Exploring Neutrino Physics and Beyond with Observables and Detectors
Delve into the realm of neutrino physics, nuclear recoils, and other phenomena like sterile neutrino oscillations using detectors such as BSM and single-phase LAr inelastic NC/CC interactions. From NSI to Supernova-relevant cross-sections and accelerator-produced DM, this research journey covers a wide array of topics relevant to modern physics experiments and observations.
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Presentation Transcript
Physics we are after Observables/tweakables Example detectors BSM physics in neutrinos (NSI, magnetic moment, ) Nuclear recoils (CEvNS) Single phase LAr Inelastic NC/CC interactions Other large CEvNS (crystals, ) Sterile neutrino oscillations L-dependence LAr TPC Nuclear physics (Rn, n skin, gA, ) Direction dependence HP Gas TPC Supernova-relevant cross-sections Accelerator-produced DM
Generic needs/wishes Strawman example Space: footprint, height, pits, floor loading ~10 ton x 2 4.5 m x 10 m x 3 m Location: proximity, osc maximum (sterile), direction wrt beam (DM), movability Basement Access Backgrounds: n s, gammas etc -> shielding cosmics -> overburden >=15 m solid fill <~15 ton crane Access T0 Amenities: power, HVAC, cranes, T0, coffee Coffee For most physics, want to be as close as possible to the target, with as little background as possible
