pith. sign in

arxiv: hep-th/0510181 · v2 · submitted 2005-10-21 · ✦ hep-th · astro-ph· hep-ph

Production of Neutral Fermion in Linear Magnetic Field through Pauli Interaction

classification ✦ hep-th astro-phhep-ph
keywords magneticproductionfieldsrategradientinteractionneutralpauli
0
0 comments X
read the original abstract

We calculate the production rate of neutral fermions in linear magnetic fields through the Pauli interaction. It is found that the production rate is exponentially decreasing function with respect to the inverse of the magnetic field gradient, which shows the non-perturbative characteristics analogous to the Schwinger process. It turns out that the production rate density depends on both the gradient and the strength of magnetic fields in 3+1 dimension. It is quite different from the result in 2+1 dimension, where the production rate depends only on the gradient of the magnetic fields, not on the strength of the magnetic fields. It is also found that the production of neutral fermions through the Pauli interaction is a magnetic effect whereas the production of charged particles through minimal coupling is an electric effect.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Gradient-Produced Neutrinos

    hep-ph 2026-04 unverdicted novelty 5.0

    Steep matter-density gradients in neutron stars can produce neutrino-antineutrino pairs analogous to the Schwinger effect.