Gravitational wave emission from rotating superfluid neutron stars
In this paper, we investigate the effect of a pinned superfluid component on the gravitational wave emission of a steadily rotating deformed neutron star. We show that the superfluid pinning allows the possibility for there to be gravitational wave emission at both the stellar spin frequency ? and i...
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| Format: | Article |
| Language: | English |
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2009-10-13.
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| Online Access: | Get fulltext |