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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2816
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dc.contributor.authorBhattacharya, D-
dc.contributor.authorDatta, B-
dc.date.accessioned2008-07-22T11:37:08Z-
dc.date.available2008-07-22T11:37:08Z-
dc.date.issued1996-10-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 282, No. 3, pp. 1059 - 1063en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/2816-
dc.description.abstractWe 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 scenarioen
dc.format.extent860343 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherRoyal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996MNRAS.282.1059Ben
dc.subjectMagnetic fields - starsen
dc.subjectNeutron - pulsarsen
dc.subjectGeneralen
dc.titleOhmic decay of magnetic flux expelled from neutron star interiorsen
dc.typeArticleen
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