Neutrino bremsstrahlung from quarks and the cooling of neutron stars

Journal Article · Wed Oct 15 00:00:00 EDT 1980 · Phys. Rev., D; (United States)

DOI:https://doi.org/10.1103/PhysRevD.22.1910· OSTI ID:5001780

Price, C

The energy flux from degenerate quark matter due to bremsstrahlung of neutrino pairs is computed. The polarization corrections to the gluon propagator are treated correctly. It is shown that the resultant emissivity is similar to that from pion-condensed neutron matter.

• Research Organization: Department of Physics, University of California, Santa Barbara, California 93106
• OSTI ID: 5001780
• Journal Information: Phys. Rev., D; (United States), Vol. 22:8
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
NEUTRINOS
BREMSSTRAHLUNG
NEUTRON STARS
EMISSIVITY
GLUONS
NUCLEAR MATTER
PION CONDENSATION
POLARIZATION
PROPAGATOR
QUANTUM CHROMODYNAMICS
QUANTUM ELECTRODYNAMICS
QUARKS
SU-3 GROUPS
ELECTRODYNAMICS
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
FERMIONS
FIELD THEORIES
LEPTONS
LIE GROUPS
MASSLESS PARTICLES
MATTER
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
POSTULATED PARTICLES
QUANTUM FIELD THEORY
RADIATIONS
STARS
SU GROUPS
SURFACE PROPERTIES
SYMMETRY GROUPS
645203* - High Energy Physics- Particle Interactions & Properties-Theoretical- Weak Interactions & Properties
640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar
Radio & X-Ray Sources