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
How viscous is a superfluid neutron star core?
β Scribed by N. Andersson; G.L. Comer; K. Glampedakis
- Publisher
- Elsevier Science
- Year
- 2005
- Tongue
- English
- Weight
- 436 KB
- Volume
- 763
- Category
- Article
- ISSN
- 0375-9474
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