[94–96], whose leading-order rates are pro- portional to the particle’s mass squared

We note that our pair-production rates differ from those of,e

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hep-ph · 2026-04-23 · unverdicted · novelty 5.0

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

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Gradient-Produced Neutrinos hep-ph · 2026-04-23 · unverdicted · none · ref 33
Steep matter-density gradients in neutron stars can produce neutrino-antineutrino pairs analogous to the Schwinger effect.