Vortex structures in neutron stars : or how I learned to stop worrying and just write it already

We suggest a mechanism that may resolve a conflict between the precession of a neutron star and the widely accepted idea that protons in the bulk of the neutron star form a type-II superconductor. We will show that if there is a persistent, non-dissipating current running along the magnetic flux...

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Bibliographic Details
Main Author: Charbonneau, James
Language:English
Published: University of British Columbia 2011
Online Access:http://hdl.handle.net/2429/32046

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