Gamma-Ray Bursts from Neutron Star Kicks

Abstract

The idea that gamma-ray bursts might be a kind of phenomena associated with neutron star kicks was first proposed by Dar & Plaga (1999). Here we study this mechanism in more detail and point out that the neutron star should be a high speed one (with proper motion larger than $\sim 1000$ km/s). It is shown that the model agrees well with observations in many aspects, such as the energetics, the event rate, the collimation, the bimodal distribution of durations, the narrowly clustered intrinsic energy, and the association of gamma-ray bursts with supernovae and star forming regions. We also discuss the implications of this model on the neutron star kick mechanism, and suggest that the high kick speed were probably acquired due to the electromagnetic rocket effect of a millisecond magnetar with an off-centered magnetic dipole.

12 pages, no figures, ApJ in press (minor revision with respect to Version 2)

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• Pulsar's kicks and Gamma-ray bursts
• Progenitors of Long-Duration Gamma-ray Bursts
• Distribution of gamma-ray bursts on the t90-hardness ratio plane and their classification revisited
• Beaming effects in GRBs and orphan afterglows
• Some statistical remarks on GRBs jointly detected by Fermi and Swift satellites