Resonant dark photon production in the gain layer of a core-collapse supernova can quench the neutrino-driven shock revival, yielding constraints that supersede the SN1987A cooling bound for masses around 0.1-0.4 MeV.
Janka, Neutrino-Driven Explosions , in Handbook of Supernovae (A
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Cooling the Shock: New Supernova Constraints on Dark Photons
Resonant dark photon production in the gain layer of a core-collapse supernova can quench the neutrino-driven shock revival, yielding constraints that supersede the SN1987A cooling bound for masses around 0.1-0.4 MeV.