Simulated magnetic field expulsion in neutron star cores

Please use this identifier to cite or link to this item:
Información del item - Informació de l'item - Item information
Title: Simulated magnetic field expulsion in neutron star cores
Authors: Elfritz, Justin G. | Pons, José A. | Rea, Nanda | Glampedakis, Konstantinos | Viganò, Daniele
Research Group/s: Astrofísica Relativista
Center, Department or Service: Universidad de Alicante. Departamento de Física Aplicada
Keywords: Methods: numerical | Stars: evolution | Stars: magnetars | Stars: magnetic field | Stars: neutron
Knowledge Area: Astronomía y Astrofísica
Issue Date: 11-Mar-2016
Publisher: Oxford University Press
Citation: Monthly Notices of the Royal Astronomical Society. 2016, 456(4): 4461-4474. doi:10.1093/mnras/stv2963
Abstract: The study of long-term evolution of neutron star (NS) magnetic fields is key to understanding the rich diversity of NS observations, and to unifying their nature despite the different emission mechanisms and observed properties. Such studies in principle permit a deeper understanding of the most important parameters driving their apparent variety, e.g. radio pulsars, magnetars, X-ray dim isolated NSs, gamma-ray pulsars. We describe, for the first time, the results from self-consistent magnetothermal simulations considering not only the effects of the Hall-driven field dissipation in the crust, but also adding a complete set of proposed driving forces in a superconducting core. We emphasize how each of these core-field processes drive magnetic evolution and affect observables, and show that when all forces are considered together in vectorial form, the net expulsion of core magnetic flux is negligible, and will have no observable effect in the crust (consequently in the observed surface emission) on megayear time-scales. Our new simulations suggest that strong magnetic fields in NS cores (and the signatures on the NS surface) will persist long after the crustal magnetic field has evolved and decayed, due to the weak combined effects of dissipation and expulsion in the stellar core.
Sponsor: J.G.E. and N.R. are funded by an NWO Vidi grant (PI: Rea). J.A.P. is funded by the grants AYA2013-42184-P and Prometeu/2014/6. N.R. and D.V. acknowledge support from the grants AYA2012-39303 and SGR 2014-1073. K.G. is supported by the Ramón y Cajal Programme of the Spanish Ministerio de Ciencia e Innovación. Authors also wish to acknowledge NewCompStar, COST action MP1304 for partial funding of this research.
ISSN: 0035-8711 (Print) | 1365-2966 (Online)
DOI: 10.1093/mnras/stv2963
Language: eng
Type: info:eu-repo/semantics/article
Rights: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Peer Review: si
Publisher version:
Appears in Collections:INV - Astrofísica Relativista - Artículos de Revistas

Files in This Item:
Files in This Item:
File Description SizeFormat 
Thumbnail2016_Elfritz_etal_MNRAS_rev.pdfVersión revisada4,39 MBAdobe PDFOpen Preview

Items in RUA are protected by copyright, with all rights reserved, unless otherwise indicated.