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Recent Progress in Neutron Star Theory

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arxiv astro-ph/0003276 v1 pith:63OHCY3K submitted 2000-03-20 astro-ph nucl-th

H. Heiselberg (Nordita) , V. Pandharipande (Urbana) This is my paper · ORCID
classification astro-phnucl-th
keywords matterneutronstartheorychapterscontainsdensedensity
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This review contains chapters discussing: Energy density fluctionals of nuclear matter, Many-body theory of nucleon matter, Hadronic and quark matter, Mixtures of phases in dense matter, Neutron star observations and predictions.

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Cited by 2 Pith papers

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

  1. Nonradial oscillations of realistic anisotropic neutron stars: Axial modes

    gr-qc 2026-05 unverdicted novelty 5.0 of 10

    Axial modes of anisotropic neutron stars show mass-scaled frequency and damping time with nearly universal quadratic dependence on compactness, insensitive to EOS and anisotropy model.

  2. Rotating neutron stars: anisotropy model comparison

    astro-ph.HE 2025-04 conditional novelty 5.0 of 10

    Anisotropic pressure can raise the maximum stable neutron-star mass by 50-60 percent in the covariant model, and normalized moment of inertia and binding energy follow nearly model-independent fits.

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