Pith. sign in

REVIEW 2 cited by

Magnetic Fields of Neutron Stars

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 1709.07106 v1 pith:I5YDDC6J submitted 2017-09-21 astro-ph.HE

Sushan Konar This is my paper · ORCID
classification astro-ph.HE
keywords neutronstarsclassesevolutionfieldsmagneticarticlebasically
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

This article briefly reviews our current understanding of the evolution of magnetic fields in neutron stars, which basically defines the evolutionary pathways between different observational classes of neutron stars. The emphasis here is on the evolution in binary systems and the newly emergent classes of millisecond pulsars.

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. Full citation record

  1. Thermal and Magnetic effects on Bulk Viscosity in Binary Neutron Star Mergers

    nucl-th 2025-10 unverdicted novelty 7.0 of 10

    Magnetic fields modify bulk viscous dissipation in post-merger neutron star matter by altering direct and modified Urca rates at finite temperature beyond the Fermi surface approximation.

  2. Transport properties in binary neutron star mergers: Effect of magnetic field

    nucl-th 2026-08 conditional novelty 5.0 of 10

    Magnetic fields up to 5e17 G increase charged-current neutrino and antineutrino opacities in neutron star merger matter by up to two orders of magnitude at low temperature, shrinking neutrino mean free paths.

Pith tools