Gadolinium in water Cherenkov detectors improves detection of supernova νₑ

الأصل · EN

Detecting supernova νₑ is essential for testing supernova and neutrino physics, but the yields are small and the backgrounds from other channels large, e.g., 10² and 10⁴ events, respectively, in Super-Kamiokande. We develop a new way to isolate supernova νₑ, using gadolinium-loaded water Cherenkov detectors. The forward-peaked nature of νₑ + e- → νₑ + e- allows an angular cut that contains the majority of events. Even in a narrow cone, near-isotropic inverse beta events, νₑ + p → e+ + n, are a large background. With neutron detection by radiative capture on gadolinium, the background events can be individually identified with high efficiency. The remaining backgrounds are smaller and can be measured separately, so they can be statistically subtracted. Super-Kamiokande with gadolinium could measure the total and average energy of supernova νₑ with 20% precision or better each (90% C.L.). Hyper-Kamiokande with gadolinium could improve this by a factor of 5. This precision will allow powerful tests of supernova neutrino emission, neutrino mixing, and exotic physics. Unless very large liquid argon or liquid scintillator detectors are built, this is the only way to guarantee precise measurements of supernova νₑ.