Neutrino physics spans an enormous range of energies and scales: from detection of low-energy cosmic neutrinos; to keV-scale recoils in coherent neutrino scattering; to MeV-scale solar, reactor, and neutrinoless double beta decay events; to GeV and TeV-scale detection of neutrinos from accelerators and the atmosphere; to cosmic sources in the PeV-ZeV range. While any particular experiment tends to focus on just one or two detection approaches, the great breadth of neutrino physics means that there is an equally broad spectrum of neutrino detection technologies and methodologies.At any one time, there are a dozen or more medium-to large-scale neutrino detectors operating worldwide, several more in the design or construction phases, and many future detectors planned. Beyond this are a diverse set of smaller scale prototypes distributed across universities and labs.The focus in this report is on new technologies and approaches that will enable future neutrino detectors, and thus experiments that are already built and running, are under construction, or for which technical designs exist are not discussed in great detail.
Recommendations for Next-Generation Neutrino DetectorsWhile there are many exciting detectors and enabling technologies described in this report, there are a few ideas that have had a particularly large community interest, and we formulate these into a set of recommendations below: 1 Future Advances in Photon-Based Neutrino Detectors arXiv:2203.07479 2 Coherent elastic neutrino-nucleus scattering: Terrestrial and astrophysical applications arXiv:2203.07361 3 Recoil imaging for dark matter, neutrinos, and physics beyond the Standard Model arXiv:2203.05914 4 Low-Energy Physics in Neutrino LArTPCs arXiv:2203.00740 5 SoLAr: Solar Neutrinos in Liquid Argon arXiv:2203.07501 6 Low Background kTon-Scale Liquid Argon Time Projection Chambers arXiv:2203.08821 7 Measuring the Neutrino Event Time in Liquid Argon by a Post-Reconstruction One-parameter Fit