Cooling modes of neutron stars

Details Cooling modes of neutron stars Cooling modes of neutron stars

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..610..480j&link_type=abstract

NUCLEAR PHYSICS IN THE 21st CENTURY:International Nuclear Physics Conference INPC 2001. AIP Conference Proceedings, Volume 610,

Physics

Nuclear Physics

Nuclear Matter Aspects Of Neutron Stars, Neutron Stars

Scientific paper

The direct Urca process is studied in the presence of kaon condensation. We consider the contributions from both strange and non-strange hadrons. Our calculations indicate that the role of hyperons is as important as the role of non-strange nucleons in the cooling mechanism of neutron stars. We also find that the temperature dependence of the weak neutral current contribution is given by T7, which intermediates between the direct Urca process of T6 and the modified Urca process of T8. .

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