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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/66182
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dc.contributor.authorVanzella, Daniel A. T.-
dc.contributor.authorMatsas, George E. A.-
dc.date.accessioned2014-05-27T11:19:55Z-
dc.date.accessioned2016-10-25T18:16:26Z-
dc.date.available2014-05-27T11:19:55Z-
dc.date.available2016-10-25T18:16:26Z-
dc.date.issued2000-06-15-
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.61.127303-
dc.identifier.citationPhysical Review D - Particles, Fields, Gravitation and Cosmology, v. 61, n. 12, p. 1-4, 2000.-
dc.identifier.issn0556-2821-
dc.identifier.urihttp://hdl.handle.net/11449/66182-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/66182-
dc.description.abstractWe discuss the possible influence of gravity in the neutronization process p+e-→νe, which is particularly important as a cooling mechanism of neutron stars. Our approach is semiclassical in the sense that leptonic fields are quantized on a classical background spacetime, while neutrons and protons are treated as excited and unexcited nucleon states, respectively. We expect gravity to have some influence wherever the energy content carried by the in state is barely above the neutron mass. In this case the emitted neutrinos would be soft enough to have a wavelength of the same order as the space curvature radius. ©2000 The American Physical Society.en
dc.format.extent1-4-
dc.language.isoeng-
dc.sourceScopus-
dc.titleSearch for semiclassical gravity effects in relativistic starsen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationInst. de Fis. Teórica Universidade Estadual Paulista, Rua Pamplona 145, 01405-900, São Paulo, SP-
dc.description.affiliationUnespInst. de Fis. Teórica Universidade Estadual Paulista, Rua Pamplona 145, 01405-900, São Paulo, SP-
dc.identifier.doi10.1103/PhysRevD.61.127303-
dc.identifier.wosWOS:000087678100071-
dc.rights.accessRightsAcesso aberto-
dc.identifier.file2-s2.0-17144394503.pdf-
dc.relation.ispartofPhysical Review D: Particles, Fields, Gravitation and Cosmology-
dc.identifier.scopus2-s2.0-17144394503-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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