Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2816
Title: Ohmic decay of magnetic flux expelled from neutron star interiors
Authors: Bhattacharya, D
Datta, B
Keywords: Magnetic fields - stars;Neutron - pulsars;General
Issue Date: Oct-1996
Publisher: Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, Vol. 282, No. 3, pp. 1059 - 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
URI: http://hdl.handle.net/2248/2816
ISSN: 0035-8711
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/1996MNRAS.282.1059B
Appears in Collections:IIAP Publications

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