches that in Minkowski spacetime with the same temperature far away from the black hole. Finally, we compare our results with others in the literature.en
dc.format.extent1040211-10402110-
dc.language.isoeng-
dc.sourceScopus-
dc.titleInteraction of Hawking radiation with static sources outside a Schwarzschild black holeen
dc.typeoutro-
dc.contributor.institutionUniversität Bern-
dc.contributor.institutionUniversity of York-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.contributor.institutionUniv. Nac. Auton. de México-
dc.description.affiliationInst. für Theoretische Physik Universität Bern, Sidlerstrasse 5, CH-3012 Bern-
dc.description.affiliationDepartment of Mathematics University of York, Heslington, York YO10 5DD-
dc.description.affiliationInst. de Fis. Teórica Universidade Estadual Paulista, Rua Pamplona 145, 01405-900-São Paulo-
dc.description.affiliationInstituto de Ciencias Nucleares Univ. Nac. Auton. de México, A. Postal 70/543, Mexico D.F. 04510-
dc.description.affiliationUnespInst. de Fis. Teórica Universidade Estadual Paulista, Rua Pamplona 145, 01405-900-São Paulo-
dc.identifier.doi10.1103/PhysRevD.58.104021-
dc.identifier.wosWOS:000077106900047-
dc.rights.accessRightsAcesso aberto-
dc.identifier.file2-s2.0-1542420420.pdf-
dc.relation.ispartofPhysical Review D: Particles, Fields, Gravitation and Cosmology-
dc.identifier.scopus2-s2.0-1542420420-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

There are no files associated with this item.
 

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.