Pion-condensed neutron star and pulsar glitch
โ Scribed by T. Takatsuka; R. Tamagaki
- Publisher
- Elsevier Science
- Year
- 1988
- Tongue
- English
- Weight
- 310 KB
- Volume
- 478
- Category
- Article
- ISSN
- 0375-9474
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๐ SIMILAR VOLUMES
Aspects of the neutron 3P 2 superfluid in the core of neutron stars are considered, by putting emphasis on specific features of the nuclear interaction leading to multi-hadronic phases in the neutron star interior and the coexistent features with pion condensates. Concerning their roles on neutron s
A theory of isospin asymmetric matter and of neutron star matter in particular, which is compatible with bulk nuclear properties, is formulated in the framework of a relativistic field theory and solved in the mean field approximation. The self-consistent conditions defining the u-. w-, K-, and p-f