Pith. sign in

REVIEW 2 cited by

Screening corrections to the Coulomb crystal elastic moduli

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1603.04227 v1 pith:AGDAJ4QG submitted 2016-03-14 astro-ph.SR astro-ph.HE

D. A. Baiko This is my paper · ORCID
classification astro-ph.SRastro-ph.HE
keywords electronscreeningcorrectionscoulombcrustcrystalelasticmoduli
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Corrections to elastic moduli, including the effective shear modulus, of a solid neutron star crust due to electron screening are calculated. At any given mass density, the crust is modelled as a body-centred cubic Coulomb crystal of fully ionized atomic nuclei of a single type with a polarizable charge-compensating electron background. Motion of the nuclei is neglected. The electron polarization is described by a simple Thomas-Fermi model of exponential electron screening. The results of numerical calculations are fitted by convenient analytic formulae. They should be used for precise neutron star oscillation modelling, a rapidly developing branch of stellar seismology.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 10 citations worldwide. Full citation record

  1. Constraining shear modulus of polycrystalline neutron star crust: Hashin-Shtrikman variational approach

    astro-ph.HE 2025-07 accept novelty 6.0 of 10

    Hashin-Shtrikman variational bounds show that the effective shear modulus of a polycrystalline neutron star crust is lower than the commonly assumed Voigt value, with narrower upper and lower limits.

  2. 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.

Pith tools