Cooling modes of neutron stars

Details Cooling modes of neutron stars Cooling modes of neutron stars

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998phrvd..57.5963j&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 57, Issue 10, 15 May 1998, pp.5963-5969

Physics

2

Neutron Stars, Nuclear Matter, Weak-Interaction And Lepton Aspects, Elementary Particle Processes

Scientific paper

The direct Urca process is studied in the presence of kaon condensation. We consider the contributions from both strange and nonstrange hadrons. Our calculations indicate that the role of hyperons is as important as the role of nonstrange 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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