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Superfluidity in Neutron Star Matter

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arxiv astro-ph/0012209 v1 pith:INLYDFCN submitted 2000-12-10 astro-ph nucl-th

classification astro-phnucl-th
keywords matterneutronstarsuperfluiditynuclearphysicsrelevantreviewed
verification ladder T0 review T1 audit T2 compute T3 formal

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Superfluidity of nuclear matter relevant for neutron star physics is reviewed.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Exploring nuclear force with pulsar glitch observation

    nucl-th 2024-12 conditional novelty 6.0 of 10

    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.

  2. Bose-Einstein condensation in a rigidly rotating relativistic boson gas

    hep-ph 2024-11 conditional novelty 6.0 of 10

    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.

  3. Impact of Anisotropy on Neutron Star Structure and Curvature

    gr-qc 2025-12 unverdicted novelty 4.0 of 10

    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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