Published September 1986
| Version v1
Journal article
Magnetic moments of neutron stars with different equations of state
Description
The magnetic moment due to the dragging of superfluid protons by rotating superfluid neutrons is calculated for different stars using different equations of state. The results obtained are of order 1029-1030 G.cm3
Additional details
Publishing Information
- Journal Title
- Astrophysics (Engl. Transl.)
- Journal Volume
- 24
- Journal Issue
- 2
- Series
- Astrophysics (Engl. Transl.).
- Journal Page Range
- 165
- ISSN
- 0004-6396
- CODEN
- ATPYA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 18034092
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC NEUTRONS; COSMIC PROTONS; DRAG; EQUATIONS OF STATE; MAGNETIC MOMENTS; NEUTRON STARS; PENETRATION DEPTH; ROTATION; RUNGE-KUTTA METHOD; STAR MODELS; SUPERCONDUCTIVITY; SUPERFLUIDITY
- Descriptors DEC
- BARYONS; CATIONS; CHARGED PARTICLES; COSMIC RADIATION; ELECTRIC CONDUCTIVITY; ELECTRICAL PROPERTIES; ELEMENTARY PARTICLES; EQUATIONS; FERMIONS; HADRONS; HYDROGEN IONS; HYDROGEN IONS 1 PLUS; INTERPOLATION; IONIZING RADIATIONS; IONS; MATHEMATICAL MODELS; NEUTRONS; NUCLEONS; NUMERICAL SOLUTION; PHYSICAL PROPERTIES; PROTONS; RADIATIONS; SECONDARY COSMIC RADIATION; STARS
Optional Information
- Notes
- Cover-to-cover translation of Astrofizika (USSR).