Steep matter-density gradients in neutron stars can produce neutrino-antineutrino pairs analogous to the Schwinger effect.
S1, S2, and S6, we pro- vide derivations of the production rate neglecting the chiral mixing while keeping the mass dependence in each chiral sector
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Gradient-Produced Neutrinos
Steep matter-density gradients in neutron stars can produce neutrino-antineutrino pairs analogous to the Schwinger effect.