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Observational constraints on the role of the crust in the post-glitch relaxation

โœ Scribed by M. Jahan-Miri

Publisher
Elsevier Science
Year
2005
Tongue
English
Weight
173 KB
Volume
11
Category
Article
ISSN
1384-1076

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โœฆ Synopsis

The observed large rates of spinning down after glitches in some radio pulsars have been previously explained in terms of a long-term spin-up behavior of a superfluid part of the crust of neutron stars. We argue that the suggested mechanism is not viable; being inconsistent with the basic requirements for a superfluid spin-up, in addition to its quantitative disagreement with the data. Hence, the observed post-glitch relaxations may not be interpreted due only to the effects of the stellar crust.

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