Neutrino emissivity from e sup minus synchrotron and e sup minus e+ annihilation processes in a strong magnetic field: General formalism and nonrelativistic limit
- A. F. Ioffe Institute of Physics and Technology, SU 194021, St. Petersburg (Russia)
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, PL-00-716 Warszawa (Poland)
A general formalism is developed for calculating the neutrino emissivities of synchrotron and {ital e}{sup {minus}}{ital e+} annihilation radiations in a plasma in the presence of a large magnetic field {ital B}{similar to}10{sup 12}--10{sup 14} G. As a first step, the formalism is used to calculate the synchrotron and annihilation radiations from a nonrelativistic electron plasma (density {rho}{approx lt}10{sup 6} g cm{sup {minus}3}, temperature {ital T}{approx lt}6{times}10{sup 9} K) including the cases of nondegenerate and degenerate electrons, and of quantizing and nonquantizing magnetic fields. We conclude that these processes can be important for neutrino production in a hot plasma of neutron star envelopes.
- OSTI ID:
- 7200020
- Journal Information:
- Physical Review, D (Particles Fields); (United States), Vol. 46:8; ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
Pa
ELECTRON-POSITRON INTERACTIONS
ANNIHILATION
HOT PLASMA
NEUTRINOS
EMISSION
NEUTRON STARS
MAGNETIC FIELDS
PARTICLE PRODUCTION
SYNCHROTRON RADIATION
WEINBERG-SALAM GAUGE MODEL
BASIC INTERACTIONS
BREMSSTRAHLUNG
ELECTROMAGNETIC INTERACTIONS
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
FERMIONS
FIELD THEORIES
INTERACTIONS
LEPTON-LEPTON INTERACTIONS
LEPTONS
MASSLESS PARTICLES
MATHEMATICAL MODELS
PARTICLE INTERACTIONS
PARTICLE MODELS
PLASMA
RADIATIONS
STARS
UNIFIED GAUGE MODELS
UNIFIED-FIELD THEORIES
662310* - Weak & Electromagnetic Interactions of Leptons- (1992-)
662210 - Specific Theories & Interaction Models
Particle Systematics- Unified Theories & Models- (1992-)