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arXiv · hep-ph/0612221

Supernovae, Landau Levels, and Pulsar Kicks

Leonard S. Kisslinger
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Abstract

We derive the energy asymmetry given the proto-neutronstar during the time when the neutrino sphere is near the surface of the proto-neutron star, using the modified URCA process. The electrons produced with the anti-neutrinos are in Landau levels due to the strong magnetic field, and this leads to asymmetry in the neutrino momentum, and a pulsar kick. Our main prediction is that the large pulsar kicks start at about 10 s and last for about 10 s, with the corresponding neutrinos correlated in the direction of the magnetic field.

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Leonard S. Kisslinger. 2006-12-18. Supernovae, Landau Levels, and Pulsar Kicks. https://doi.org/10.1142/s0217732307025315

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