Neutrino Cooling of Neutron Stars by Percolating Quarks

Details Neutrino Cooling of Neutron Stars by Percolating Quarks Neutrino Cooling of Neutron Stars by Percolating Quarks

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pthph..66..725k&link_type=abstract

Progress of Theoretical Physics, Vol. 66, No. 2, pp. 725-728

Physics

10

Scientific paper

The neutrino emissivity of percolating quarks due to URCA process is
calculated. It is shown that the resultant emissivity is almost
comparable to that of pion-condensed matter. As a result, if nucleons
overlap and quarks percolate in a neutron star, it also cools rapidly.

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