Response of photomultiplier tubes to xenon scintillation light
B. L\'opez Paredes, H. M. Ara\'ujo, F. Froborg, N. Marangou, I., Olcina, T. J. Sumner, R. Taylor, A. Tom\'as, A. Vacheret

TL;DR
This study calibrates 35 xenon-sensitive photomultiplier tubes for dark matter detection, revealing temperature-dependent quantum efficiency and double photoelectron emission probabilities crucial for interpreting liquid xenon scintillation data.
Contribution
First comprehensive calibration of Hamamatsu R11410-22 PMTs at low temperature, quantifying DPE and QE variations relevant for dark matter experiments.
Findings
QE improves by ~18% when cooled to -100°C
DPE probability increases by ~12% at low temperature
Triple photoelectron emission observed at ~0.6%
Abstract
We present the precision calibration of 35 Hamamatsu R11410-22 photomultiplier tubes (PMTs) with xenon scintillation light centred near 175 nm. This particular PMT variant was developed specifically for the LUX-ZEPLIN (LZ) dark matter experiment. A room-temperature xenon scintillation cell coupled to a vacuum cryostat was used to study the full-face PMT response at both room and low temperature \textrm{(\sim^\circC)}, in particular to determine the quantum efficiency (QE) and double photoelectron emission (DPE) probability in LZ operating conditions. For our sample with an average QE of \textrm{(32.4\pm at room temperature, we find a relative improvement of \textrm{(17.9\pm upon cooling (where uncertainty values refer to the sample standard deviation). The mean DPE probability in response to single vacuum ultraviolet (VUV) photons is…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
