Searching for beyond-Standard-Model solar neutrino interactions using directional detectors
Anirudh Chandra Shekar, Chiara Lisotti, Nityasa Mishra, Ciaran A. J. O'Hare, Louis E. Strigari

TL;DR
This paper forecasts the potential of large-scale directional gaseous detectors to explore non-standard neutrino interactions and new light mediators by analyzing solar neutrino recoil data with improved sensitivity.
Contribution
It introduces a framework for using upcoming 30 m³ MPGDs to detect beyond-Standard-Model neutrino interactions through recoil energy and angle measurements.
Findings
Sensitivity approaches Borexino's with background reduction
Directionality enables event-by-event neutrino energy reconstruction
Motivates development of small-scale directional gas detectors
Abstract
Micro-pattern gaseous detectors (MPGDs) are a class of technologies that enable the full three-dimensional spatial reconstruction of ionisation tracks from nuclear and electron recoils in gas. Anticipating near-future 30 m-scale time projection chambers with MPGD-based readout, we forecast the sensitivity of such directionally-sensitive low-energy recoil detectors to neutrino interactions beyond the Standard Model. We work in the framework of neutrino non-standard interactions (NSIs), and calculate the combined recoil energy-angle distributions of the electron recoil signal generated by solar neutrinos in atmospheric-pressure He:CF gas. We estimate the expected exclusion limits that such an experiment could place on various NSI parameters, as well as the mass and coupling of a new light mediator that interacts with electrons and neutrinos. We find that with an achievable…
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