Glitches and pinned vorticity in the Crab pulsar

  1. M. A. Alpar*,
  2. P. W. Anderson,
  3. D. Pines,§, and
  4. J. Shaham
  1. *Physics Department, Bogazici University, Istanbul, Turkey
  2. Bell Laboratories, Murray Hill, New Jersey 07974
  3. Department of Physics, Princeton University, Princeton, New Jersey 08544
  4. Physics Department, University of Illinois, Urbana, Illinois 61801
  5. Racah Institute of Physics, Hebrew University, Jerusalem, Israel

Abstract

We suggest that the glitch behavior observed in the Crab pulsar is associated with vorticity jumps induced by a starquake or a comparable external fluctuation in the weakly pinned vortex region expected in the crust of a young neutron star, and that the differences in the glitch behavior of the Crab, Vela, and older pulsars may be explained on evolutionary grounds.

Footnotes

  • § To whom reprint requests should be addressed.

« Previous | Next Article »Table of Contents