Published January 1991
| Version v1
Journal article
Neutron gas of a degenerate superdense star with frozen-in magnetic field
Creators
- 1. Brestskij Gosudarstvennyj Pedagogicheskij Inst., Brest (Byelorussian SSR)
Description
Filling energy subzones of the degenerate nonrelativistic neutron gas of a superdense star is calculated in dependence on the intensity of the magnetic field. It is shown, that with an increase of magnetic field intensity the Fermi kinetic energy of degenerate gas increases to the limit, to which corresponds the filling with neutrons of all the magnetic states with magnetic moments parallel to the direction of the magnetic field
Additional details
Additional titles
- Original title (Russian)
- Нейтронный газ вырожденной сверхплотной звезды с вмороженным магнитным полем
Publishing Information
- Journal Title
- Astronomicheskij Zhurnal
- Journal Volume
- 68
- Journal Issue
- 1
- Series
- Astron. Zh.
- Journal Page Range
- 101-108
- ISSN
- 0004-6299
- CODEN
- ASZHA
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 22070447
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- FERMI LEVEL; MAGNETIC FIELDS; NEUTRON DENSITY; NEUTRON STARS; NEUTRONS; NUCLEAR MATTER
- Descriptors DEC
- BARYONS; ELEMENTARY PARTICLES; ENERGY LEVELS; FERMIONS; HADRONS; MATTER; NUCLEONS; STARS