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