Magnetic Field Evolution in Neutron Star Crusts: Beyond the Hall Effect

Gourgouliatos, K, De Grandis, D and Igoshev, A orcid.org/0000-0003-2145-1022 (2022) Magnetic Field Evolution in Neutron Star Crusts: Beyond the Hall Effect. Symmetry, 14 (1). 130. ISSN 2073-8994

Abstract

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Authors/Creators:
Copyright, Publisher and Additional Information: © 2022 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/).
Keywords: neutron stars; pulsars; magnetars; magnetohydrodynamics; astrophysics
Dates:
  • Accepted: 2 January 2022
  • Published (online): 11 January 2022
  • Published: January 2022
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Mathematics (Leeds) > Applied Mathematics (Leeds)
Depositing User: Symplectic Publications
Date Deposited: 07 Jan 2022 17:03
Last Modified: 14 Apr 2022 00:42
Status: Published
Publisher: MDPI
Identification Number: https://doi.org/10.3390/sym14010130

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