Magnetic field evolution in magnetar crusts through three dimensional simulations

This is the latest version of this eprint.

Gourgouliatos, KN, Wood, TS and Hollerbach, R (2016) Magnetic field evolution in magnetar crusts through three dimensional simulations. Proceedings of the National Academy of Sciences, 113 (15). pp. 3944-3949. ISSN 0027-8424

Abstract

Metadata

Authors/Creators:
  • Gourgouliatos, KN
  • Wood, TS
  • Hollerbach, R
Copyright, Publisher and Additional Information: (c) 2016, The Authors. This is an author produced version of a paper published in Proceedings of the National Academy of Sciences. Uploaded in accordance with the publisher's self-archiving policy. In order to comply with the publisher requirements the University does not require the author to sign a non-exclusive licence for this paper.
Keywords: neutron stars; magnetars; Magnetohydrodynamics; pulsars
Dates:
  • Published: 12 April 2016
  • Accepted: 26 February 2016
  • Published (online): 28 March 2016
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Maths and Physical Sciences (Leeds) > School of Mathematics (Leeds) > Applied Mathematics (Leeds)
Depositing User: Symplectic Publications
Date Deposited: 04 Mar 2016 16:38
Last Modified: 16 Jan 2018 12:53
Published Version: http://dx.doi.org/10.1073/pnas.1522363113
Status: Published
Publisher: National Academy of Sciences
Identification Number: https://doi.org/10.1073/pnas.1522363113

Available Versions of this Item

  • Magnetic field evolution in magnetar crusts through three dimensional simulations. (deposited 04 Mar 2016 16:38) [Currently Displayed]

Share / Export

Statistics