Proto-Neutron and Neutron Stars

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dc.creatorDexheimer, V.
dc.creatorSchramm, S.
dc.creatorStoecker, H.
dc.date2008-01-16
dc.date.accessioned2026-07-07T08:54:52Z
dc.date.available2026-07-07T08:54:52Z
dc.descriptionThe parity doublet model, containing the SU(2) multiplets including the baryons identified as the chiral partners of the nucleons is applied to neutron stars. The maximum mass for the star is calculated for different stages of the cooling taking into account finite temperature/entropy effect, trapped neutrinos and fixed baryon number. Rotation effects are also included.
dc.descriptionPrepared for International Workshop on Astronomy and Relativistic Astrophysics (IWARA 2007), Joao Pessoa, Brazil, 3-6 Oct 2007
dc.identifierhttps://arxiv.org/abs/0801.2523
dc.identifierhttp://arxiv.org/abs/0801.2523
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/146094
dc.subjectAstrophysics
dc.titleProto-Neutron and Neutron Stars
dc.typetext

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