Thermal spectra can be produced by certain classes of emission kernels without probe thermalization, as when the differential cross section depends on angle but not on the Mandelstam variable s, providing a kernel-based criterion to distinguish genuine equilibrium from kernel artifacts.
Reactor Neutrino Spec- tra
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A 2023 reactor antineutrino flux calculation revives the Reactor Antineutrino Anomaly to 2.2 sigma and produces 3.8 sigma tension with gallium data that drops to 1.3 sigma when gallium uncertainties are enlarged.
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Thermal Spectra Without Detailed Balance
Thermal spectra can be produced by certain classes of emission kernels without probe thermalization, as when the differential cross section depends on angle but not on the Mandelstam variable s, providing a kernel-based criterion to distinguish genuine equilibrium from kernel artifacts.
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Revival of the Reactor Antineutrino Anomaly
A 2023 reactor antineutrino flux calculation revives the Reactor Antineutrino Anomaly to 2.2 sigma and produces 3.8 sigma tension with gallium data that drops to 1.3 sigma when gallium uncertainties are enlarged.