Hunting Nonstandard Neutrino Interactions and Leptoquarks in Dark Matter Experiments
arXiv:2307.15736 · doi:10.1088/1475-7516/2024/11/068
Abstract
Next generation direct dark matter (DM) detection experiments will have unprecedented capabilities to explore coherent neutrino-nucleus scattering (CENS) complementary to dedicated neutrino experiments. We demonstrate that future DM experiments can effectively probe nonstandard neutrino interactions (NSI) mediated by scalar fields in the scattering of solar and atmospheric neutrinos. We set first limits on leptoquark models that result in sizable and sector neutrino NSI CENS contributions using LUX-ZEPLIN (LZ) data. As we show, near future DM experiments reaching ton-year exposure, such as argon-based ARGO and xenon-based DARWIN, can probe parameter space of leptoquarks beyond the reach of current and planned collider facilities. We also analyze for the first time prospects for testing NSI in lead-based detectors. We discuss the ability of leptoquarks in the parameter space of interest to also explain the neutrino masses and observations.
Discussion of scalar/vector NSI revised, improved oscillation analysis, accepted for publication in JCAP 33 pages, 12 figures, 1 table
References in corpus (35)
- Observation of Coherent Elastic Neutrino-Nucleus Scattering
- First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment
- First Dark Matter Search with Nuclear Recoils from the XENONnT Experiment
- A new Generation of Standard Solar Models
- The Diffuse Supernova Neutrino Background
- The Diffuse Supernova Neutrino Background is detectable in Super-Kamiokande
- Precision Measurement of the Weak Charge of the Proton
- COHERENT constraints on nonstandard neutrino interactions
- The Leptoquark Hunter's Guide: Pair Production
- Neutrinophilic Non-Standard Interactions
- Low-energy phenomenology of scalar leptoquarks at one-loop accuracy
- Diffuse Supernova Neutrino Background Search at Super-Kamiokande
- Parity and Time-Reversal Violation in Atomic Systems
- Leptoquarks: Neutrino masses and accelerator phenomenology
- Implications of the first detection of coherent elastic neutrino-nucleus scattering (CEvNS) with Liquid Argon
- Unified Framework for -Anomalies, Muon , and Neutrino Masses
- Constraints on light vector mediators through coherent elastic neutrino nucleus scattering data from COHERENT
- Light new physics in XENON1T
- Novel constraints on neutrino physics beyond the standard model from the CONUS experiment
- Improved measurement of solar neutrinos from the Carbon-Nitrogen-Oxygen cycle by Borexino and its implications for the Standard Solar Model
- A Statistical Analysis of the COHERENT Data and Applications to New Physics
- Leptoquarks and Matter Unification: Flavor Anomalies and the Muon
- Radiative neutrino masses, lepton flavor mixing and muon in a leptoquark model
- Leptoquark Option for -meson Anomalies and Leptonic Signatures
- A Direct Detection View of the Neutrino NSI Landscape
- Detecting Beyond the Standard Model Interactions of Solar Neutrinos in Low-Threshold Dark Matter Detectors
- Complementarity between dark matter direct searches and CENS experiments in models
- Dark matter detectors as a novel probe for light new physics
- Probing models with CENS: A new look at the combined COHERENT CsI and Ar data
- Atmospheric neutrinos in a next-generation xenon dark matter experiment
- Constraining Light Mediators via Detection of Coherent Elastic Solar Neutrino Nucleus Scattering
- CP-Violating and Charged Current Neutrino Non-standard Interactions in CENS
- Time variation of the atmospheric neutrino flux at dark matter detectors
- Probing Neutrino Mass Models through Resonances at Neutrino Telescopes
- Search for excited -leptons and leptoquarks in the final state with -leptons and jets in pp collisions at TeV with the ATLAS detector