Asymmetric Nuclear Matter with Pion Dressing

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dc.creatorSarangi, S.
dc.creatorPanda, P. K.
dc.creatorSahu, S. K.
dc.creatorMaharana, L.
dc.date2007-11-30
dc.date.accessioned2026-07-07T08:46:23Z
dc.date.available2026-07-07T08:46:23Z
dc.descriptionWe discuss a self-consistent method to calculate the properties of cold asymmetric nuclear matter which is dressed with isoscalar scalar pion condensates. The nucleon-nucleon interaction is mediated by these pion pairs, omega- and rho- mesons. The parameters of these interactions are evaluated self-consistently using the saturation properties of nuclear matter like binding energy, pressure, compressibility and symmetry energy. The computed equation of state of pure neutron matter (PNM) is used to calculate mass and radius of a pure neutron star.
dc.description12 pages, 9 figures, 1 table
dc.identifierhttps://arxiv.org/abs/0711.4874
dc.identifierhttp://arxiv.org/abs/0711.4874
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/143233
dc.subjectNuclear Theory
dc.titleAsymmetric Nuclear Matter with Pion Dressing
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