Bulk viscosity of hot-neutron-star matter from direct URCA processes

Details Bulk viscosity of hot-neutron-star matter from direct URCA processes Bulk viscosity of hot-neutron-star matter from direct URCA processes

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvd..45.4708h&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 45, Issue 12, 15 June 1992, pp.4708-4712

Physics

31

Neutron Stars, Nuclear Matter, Elementary Particle Processes

Scientific paper

Direct URCA processes, occurring in neutron-star matter with a proton
fraction exceeding the critical value of (11-15)%, can strongly enhance
the bulk viscosity of the matter.

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