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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/961

Title: The evolution of the magnetic fields of neutron stars
Authors: Bhattacharya, D.
Keywords: Neutron stars;
pulsars;
magnetic field;
Issue Date: 1995
Publisher: Indian Academy of Sciences, Bangalore, India.
Citation: Journal of Astrophysics and Astronomy, 1995, Vol. 16, p217-232.
Abstract: Observational evidence, and theoretical models of the magnetic field evolution of neutron stars is discussed. Observational data indicates that the magnetic field of a neutron star decays significantly only if it has been a member of a close interacting binary. Theoretically, the magnetic field evolution has been related to the processing of a neutron star in a binary system through the spin evolution of the neutron star, and also through the accretion of matter on the neutron star surface. I describe two specific models, one in which magnetic flux is expelled from the superconducting core during spin-down, via a copuling between Abrikosov fluxoids and Onsager-Feynman vortices; and another in which the compression and heating of the stellar crust by the accreted mass drastically reduces the ohmic decay time scale of a magnetic field configuration confined entirely to the crust. General remarks about the behaviour of the crustal field under ohmic diffusion are also made.
Description: Diamond jubilee symposium on pulsars,14-17 March 1994, RRI, Bangalore.
URI: http://hdl.handle.net/2289/961
ISSN: 0250-6335
Copyright: Indian Academy of Sciences, Bangalore, India.
Appears in Collections:Research Papers (A&A)

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