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• W1945484683 abstract "We present analytic calculations of the electromagnetic torques acting on a magnetic neutron star rotating in vacuum, including near-zone torques associated with the inertia of dipole and quadrupole magnetic fields. We incorporate these torques into the rotational dynamics of a rigid-body neutron star, and show that the effects of the inertial torque can be understood as a modification of the moment of inertia tensor of the star. We apply our rotational dynamics equation to the Crab pulsar, including intrinsic distortions of the star and various electromagnetic torques, to investigate the possibility that the counter-alignment of the magnetic inclination angle, as suggested by recent observations, could be explained by pulsar precession. We find that if the effective principal axis of the pulsar is nearly aligned with either the magnetic dipole axis or the rotation axis, then precession may account for the observed counter-alignment over decade timescales. Over the spindown timescale of the pulsar, the magnetic inclination angle always decreases." @default.
• W1945484683 created "2016-06-24" @default.
• W1945484683 creator A5007773051 @default.
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• W1945484683 date "2015-05-28" @default.
• W1945484683 modified "2023-10-16" @default.
• W1945484683 title "Electromagnetic torques, precession and evolution of magnetic inclination of pulsars" @default.
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• W1945484683 doi "https://doi.org/10.1093/mnras/stv955" @default.
• W1945484683 hasPublicationYear "2015" @default.
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