Pion-Condensed Neutron Star and Supernova 1987A

Details Pion-Condensed Neutron Star and Supernova 1987A Pion-Condensed Neutron Star and Supernova 1987A

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pthph..78..516t&link_type=abstract

Progress of Theoretical Physics, Vol. 78, No. 3, pp. 516-520

Physics

9

Scientific paper

Characteristics of pion-condensed neutron star are discussed. Based on these, an attempt is made to explain the existence of two dominant peaks with the time interval Delta t( ~ 10 s) in neutrino flux from the supernova 1987A. It is remarked that Delta t is closely related to the temperature and central density of the neutron star assumed in the supernova.

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