Published May 1975
| Version v1
Journal article
Neutron star models with condensed π- phase
Description
Following Sawyer, models of neutron stars with condensed phase at the core were constructed by numerically integrating the differential equation. All such models are unstable. (author)
Additional details
Publishing Information
- Journal Title
- Indian J. Phys.
- Journal Volume
- 49
- Journal Issue
- 5
- Series
- Indian J. Phys.
- Journal Page Range
- 333-337
INIS
- Country of Publication
- India
- Country of Input or Organization
- India
- INIS RN
- 7238773
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- MATHEMATICAL MODELS; NEUTRON STARS; NEUTRONS; PIONS; PROTONS; STABILITY
- Descriptors DEC
- BARYONS; BOSONS; CATIONS; CHARGED PARTICLES; ELEMENTARY PARTICLES; FERMIONS; HADRONS; HYDROGEN IONS; HYDROGEN IONS 1 PLUS; IONS; MESONS; NUCLEONS; PSEUDOSCALAR MESONS; STARS
Optional Information
- Notes
- 7 refs.