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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1533

Title: Ohmic decay of magnetic flux expelled from neutron star interiors
Authors: Bhattacharya, D.
Datta, Bhaskar
Keywords: MAGNETIC FIELDS - STARS,
NEUTRON - PULSARS,GENERAL.
Issue Date: Oct-1996
Publisher: Blackwell Publishing for the Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 1996, Vol.282, p1059-1063
Abstract: We study Ohmic diffusion of magnetic flux expelled from the superconducting core of a neutron star to its crust owing to spindown-induced field evolution. We find that Ohmic decay time-scales in the range 10^7.5-10^9 yr obtain for a wide range of crustal temperatures and impurity concentrations for various equation of state models of neutron star matter. This result is in agreement with the Ohmic time-scale that appears to be required to explain observed magnetic field strengths of isolated and binary neutron stars in the spindown-induced magnetic flux expulsion scenario.
Description: Sorry, the full text of this article is not available here. Please click on the alternative location to access it.
URI: http://hdl.handle.net/2289/1533
ISSN: 0035-8711
Alternative Location: http://adsabs.harvard.edu/cgi-bin/bib_query?1996MNRAS.282.1059B
http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996MNRAS.282.1059B&link_type=ARTICLE&db_key=AST
Copyright: (1996) Royal Astronomical Society
Appears in Collections:Research Papers (A&A)

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