The Largest Pulsar Glitch and the Universality of Glitch Behavior

Details The Largest Pulsar Glitch and the Universality of Glitch Behavior The Largest Pulsar Glitch and the Universality of Glitch Behavior

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1379..166a&link_type=abstract

ASTROPHYSICS OF NEUTRON STARS 2010: A Conference in Honor of M. Ali Alpar. AIP Conference Proceedings, Volume 1379, pp. 166-174

Astronomy and Astrophysics

Astrophysics

Magellanic Clouds, Superfluidity, X-Ray Sources (Astronomical), Gamma-Ray Sources (Astronomical), Magellanic Stream, Hydrodynamic Aspects Of Superfluidity, Quantum Fluids, X-Ray Sources, X-Ray Bursts, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

Several recent observations of pulsar glitches indicate rich and intriguing new types of behavior added to the reservoir of large glitches with seemingly universal behavior explained by the vortex creep and unpinning model. The very large recent glitch in PSR B2334+61 gives detailed information on the universal glitch and post-glitch behavior of isolated pulsars. The implied moment of inertia distribution of the neutron star components active in glitch dynamics provides new clues and raises interesting questions.

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