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arxiv: 1705.00508 · v2 · pith:F7LAPXVXnew · submitted 2017-05-01 · 🌌 astro-ph.HE

Evolution of the magnetic field in neutron stars

M.E. Gusakov , E.M. Kantor , D.D. Ofengeim (Ioffe Institute) This is my paper
classification 🌌 astro-ph.HE
keywords fieldmagneticevolutionneutronstarsapproachcalculationcores
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We propose a general method to self-consistently study the quasistationary evolution of the magnetic field in the cores of neutron stars. The traditional approach to this problem is critically revised. Our results are illustrated by calculation of the typical timescales for the magnetic field dissipation as functions of temperature and the magnetic field strength.

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

  1. Magnetic field dynamics in isolated neutron stars with an external dipole field

    astro-ph.HE 2026-05 unverdicted novelty 5.0

    Long-term numerical relativity simulations find that neutron star magnetic fields relax to stable mixed configurations with toroidal energy fraction ≲10% within one Alfvén time after Tayler instability saturation.