Please use this identifier to cite or link to this item: https://hdl.handle.net/10316/46530
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dc.contributor.authorPais, H.-
dc.contributor.authorProvidência, C.-
dc.date.accessioned2018-01-17T14:54:53Z-
dc.date.available2018-01-17T14:54:53Z-
dc.date.issued2016-07-29-
dc.identifier.urihttps://hdl.handle.net/10316/46530-
dc.language.isoengpor
dc.publisherAmerican Physical Societypor
dc.relationsupported by Fundação para a Ciência e Tecnologia (FCT) under Project No. SFRH/BPD/95566/2013por
dc.rightsopenAccesspor
dc.titleVlasov formalism for extended relativistic mean field models: The crust-core transition and the stellar matter equation of statepor
dc.typearticlepor
degois.publication.issuePhys. Rev. Cpor
dc.identifier.doi10.1103/PhysRevC.94.015808-
degois.publication.volumeVol. 94, Iss. 1por
uc.controloAutoridadeSim-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.openairetypearticle-
item.cerifentitytypePublications-
item.grantfulltextopen-
item.fulltextCom Texto completo-
item.languageiso639-1en-
crisitem.author.researchunitCFisUC – Center for Physics of the University of Coimbra-
crisitem.author.orcid0000-0001-7247-1950-
crisitem.author.orcid0000-0001-6464-8023-
Appears in Collections:I&D CFis - Artigos em Revistas Internacionais
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