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Postglitch relaxation

Several theories were proposed in the past to describe the postglitch relaxation of pulsars angular velocity. Each physical model considers the spin-down of the superfluid in a different way. Alpar et al. [3, 4] suggest that the crustal superfluid is responsible for the glitches and postglitch relaxation they describe the dynamical properties of the crust superfluid in terms of a thermal... [Pg.45]

See other pages where Postglitch relaxation is mentioned: [Pg.44]    [Pg.44]    [Pg.45]    [Pg.46]    [Pg.46]    [Pg.47]    [Pg.48]    [Pg.50]    [Pg.52]    [Pg.44]    [Pg.44]    [Pg.45]    [Pg.46]    [Pg.46]    [Pg.47]    [Pg.48]    [Pg.50]    [Pg.52]   
See also in sourсe #XX -- [ Pg.44 , Pg.46 ]



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