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arXiv · hep-ph/9711206

Electron neutrino opacity in magnetised media

Abstract

We study the effects of strong magnetic fields ($B> 10^{13}$~G) in the cross section for $ν_e n\to p e$ scattering in the presence of a degenerate electron background. This can be relevant for the $ν_e$ propagation in the proto-neutron star stage after supernovae collapse. We find that for field strengths $B> 10^{16}$~G$(E_ν/10$ MeV$)^2$ the $ν_e$ opacity is sizeably affected by the magnetic field and can lead to a shift in the location of the electron neutrino sphere towards lower densities. We discuss the implications that this may have for scenarios proposed to explain the observed pulsar velocities.

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Esteban Roulet. 1997-11-03. Electron neutrino opacity in magnetised media. https://doi.org/10.1088/1126-6708%2F1998%2F01%2F013

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