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Superfluidity in Neutron Star Matter

1 Pith paper cite this work. Polarity classification is still indexing.

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abstract

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

fields

gr-qc 1

years

2025 1

verdicts

UNVERDICTED 1

representative citing papers

Impact of Anisotropy on Neutron Star Structure and Curvature

gr-qc · 2025-12-30 · unverdicted · novelty 4.0

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 scalar stays largely insensitive.

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  • Impact of Anisotropy on Neutron Star Structure and Curvature gr-qc · 2025-12-30 · unverdicted · none · ref 19 · internal anchor

    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 scalar stays largely insensitive.