You are in the accessibility menu

Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/23111
Full metadata record
DC FieldValueLanguage
dc.contributor.authorPanda, P. K.-
dc.contributor.authorSahu, R.-
dc.contributor.authorMishra, S.-
dc.date.accessioned2014-05-20T14:05:52Z-
dc.date.available2014-05-20T14:05:52Z-
dc.date.issued2001-01-01-
dc.identifier.citationInternational Workshop on Hadron Physics 2000. Singapore: World Scientific Publ Co Pte Ltd, p. 405-408, 2001.-
dc.identifier.urihttp://hdl.handle.net/11449/23111-
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 star.en
dc.format.extent405-408-
dc.language.isoeng-
dc.publisherWorld Scientific Publ Co Pte Ltd-
dc.sourceWeb of Science-
dc.titleEffects of vacuum structure on neutron staren
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, Brazil-
dc.identifier.wosWOS:000172097700040-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofInternational Workshop on Hadron Physics 2000-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

There are no files associated with this item.
Show simple item record Show full item record   View Statistics
 

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