SN1987A Pulsar Velocity From Modified URCA Processes and Landau Levels

Astronomy; Carnegie Mellon University) Sandip Pakvasa (Department of Physics; Honolulu); Leonard S Kisslinger (Department of Physics; University of Hawaii at Manoa

arxiv: 0802.1689 · v1 · submitted 2008-02-12 · 🌌 astro-ph

SN1987A Pulsar Velocity From Modified URCA Processes and Landau Levels

Leonard S Kisslinger (Department of Physics , Carnegie Mellon University) Sandip Pakvasa (Department of Physics , Astronomy , University of Hawaii at Manoa , Honolulu) This is my paper

classification 🌌 astro-ph

keywords velocitylevelsmodifiedneutrinosprocessespulsarsn1987aurca

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Using a recent estimate of the velocity of pulsars arising from neutrinos emitted with modified URCA processes with electrons in Landua levels, and the temperture of the protoneutron star created by SN1987A, derived from the energy of the observed neutrinos, we predict the velocity of the resulting pulsar.

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SN1987A Pulsar Velocity From Modified URCA Processes and Landau Levels

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