Relaxation of the Angular Velocity of Pulsars after Glitches View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2014-03

AUTHORS

D. M. Sedrakian, M. V. Hayrapetyan, D. Baghdasaryan

ABSTRACT

The rotational dynamics of superfluid neutron stars is examined in order to study the relaxation of the angular velocity of pulsars after glitches. The motion of the neutron-proton vortex system is investigated taking the sphericity of the superfluid core and vortex pinning and depinning into account. A relaxation solution is obtained for the angular rotation velocity of pulsars after glitches. In order to compare this solution with observational data for the Vela pulsar, the inverse problem of finding the initial distribution of vortices immediately after a glitch is solved. More... »

PAGES

90-104

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s10511-014-9317-x

DOI

http://dx.doi.org/10.1007/s10511-014-9317-x

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1032164940


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