Constraining Ultra-Light Vector Bosons via Solar Neutrino Oscillations: The Gauged L mu - L tau Model and Prospects for JUNO and XLZD
hep-ph, astro-ph.SR, hep-ex, hep-th
Submitted: 2026-09-27
Updated: 2026-09-27
Terminology
Sources
- Galactic Searches for Dark Matter
- Gravitational probes of dark matter physics
- Dark matter and the early Universe: a review
- Light Dark Matter Annihilation and Scattering in LHC Detectors
- Experimental Searches for the Axion and Axion-like Particles
- Wave Dark Matter
- Status of global fits to neutrino oscillations
- Status and Perspectives of Neutrino Physics
- Solar neutrino physics
- Status of the solution to the solar neutrino problem based on non-standard neutrino interactions
- Status of a hybrid three-neutrino interpretation of neutrino data
- Atmospheric Neutrino Oscillations and New Physics
- Non standard neutrino interactions
- Neutrino oscillations and Non-Standard Interactions
- A Direct Detection View of the Neutrino NSI Landscape
- Gauged L_mu - L_tau and different Muon Neutrino and Anti-Neutrino Oscillations: MINOS and beyond
- To (b)e or not to (b)e: No electrons at LHCb
- The anomalous magnetic moment of the muon in the Standard Model: an update
- Solar Neutrino Spectroscopy
- The Future of Solar Neutrinos
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