The large glitch from PSR 0355+54 and its post-glitch relaxation

Details The large glitch from PSR 0355+54 and its post-glitch relaxation The large glitch from PSR 0355+54 and its post-glitch relaxation

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.233...25a&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 233, July 1, 1988, p. 25-31.

Astronomy and Astrophysics

Astronomy

20

Creep Analysis, Frequency Shift, Pulsars, Superfluidity, Energy Dissipation, Equations Of Motion, Time Measurement, Vortices

Scientific paper

The authors interpret the recently observed large glitch of PSR 0355+54 and its post-glitch relaxation within the vortex creep model applied previously to the post-glitch timing data for the Crab and Vela pulsars and for PSR 0525+21. A linear response regime of vortex creep is shown to explain the post-glitch observations and is likely to be operative in parts of the neutron star crust superfluid.

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