WLS R\&D for the Detection of Noble Gas Scintillation at LBL: seeing the light from neutrinos, to dark matter, to double beta decay
arXiv:1308.2699 · doi:10.1088/1748-0221/8/09/C09007
Abstract
Radiation detectors with noble gasses as the active medium are becoming increasingly common in experimental programs searching for physics beyond the standard model. Nearly all of these experiments rely to some degree on collecting scintillation light from noble gasses. The VUV wavelengths associated with noble gas scintillation mean that most of these experiments use a fluorescent material to shift the direct scintillation light into the visible or near UV band. We present an overview of the R&D program at LBL related to noble gas detectors for neutrino physics, double beta decay, and dark matter. This program ranges from precise measurements of the fluorescence behavior of wavelength shifting films, to the prototyping of large are VUV sensitive light guides for multi-kiloton detectors.
Six Pages, Four Figures. Proceeding for "Light Detection in Noble Elements." 29-13 May, 2013. FNAL. Batavia, IL
References in corpus (5)
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- The Large Underground Xenon (LUX) Experiment
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Cited by in corpus (4)
- Wavelength shifters for applications in liquid argon detectors
- Expected performance of an ideal liquid argon neutrino detector with enhanced sensitivity to scintillation light
- Measurement of the Angular Distribution of Wavelength-Shifted Light Emitted by TPB
- Xenon Bubble Chambers for Direct Dark Matter Detection