Neutrino opacity of neutron-star matter

Details Neutrino opacity of neutron-star matter Neutrino opacity of neutron-star matter

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975phrvd..11.2740s&link_type=abstract

Physical Review D - Particles and Fields, 3rd Series, vol. 11, May 15, 1975, p. 2740-2745. NSF-supported research.

Astronomy and Astrophysics

Astronomy

46

Equations Of State, Neutrinos, Neutron Stars, Opacity, Stellar Temperature, Astronomical Models, Density Distribution, Mean Free Path, Temperature Effects

Scientific paper

Scattering of neutrinos from neutron-star matter is calculated for the case of very high neutron-star temperatures, under the assumption of a neutral-current interaction of the form given by the Weinberg-Salam theory. The resulting neutrino opacity depends in an interesting way upon the equation of state of the matter. The maximum possible opacity of a thin layer of matter is estimated for the case of an arbitrary equation of state.

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