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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/66273
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dc.contributor.authorPanda, P. K.-
dc.contributor.authorSahu, R.-
dc.contributor.authorMishra, S.-
dc.date.accessioned2014-05-27T11:19:57Z-
dc.date.accessioned2016-10-25T18:16:36Z-
dc.date.available2014-05-27T11:19:57Z-
dc.date.available2016-10-25T18:16:36Z-
dc.date.issued2000-11-01-
dc.identifierhttp://dx.doi.org/10.1103/PhysRevC.62.055802-
dc.identifier.citationPhysical Review C - Nuclear Physics, v. 62, n. 5, p. 558021-558028, 2000.-
dc.identifier.issn0556-2813-
dc.identifier.urihttp://hdl.handle.net/11449/66273-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/66273-
dc.description.abstractWe study the equation of state for neutron matter using the Walecka model including quantum corrections for baryons and sigma mesons through a realignment of the vacuum. We next use this equation of state to calculate the radius, mass, and other properties of rotating neutron stars.en
dc.format.extent558021-558028-
dc.language.isoeng-
dc.sourceScopus-
dc.titleEffects of vacuum structure on neutron starsen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.contributor.institutionBerhampur University-
dc.description.affiliationInstituto de Física Teorica Universidade Estadual Paulista, Rua Pamplona 145, 01405-900 Sao Paulo - SP-
dc.description.affiliationDepartment of Physics Berhampur University, Berhampur-760007, Orissa-
dc.description.affiliationUnespInstituto de Física Teorica Universidade Estadual Paulista, Rua Pamplona 145, 01405-900 Sao Paulo - SP-
dc.identifier.doi10.1103/PhysRevC.62.055802-
dc.identifier.wosWOS:000165369400065-
dc.rights.accessRightsAcesso restrito-
dc.identifier.file2-s2.0-0039000175.pdf-
dc.relation.ispartofPhysical Review C: Nuclear Physics-
dc.identifier.scopus2-s2.0-0039000175-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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