Kick velocity induced by magnetic dipole and quadrupole radiation
arXiv:1012.1376 · doi:10.1088/0004-637X/728/2/75
Abstract
We examine the recoil velocity induced by the superposition of the magnetic dipole and quadrupole radiation from a pulsar/magnetar born with rapid rotation. The resultant velocity depends on not the magnitude, but rather the ratio of the two moments and their geometrical configuration. The model does not necessarily lead to high spatial velocity for a magnetar with a strong magnetic field, which is consistent with the recent observational upper bound. The maximum velocity predicted with this model is slightly smaller than that of observed fast-moving pulsars.
10 pages, 3 color figures
References in corpus (5)
- Magnetic field generation in fully convective rotating spheres
- Getting Its Kicks: A VLBA Parallax for the Hyperfast Pulsar B1508+55
- Protoneutron star dynamos: pulsars, magnetars, and radio-silent X-ray emitting neutron stars
- Numerical Simulations of Equatorially-Asymmetric Magnetized Supernovae: Formation of Magnetars and Their Kicks
- Constraining the Proper Motions of Two Magnetars