Reconciling 2 M&sun; Pulsars and SN1987A:. Two Branches of Neutron Stars

Details Reconciling 2 M&sun; Pulsars and SN1987A:. Two Branches of Neutron Stars Reconciling 2 M&sun; Pulsars and SN1987A:. Two Branches of Neutron Stars

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008esnm.conf..235h&link_type=abstract

EXOTIC STATES OF NUCLEAR MATTER. Proceedings of the International Symposium EXOCT07. Held 11-15 June 2007 in Catania University,

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The analysis of SN1987A led Brown and Bethe1,2 to conclude that the maximum mass of cold neutron stars is Mmax ≈ 1.5M&sun;. On the other hand, recent evaluation of the mass of PSR J0751+1807 implies Mmax > 1.5M&sun;. This contradicts the original Bethe-Brown model but can be reconciled within evolutionary scenarios proposed in this talk.3

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