Uploaded January 2024 | Updated September 2026, 2 weeks ago
Speaker: Diego Aristizabal (Universidad Tecnica Federico Santa Maria, Chile)
Abstract: CEvNS experimental facilities provide a rather rich environment for precise measurements of SM parameters and searches of new physics. In this talk, I will discuss a few aspects of this program involving solar neutrinos and third generation DM detectors as well as directional detectors in the FNAL neutrino beamlines. I will briefly comment on ALPs searches sourced by nuclear reactors and potentially detectable with the same technology used in the CEvNS program.
Speaker: Diego Aristizabal (Universidad Tecnica Federico Santa Maria, Chile)
Abstract: CEvNS experimental facilities provide a rather rich environment for precise measurements of SM parameters and searches of new physics. In this talk, I will discuss a few aspects of this program involving solar neutrinos and third generation DM detectors as well as directional detectors in the FNAL neutrino beamlines. I will briefly comment on ALPs searches sourced by nuclear reactors and potentially detectable with the same technology used in the CEvNS program.
