Sensitivity to Non-Standard Interactions (NSI) with KM3NeT-ORCA

• Published in: Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)
• Main Authors: Khan Chowdhury, N.R., Thakore, T., Coelho, J.A. B., Zornoza, J.D., Navas, S.
• Other Authors: Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), KM3NeT
• Format: Conference Object
• Language: English
• Published: HAL CCSD 2019
• Subjects: neutrino: interaction; neutrino: atmosphere; neutrino: oscillation; neutrino: mass: hierarchy; neutrino: detector; sensitivity; Cherenkov counter; KM3NeT; numerical calculations; new physics; [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]; [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]; Orca
• Online Access: https://hal.science/hal-02966281; https://doi.org/10.22323/1.358.0931

International audience ORCA (Oscillations Research with Cosmics in the Abyss) is the low-energy detector of KM3NeT, the next generation underwater Cherenkov neutrino detector in the Mediterranean Sea. Although its primary goal is to determine the Neutrino Mass Ordering (NMO) with atmospheric neutrinos, its access to a wide range of energies and baselines makes it optimal to discover exotic physics beyond the Standard Model (SM) such as Non-Standard Interactions (NSI).Non-Standard Interactions with neutrinos will introduce modifications in the SM potential, which will alter the event spectra at the ORCA detector. Using these NSI induced distortions inthe flavour content over three flavour standard oscillations, it is possible to constrain NSI modelparameters. This report outlines the sensitivity that ORCA can achieve in puttingupper bounds on some of these non-standard neutrino interaction parameters.