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Author Flowers, E. G. ♦ Sutherland, P. G. ♦ Bond, J. R.
Sponsorship USDOE
Source United States Department of Energy Office of Scientific and Technical Information
Content type Text
Language English
Subject Keyword Physics (Astrophysics & Cosmology)-Stars ♦ Physics (High Energy)-Particle Interactions & Properties (Theoretical)-Strong (Baryon No. >= 2) ♦ Physics Research-Astrophysics & Cosmology-Stars ♦ NEUTRINOS- PAIR PRODUCTION ♦ NEUTRON STARS- WEAK NEUTRAL CURRENTS ♦ NEUTRON-NEUTRON INTERACTIONS- BREMSSTRAHLUNG ♦ PROTON-NEUTRON INTERACTIONS- BREMSSTRAHLUNG ♦ S MATRIX ♦ TEMPERATURE DEPENDENCE ♦ THERMODYNAMIC PROPERTIES ♦ V-A THEORY
Abstract We calculate neutrino pair bremsstrahlung from nucleons in neutron-star matter via weak neutral currents. We find bremsstrahlung in neutron-neutron collisions to be unimportant, but find that the bremsstrahlung emissivity in neutron-proton collisions is of the same order as that for the modified URCA process.
Educational Use Research
Learning Resource Type Article
Publisher Date 1975-07-15
Publisher Place United States
Journal Phys. Rev., D
Volume Number 12
Issue Number 2
Organization Department of Physics, New York University, New York, New York 10003


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