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dc.contributor.authorLagaris, I. E.en
dc.contributor.authorPandharipande, V. R.en
dc.date.accessioned2015-11-24T17:02:53Z-
dc.date.available2015-11-24T17:02:53Z-
dc.identifier.issn0375-9474-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/11107-
dc.rightsDefault Licence-
dc.titleVariational calculations of asymmetric nuclear matteren
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.primary10.1016/0375-9474(81)90032-4-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Θετικών Επιστημών. Τμήμα Μηχανικών Ηλεκτρονικών Υπολογιστών και Πληροφορικήςel
heal.publicationDate1981-
heal.abstractWe report on variational calculations of the energy E(ρ, β) of asymmetric nuclear matter having ? = ?n + ?p = 0.05 to 0.35 fm?3, and β = (?n ? ?p/g9 = 0 to 1. The nuclear h used in this work consists of a realistic two-nucleon interaction, called v14, that fits the available nucleon-nucleon scattering data up to 425 MeV, and a phenomenological three nucleon interaction adjusted to reproduce the empirical properties of symmetric nuclear matter. The variational many-body theory of symmetric nuclear matter is extended to treat matter with neutron excess. Numerical and analytic studies of the β-dependence of various contributions to the nuclear matter energy show that at ? < 0.35 fm?3 the β4 terms are very small, and that the interaction energy EI(ρ, β) defined as E(ρ, β) ? TF(ρ, β), where TF is the Fermi-gas energy, is well approximated by EI0(?) + β2EI2(ρ). The calculated symmetry energy at equilibrium density is 30 MeV and it increases from 15 to 38 MeV as ? increases from 0.05 to 0.35 fm?3.en
heal.journalNameNuclear Physics Aen
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
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