dc.contributorUniversidade Estadual Paulista (UNESP)
dc.creatorCastiñeiras, Jorge
dc.creatorCrispino, Luis C. B.
dc.creatorMatsas, George E. A.
dc.creatorVanzella, Daniel A. T.
dc.date2014-05-20T14:06:56Z
dc.date2016-10-25T21:21:03Z
dc.date2014-05-20T14:06:56Z
dc.date2016-10-25T21:21:03Z
dc.date2002-05-10
dc.date.accessioned2017-04-06T09:21:33Z
dc.date.available2017-04-06T09:21:33Z
dc.identifierPhysical Review D - Particles, Fields, Gravitation and Cosmology, v. 65, n. 10, p. 1040191-10401910, 2002.
dc.identifier0556-2821
dc.identifierhttp://hdl.handle.net/11449/130393
dc.identifierhttp://acervodigital.unesp.br/handle/11449/130393
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.65.104019
dc.identifierWOS:000175774200053
dc.identifier2-s2.0-0037053176
dc.identifierhttp://journals.aps.org/prd/abstract/10.1103/PhysRevD.65.104019
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/940936
dc.descriptionWe analyze free elementary particles with a rest mass m and total energy E<mc2 in the Rindler wedge, outside Reissner-Nordstrom black holes and in the spacetime of relativistic (and nonrelativistic) stars, and use Unruh-DeWitt-like detectors to calculate the associated particle detection rate in each case. The (mean) particle position is identified with the spatial average of the excitation probability of the detectors, which are supposed to cover the whole space. Our results are shown to be in harmony with general relativity classical predictions. Eventually we reconcile our conclusions with Earth-based experiments which are in good agreement with E ≥mc2.
dc.languageeng
dc.publisherAmerican Physical Soc
dc.relationPhysical Review D: Particles, Fields, Gravitation and Cosmology
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectCosmos
dc.subjectDispersion
dc.subjectParticle radiation
dc.subjectPrediction
dc.subjectProbability
dc.subjectQuantum theory
dc.subjectRadiation detection
dc.titleFree massive particles with total energy E<mc2 in curved spacetimes
dc.typeOtro


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