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arxiv: 1709.07106 · v1 · pith:I5YDDC6Jnew · submitted 2017-09-21 · 🌌 astro-ph.HE

Magnetic Fields of Neutron Stars

Sushan Konar This is my paper
classification 🌌 astro-ph.HE
keywords neutronstarsclassesevolutionfieldsmagneticarticlebasically
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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.

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

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

    nucl-th 2025-10 unverdicted novelty 7.0

    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.