Protoneutron stars and constraints on maximum and minimum mass of neutron stars

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dc.creatorGondek, D.
dc.creatorHaensel, P.
dc.creatorZdunik, J. L.
dc.date2000-12-29
dc.date.accessioned2026-07-07T01:57:13Z
dc.date.available2026-07-07T01:57:13Z
dc.descriptionConstraints on minimum and maximum mass of ordinary neutron stars are imposed by the consideration of their early evolution (protoneutron star stage). Calculations are performed for a realistic standard model of hot, dense matter (Lattimer & Swesty 1991) valid for both supranuclear and subnuclear densities. Various assumptions concerning protoneutron star interior (large trapped lepton number, no trapped lepton number, isentropic, isothermal) are taken into account.
dc.description4 pages, 2 figures, ASP Conference Series, Vol 138, 131, eds K. L. Chan, K. S. Cheng, H. P. Singh
dc.identifierhttps://arxiv.org/abs/astro-ph/0012541
dc.identifierhttp://arxiv.org/abs/astro-ph/0012541
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2297
dc.subjectAstrophysics
dc.titleProtoneutron stars and constraints on maximum and minimum mass of neutron stars
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