Bulk viscosity of neutron-star matter

Details Bulk viscosity of neutron-star matter Bulk viscosity of neutron-star matter

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001phrvd..64h4003j&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 64, Issue 8, 15 October 2001, id.084003

Physics

56

Relativistic Stars: Structure, Stability, And Oscillations, Wave Generation And Sources, Neutron Stars

Scientific paper

Hyperon bulk viscosity is the most significant transport coefficient affecting the growth or decay of any neutron-star mode of oscillation which has, even to second order in its amplitude, a periodic density fluctuation. This paper evaluates both the direct Urca and strangeness-changing four-baryon weak-interaction terms in the coefficient.

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