Protoneutron stars and neutron stars
2000 ◽
Vol 177
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pp. 663-664
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AbstractWe find constraints on minimum and maximum mass of ordinary neutron stars imposed by their early evolution (protoneutron star stage). We calculate models of protoneutron stars using a realistic standard equation of state of hot, dense matter valid for both supranuclear and subnuclear densities. Results for different values of the nuclear incompressibility are presented.
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2002 ◽
Vol 385
(1)
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pp. 301-307
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1971 ◽
Vol 46
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pp. 352-355
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2016 ◽
Vol 463
(3)
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pp. 2667-2679
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