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
✦ LIBER ✦
Glitches induced by the core superfluid in a neutron star
✍ Scribed by M. Jahan-Miri
- Publisher
- John Wiley and Sons
- Year
- 2002
- Tongue
- English
- Weight
- 222 KB
- Volume
- 330
- Category
- Article
- ISSN
- 0035-8711
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