Neutrino Cooling of Neutron Stars in Pion-Condensed Phase

Details Neutrino Cooling of Neutron Stars in Pion-Condensed Phase Neutrino Cooling of Neutron Stars in Pion-Condensed Phase

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pthph..58.1766k&link_type=abstract

Progress of Theoretical Physics, Vol. 58, No. 6, pp. 1766-1774

Physics

5

Scientific paper

Neutrino energy loss rates of neutron stars in the pion-condensed phase are calculated. The studied processes are the decay of thermally excited pions and the nucleon URCA process. The nucleon URCA process makes a major contribution to the cooling rate. The expected neutrino luminosity is about 7.6 × 1044 ergs/sec (T/109K)6 for 1M&sun; neutron stars. This luminosity is 107 times as high as the standard value.

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