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Superfluidity in Neutron Star Matter
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Superfluidity of nuclear matter relevant for neutron star physics is reviewed.
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Cited by 3 Pith papers
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Exploring nuclear force with pulsar glitch observation
A self-consistent neutron star glitch model for the 2000 Vela event constrains the nuclear symmetry energy slope to below 40 MeV and suggests Vela is a massive neutron star.
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Bose-Einstein condensation in a rigidly rotating relativistic boson gas
In a slowly rotating ideal Bose gas, the BEC critical temperature scales as (density x angular velocity)^{2/5} in the nonrelativistic limit, and the heat capacity acquires a jump at the transition.
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Impact of Anisotropy on Neutron Star Structure and Curvature
Moderate positive pressure anisotropy raises neutron star maximum mass to about 2.4 solar masses and compactness by up to 20 percent, with curvature scalars tied to matter showing strong sensitivity while the Weyl sca...
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