Pre-Supernova Alert System for Super-Kamiokande
arXiv:2205.09881 · doi:10.3847/1538-4357/ac7f9c
Abstract
In 2020, the Super-Kamiokande (SK) experiment moved to a new stage (SK-Gd) in which gadolinium (Gd) sulfate octahydrate was added to the water in the detector, enhancing the efficiency to detect thermal neutrons and consequently improving the sensitivity to low energy electron anti-neutrinos from inverse beta decay (IBD) interactions. SK-Gd has the potential to provide early alerts of incipient core-collapse supernovae through detection of electron anti-neutrinos from thermal and nuclear processes responsible for the cooling of massive stars before the gravitational collapse of their cores. These pre-supernova neutrinos emitted during the silicon burning phase can exceed the energy threshold for IBD reactions. We present the sensitivity of SK-Gd to pre-supernova stars and the techniques used for the development of a pre-supernova alarm based on the detection of these neutrinos in SK, as well as prospects for future SK-Gd phases with higher concentrations of Gd. For the current SK-Gd phase, high-confidence alerts for Betelgeuse could be issued up to nine hours in advance of the core-collapse itself.
20 pages
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Cited by in corpus (5)
- The Science of the Einstein Telescope
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- Combined Pre-Supernova Alert System with Kamland and Super-Kamiokande
- Supernova model discrimination with a kilotonne-scale Gd-HO Cherenkov detector
- Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase