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

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Constraints 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.
4 pages, 2 figures, ASP Conference Series, Vol 138, 131, eds K. L. Chan, K. S. Cheng, H. P. Singh

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/2297

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0012541
 http://arxiv.org/abs/astro-ph/0012541

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arXiv