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  Are Pulsar Glitches Triggered by a Superfluid Two-Stream Instability?

Andersson, N., Comer, G. L., & Prix, R. (2003). Are Pulsar Glitches Triggered by a Superfluid Two-Stream Instability? Physical Review Letters, 90(9): 091101. doi:10.1103/PhysRevLett.90.091101.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5246-4 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5247-2
Genre: Journal Article

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 Creators:
Andersson, Nils, Author
Comer, G. L., Author
Prix, Reinhard1, Author              
Affiliations:
1Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24011              

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 Abstract: Mature neutron stars are expected to have several superfluid components. Strong evidence for this is provided by the glitches that have been observed in dozens of pulsars. We describe a superfluid analog of the two-stream instability that is well known in plasma physics and provide arguments that this instability is likely to be relevant for neutron stars. This is a new physical mechanism which may play a key role in explaining the glitch mechanism and which could also prove to be relevant in laboratory experiments on various superfluid systems.

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 Dates: 2003-03-06
 Publication Status: Published in print
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 Identifiers: eDoc: 379322
Other: arXiv:astro-ph/0210486v1
DOI: 10.1103/PhysRevLett.90.091101
URI: http://link.aps.org/abstract/PRL/v90/e091101
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Title: Physical Review Letters
Source Genre: Journal
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Pages: - Volume / Issue: 90 (9) Sequence Number: 091101 Start / End Page: - Identifier: -