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Supernova neutrino fluxes in HALO-1kT, Super-Kamiokande, and JUNO
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Supernova neutrino fluxes in HALO-1kT, Super-Kamiokande, and JUNO
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Paper
Supernova neutrino fluxes in HALO-1kT, Super-Kamiokande, and JUNO
2021
Overview
When the next galactic core-collapse supernova occurs, we must be ready to obtain as much information as possible. Although many present and future detectors are well equipped to detect \\(_e\\) and \\(_x\\) neutrinos, the detection of the \\(_e\\) species presents the biggest challenges. We assess the impact that a 1 ktonne lead-based detector, such as HALO-1kT, can have in constraining electron neutrino time-integrated fluxes. The study involves the detector taken alone as well as when combined with massive \\(_e\\)-sensitive detectors such as Super-Kamiokande and JUNO. We find that HALO-1kT alone is not able to strongly constrain the emission parameters. When combined with other detectors, however, the orthogonal information might be helpful in improving the \\(_e\\) total emitted energy and mean energy accuracy, up to about \\(50\\%\\), if no other \\(_e\\)-sensitive channel is implemented. A discussion on the reconstruction of \\(_e\\) and \\(_x\\) species, as well as the total emitted energy, is also presented.
