Rotating Neutron Stars in a Chiral SU(3) Model

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dc.creatorSchramm, S.
dc.creatorZschiesche, D.
dc.date2002-04-30
dc.date.accessioned2026-07-07T10:50:50Z
dc.date.available2026-07-07T10:50:50Z
dc.descriptionWe study the properties of rotating neutron stars within a generalized chiral SU(3)-flavor model. The influence of the rotation on the inner structure and the hyperon matter content of the star is discussed. We calculate the Kepler frequency and moments of inertia of the neutron star sequences. An estimate for the braking index of the associated pulsars is given.
dc.description14 pages, 9 figures
dc.identifierhttps://arxiv.org/abs/nucl-th/0204075
dc.identifierhttp://arxiv.org/abs/nucl-th/0204075
dc.identifierJ.Phys.G29:531-542,2003
dc.identifierdoi:10.1088/0954-3899/29/3/307
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/184661
dc.subjectNuclear Theory
dc.titleRotating Neutron Stars in a Chiral SU(3) Model
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