Gadolinium in water Cherenkov detectors improves detection of supernova νe

Detecting supernova nu(e) is essential for testing supernova and neutrino physics, but the yields are small and the backgrounds from other channels large, e.g., similar to 10(2) and similar to 10(4) events, respectively, in Super-Kamiokande. We develop a new way to isolate supernova nu(e), using gadolinium-loaded water Cherenkov detectors. The forward-peaked nature of nu(e) + e(-) -> nu(e) + e(-) allows an angular cut that contains the majority of events. Even in a narrow cone, near-isotropic inverse beta events, (nu) over bar (e) + p -> e(+) + n, are a large background. With neutron detection by radiative capture on gadolinium, these 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 nu(e) with similar to 20% precision or better each (90% C.L.). Hyper-Kamiokande with gadolinium could improve this by a factor of similar to 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 nu(e).