Published July 1985
| Version v1
Journal article
Relaxation times in superfluid cores of neutron stars
Description
The velocity relaxation times of electrons on proton vortex filaments formed by the drag effect in the npe phase of a neutron star are considered. It is shown that the npe phase is rigidly connected to the crust of the star
Additional details
Publishing Information
- Journal Title
- Astrophysics (Engl. Transl.)
- Journal Volume
- 21
- Journal Issue
- 1
- Series
- Astrophysics (Engl. Transl.).
- Journal Page Range
- 34-38
- ISSN
- 0004-6396
- CODEN
- ATPYA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 18003774
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC ELECTRONS; DRAG; ELECTRON-PROTON INTERACTIONS; NEUTRON STARS; PARTICLE KINEMATICS; RELAXATION TIME; STAR EVOLUTION; SUPERFLUIDITY; VELOCITY; VORTICES
- Descriptors DEC
- COSMIC RADIATION; ELECTRON-NUCLEON INTERACTIONS; ELECTRONS; ELEMENTARY PARTICLES; FERMIONS; INTERACTIONS; IONIZING RADIATIONS; LEPTON-BARYON INTERACTIONS; LEPTON-HADRON INTERACTIONS; LEPTON-NUCLEON INTERACTIONS; LEPTONS; PARTICLE INTERACTIONS; RADIATIONS; SECONDARY COSMIC RADIATION; STARS
Optional Information
- Notes
- Translated from Astrofizika, Vol. 22, No. 1, pp. 137-144, January-February, 1985.. Cover-to-cover translation of Astrofizika (USSR).