The Wavelength-Shifting Optical Module
Authors:
- Benjamin Bastian-QuernerBBBenjamin Bastian-Querner
- Lucas S. BinnLBLucas S. Binn
- Sebastian BöserSBSebastian Böser
- Jannes Brostean-KaiserJBJannes Brostean-Kaiser
- Dustin HebeckerDHDustin Hebecker
- Klaus HelbingKHKlaus Helbing
- Timo KargTKTimo Karg
- Lutz KöpkeLKLutz Köpke
- Marek KowalskiMKMarek Kowalski
- Peter PeifferPPPeter Peiffer
- Anna PollmannAPAnna Pollmann
- John Rack-HelleisJRJohn Rack-Helleis
Open Access
Abstract
The Wavelength-shifting Optical Module (WOM) is a novel photosensor concept for the instrumentation of large detector volumes with single-photon sensitivity. The key objective is to improve the signal-to-noise ratio, which is achieved by decoupling the photosensitive area of a sensor from the cathode area of its photomultiplier tube (PMT). The WOM consists of a transparent tube with two PMTs attached to its ends. The tube is coated with wavelength-shifting paint that absorbs ultraviolet photons with nearly 100% efficiency. Depending on the environment, e.g., air (ice), up to 73% (41%) of the subsequently emitted optical photons can be captured by total internal reflection and propagate towards the PMTs, where they are recorded. The optical properties of the paint, the geometry of the tube, and the coupling of the tube to the PMTs have been optimized for maximal sensitivity based on theoretical derivations and experimental evaluations. Prototypes were built to demonstrate the technique and to develop a reproducible construction process. Important measurable characteristics of the WOM are the wavelength-dependent effective area, the transit time spread of detected photons, and the signal-to-noise ratio. The WOM outperforms bare PMTs, especially with respect to the low signal-to-noise ratio with an increase of a factor up to 8.9 in air (5.2 in ice). Since the gain in sensitivity is mostly in the UV regime, the WOM is an ideal sensor for Cherenkov and scintillation detectors.Keywords
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This publication has 18 references indexed in Scilit:
- Neutrino physics with JUNOJournal of Physics G: Nuclear and Particle Physics, 2016
- Dip Coating2013
- The Large Underground Xenon (LUX) experimentNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2013
- The XENON100 dark matter experimentAstroparticle Physics, 2012
- Ellipsometric measurements of the refractive indices of linear alkylbenzene and EJ-301 scintillators from 210 to 1000 nmPhysica Scripta, 2011
- First Dark Matter Results from the XENON100 ExperimentPhysical Review Letters, 2010
- The Borexino detector at the Laboratori Nazionali del Gran SassoNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2009
- Optical Study on Poly(methyl methacrylate)/Poly(vinyl acetate) BlendsInternational Journal of Photoenergy, 2009
- The Sudbury Neutrino ObservatoryNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2000
- On the thickness of the liquid film adhering to the walls of a vessel after emptyingProgress in Surface Science, 1993