Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-12-29
Astronomy and Astrophysics
Astrophysics
4 pages, 2 figures, ASP Conference Series, Vol 138, 131, eds K. L. Chan, K. S. Cheng, H. P. Singh
Scientific paper
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.
Gondek D.
Haensel Pawel
Zdunik Leszek J.
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