The equation of state for neutron stars
β Scribed by F. Ferrini
- Publisher
- Springer Netherlands
- Year
- 1975
- Tongue
- English
- Weight
- 549 KB
- Volume
- 32
- Category
- Article
- ISSN
- 0004-640X
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π SIMILAR VOLUMES
The role of the equation of state in the structure of neutron stars is summarized. At densities beyond a few times the normal nuclear saturation density, the neutron-proton-electron sea can be supplemented with more exotic matter, usually involving strangeness, such as hyperons, kaon or pion condens
Baryon pairing and neutron superfluidity are believed to play an important role in the evolution of neutron stars. The pairing interaction provides a partial antisymmetrization of the nucleons in the stars with the evidence that fractional statistics must hold. By using a kinetic approach recently p