Published May 1978
| Version v1
Journal article
Neutrino-pair Bremsstrahlung from a hot plasma in the presence of a strong magnetic field
Description
The stellar energy loss rate due to the production of neutrino pairs by Bremsstrahlung is calculated for neutron stars in the presence of a strong magnetic field (B <= 1012 G) and the Coulomb field of the positive ions. The calculated energy loss rates are applied to nonrelativistic electrons at low densities <= 105 gm/cm3 and relatively low temperatures T <= 109 K. (author)
Additional details
Identifiers
Publishing Information
- Journal Title
- Annalen der Physik
- Journal Volume
- 490
- Journal Issue
- 1
- Series
- Ann. Phys. (Leipzig).
- Journal Page Range
- 1-9
- ISSN
- 0003-3804
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- German Democratic Republic
- INIS RN
- 9415850
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BREMSSTRAHLUNG; CATIONS; COULOMB FIELD; ENERGY LOSSES; HAMILTONIANS; HOT PLASMA; MAGNETIC FIELDS; NEUTRINO-ELECTRON INTERACTIONS; NEUTRINOS; NEUTRON STARS; PAIR PRODUCTION; PROPAGATOR
- Descriptors DEC
- CHARGED PARTICLES; ELECTRIC FIELDS; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; INTERACTIONS; IONS; LEPTON-LEPTON INTERACTIONS; LEPTONS; MASSLESS PARTICLES; MATHEMATICAL OPERATORS; PARTICLE INTERACTIONS; PARTICLE PRODUCTION; PLASMA; QUANTUM OPERATORS; RADIATIONS; STARS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent