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Coherent elastic neutrino-nucleus scattering (CEvNS), the gentlest kind of interaction of a neutrino with an entire nucleus, was first predicted in 1974, but not observed until 2017 by the COHERENT collaboration. COHERENT and many other experiments are pursuing further measurements of this low momentum transfer process. We review the physics motivations for these measurements and prospects and status of current and future CEvNS experiments.

I describe physics potential and experimental prospects for coherent elastic neutrino-nucleus scattering (CEvNS), a process which has not yet been observed. Germanium- based detectors represent a promising technology for CEvNS experiments. I focus primarily on stopped-pion neutrino sources.

Alec Habig and Kate Scholberg describe the Supernova Early Warning System (SNEWS), an international network of neutrino detectors set up to provide a fast alert to the astronomical community if the participating experiments detect the distinctive burst of neutrinos from a stellar core collapse in or near the Milky Way.Alec Habig and Kate Scholberg describe the Supernova Early Warning System (SNEWS), an international network of neutrino detectors aimed to alert the astronomical community if supernova neutrinos are detected.

This joint neutrino-gravitational wave session talk will describe current, near future and farther future supernova neutrino detectors. I will comment on the potential of future supernova neutrino-gravitational wave correlation searches.

A new generation of large underground detectors is being planned to further investigate neutrino mass and mixing and to search for possible CP violation that may provide a hint to the origin of our asymmetric universe. Such detectors would also investigate neutrinos in nature - from the earth's crust to supernovae. The physics case for such a program is presented and plans for detectors worldwide are summarized.

When a massive star collapses at the end of its life, nearly all of the gravitational binding energy of the resulting remnant is released in the form of neutrinos. The burst of neutrinos from a Galactic core collapse supernova will be detected in neutrino detectors worldwide. This talk will cover supernova neutrino detection techniques in general, current supernova neutrino detectors, and prospects for specific future experiments.

This talk will describe sensitivity of past, current and future water Cherenkov detectors to a burst of supernova neutrinos.

When a massive star collapses at the end of its life, nearly all of the gravitational binding energy of the resulting remnant is released in the form of neutrinos. The burst of neutrinos from a Galactic core collapse supernova will be detected in neutrino detectors worldwide. This talk will cover supernova neutrino detection techniques in general, current supernova neutrino detectors, and prospects for specific future experiments.

A new generation of large underground detectors is being planned to further investigate neutrino mass and mixing and to search for possible CP violation that may provide a hint to the origin of our asymmetric universe. Such detectors would also investigate neutrinos in nature - from the earth's crust to supernovae. The physics case for such a program is presented and plans for detectors worldwide are summarized.

This talk will summarize the current experimental understanding of neutrino mass and oscillation parameters, and will discuss prospects for future experiments.