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Experimental Nuclear Masses and the Ground State of Cold Dense Matter

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arxiv nucl-th/9310003 v1 pith:NIUBUXBO submitted 1993-10-04 nucl-th astro-ph

Pawel HAENSEL , Bernard PICHON CNRS (Observatoire de Paris-Meudon) This is my paper
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abstract

We study the consequences of recent progress in the experimental determination of masses of neutron rich nuclei for our knowledge of the ground state of cold dense matter. The most recent experimental data determine the ground state of cold dense matter up to $ \rho \simeq 10^{11}~{\rm g~cm^{-3}} $. The composition and the equation of state of the ground state of matter, in this density interval, are calculated.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 67 citations worldwide. Full citation record

  1. Bayesian analysis of the shear modulus in the neutron-star crust

    astro-ph.HE 2026-06 unverdicted novelty 4.0 of 10

    Bayesian modeling with informed priors reduces uncertainties in neutron-star crust shear properties, predicting torsional mode frequencies of 20-50 Hz compatible with observations.

  2. Crust (Unified) Tool for Equation-of-state Reconstruction (CUTER) v2

    astro-ph.HE 2025-06 accept novelty 4.0 of 10

    CUTER v2 reconstructs the missing or inconsistent low-density crust of arbitrary neutron-star equations of state, producing unified EoSs whose global properties match original models to within about one percent.

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