Many-body theory of nuclear and neutron star matter

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dc.creatorPandharipande, V. R.
dc.creatorAkmal, A.
dc.creatorRavenhall, D. G.
dc.date1998-02-16
dc.date.accessioned2026-07-07T05:42:19Z
dc.date.available2026-07-07T05:42:19Z
dc.descriptionWe present results obtained for nuclei, nuclear and neutron star matter, and neutron star structure obtained with the recent Argonne v18 two- nucleon and Urbana IX three-nucleon interactions including relativistic boost corrections. These interactions predict that matter will undergo a transition to a spin layered phase with neutral pion condensation. We also consider the possibility of a transition to quark matter.
dc.description18 pages, 10 figures included as .eps files. To appear in "Hirschegg '98: Nuclear Astrophysics", Proc. Int. Workshop XXVI on Gross Properties of Nuclei and Nuclear Excitations, January 11-17, 1998, Hirschegg, Austria
dc.identifierhttps://arxiv.org/abs/nucl-th/9802048
dc.identifierhttp://arxiv.org/abs/nucl-th/9802048
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/82884
dc.subjectNuclear Theory
dc.titleMany-body theory of nuclear and neutron star matter
dc.typetext

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