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29 March 2024
 
  » arxiv » astro-ph/0312542

 Article overview


Neutron Star Kicks and Supernova Asymmetry
Dong Lai ;
Date 19 Dec 2003
Subject astro-ph
AffiliationCornell
AbstractObservations over the last decade have shown that neutron stars receive a large kick velocity (of order a hundred to a thousand km/s) at birth. The physical origin of the kicks and the related supernova asymmetry is one of the central unsolved mysteries of supernova research. We review the physics of different kick mechanisms, including hydrodynamically driven, neutrino -- magnetic field driven, and electromagnetically driven kicks. The viabilities of the different kick mechanisms are directly related to the other key parameters characterizing nascent neutron stars, such as the initial magnetic field and the initial spin. Recent observational constraints on kick mechanisms are also discussed.
Source arXiv, astro-ph/0312542
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