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Nuclear matter with scalar-vector interactions

dc.contributor.authorMoncada A.
dc.contributor.authorScholtz F.G.
dc.contributor.authorHahne F.J.W.
dc.date.accessioned2011-05-15T16:00:11Z
dc.date.available2011-05-15T16:00:11Z
dc.date.issued1994
dc.identifier.citationPhysical Review C
dc.identifier.citation50
dc.identifier.citation3
dc.identifier.issn5562813
dc.identifier.other10.1103/PhysRevC.50.1412
dc.identifier.urihttp://hdl.handle.net/10019.1/11571
dc.description.abstractThe properties of cold nuclear matter are investigated in a class of nonlinear mean field - theories which includes a density dependence of the meson parameters. This dependence can be both explicit and implicit through the effective nucleon mass. We apply the theory to the case of an interaction between the scalar and the vector mesons and investigate the properties of neutron stars using the resulting equation of state. © 1994 The American Physical Society.
dc.titleNuclear matter with scalar-vector interactions
dc.typeArticle
dc.description.versionArticle


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