Supernovae, Landau Levels, and Pulsar Kicks

Details Supernovae, Landau Levels, and Pulsar Kicks Supernovae, Landau Levels, and Pulsar Kicks

2006-12-18

arxiv.org/abs/hep-ph/0612221v1

Mod.Phys.Lett.A22:2071-2080,2007

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages, seven figures

Scientific paper

10.1142/S0217732307025315

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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