Neutrino Transport in Strongly Magnetized Proto-Neutron Stars and the Origin of Pulsar Kicks: I. The Effect of Parity Violation in Weak Interactions

Preprint

21 June 1998

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/9802344

Abstract

The original paper describes neutrino cooling calculations in the presence of asymmetric neutrino opacities due to parity violation in strong magnetic fields. In early April, through the work of P. Arras and D. Lai at Cornell (see astro-ph/9806285) we became aware that the paper contains a serious flaw: although the neutrino scattering opacities depend asymmetrically on the initial and final neutrino momenta, detailed balance requires that there be no cumulative effect from multiple scatterings in the bulk interior of the proto-neutron star where local thermodynamic equilibrium applies to a good approximation. This paper was therefore withdrawn from ApJ in April. Also in April, we submitted an erratum to ApJ Lett. pointing out this error. (The erratum will appear in the July 1, 1998 issue of ApJ Lett.)

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