Postglitch behavior of the Crab pulsar - Evidence for external torque variations

Details Postglitch behavior of the Crab pulsar - Evidence for external torque variations Postglitch behavior of the Crab pulsar - Evidence for external torque variations

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...390l..21l&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 390, no. 1, May 1, 1992, p. L21, L22. Research sponsored by DOE.

Physics

Condensed Matter

23

Condensed Matter Physics, Crab Nebula, Pulsars, Stellar Interiors, Torque, Angular Momentum, Stellar Magnetic Fields, Stellar Magnetospheres, Stellar Rotation, Superfluidity

Scientific paper

Attention is given to the persistent offset in the spin-down rate of the Crab pulsar following the 1975 glitch which is difficult to explain by the usually assumed dynamic coupling between the crust and the superfluid interior. One explanation of the observed behavior is an increase in the external torque caused by a rearrangement of the stellar magnetic field.

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