Quantized fields and gravitational particle creation in f (R) expanding universes

dc.creatorPEREIRA, S. H.
dc.creatorBESSA, C. H. G.
dc.creatorLIMA, J. A. S.
dc.date.accessioned2012-10-20T02:13:02Z
dc.date.accessioned2018-07-04T15:30:14Z
dc.date.available2012-10-20T02:13:02Z
dc.date.available2018-07-04T15:30:14Z
dc.date.created2012-10-20T02:13:02Z
dc.date.issued2010
dc.identifierPHYSICS LETTERS B, v.690, n.2, p.103-107, 2010
dc.identifier0370-2693
dc.identifierhttp://producao.usp.br/handle/BDPI/27090
dc.identifier10.1016/j.physletb.2010.05.027
dc.identifierhttp://dx.doi.org/10.1016/j.physletb.2010.05.027
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1623740
dc.description.abstractThe problem of cosmological particle creation for a spatially flat, homogeneous and isotropic universes is discussed in the context of f (R) theories of gravity. Different from cosmological models based on general relativity theory, it is found that a conformal invariant metric does not forbid the creation of massless particles during the early stages (radiation era) of the universe. (C) 2010 Elsevier B.V. All rights reserved.
dc.languageeng
dc.publisherELSEVIER SCIENCE BV
dc.relationPhysics Letters B
dc.rightsCopyright ELSEVIER SCIENCE BV
dc.rightsrestrictedAccess
dc.subjectParticle creation
dc.subjectf(R) theories
dc.titleQuantized fields and gravitational particle creation in f (R) expanding universes
dc.typeArtículos de revistas


Este ítem pertenece a la siguiente institución