Design Constraints for a WIMP Dark Matter and pp Solar Neutrino Liquid Neon Scintillation Detector
M.G. Boulay, A. Hime, J. Lidgard

TL;DR
This paper evaluates a liquid neon scintillation detector's performance for dark matter and solar neutrino detection, demonstrating improved resolution and sensitivity through advanced simulation and calibration techniques.
Contribution
It introduces a maximum-likelihood event vertex fitter and assesses detector design parameters for optimal sensitivity to WIMPs and solar neutrinos.
Findings
Achieves ~13 keV energy threshold with 300 cm radius detector
Limits on WIMP-nucleon cross-section of ~10^{-46} cm^2 at 100 GeV
Provides calibration strategies for internal radioactivity and krypton-85
Abstract
Detailed Monte-Carlo simulations were used to evaluate the performance of a liquid neon scintillation detector for dark matter and low-energy solar neutrino interactions. A maximum-likelihood event vertex fitter including PMT time information was developed, which significantly improves position resolution over spatial-only algorithms, and substantially decreases the required detector size and achievable analysis energy threshold. The ultimate sensitivity to WIMP dark matter and the pp flux uncertainty are evaluated as a function of detector size. The dependence on the neon scintillation and PMT properties are evaluated. A 300 cm radius detector would allow a ~13 keV threshold, a pp flux uncertainty of ~1%, and limits on the spin-independent WIMP-nucleon cross-section of ~10^{-46} cm^2 for a 100 GeV WIMP, using commercially available PMTs. Detector response calibration and background…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Neutrino Physics Research · Atomic and Subatomic Physics Research
