D. Mayani
University of Zurich
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Publication
Featured researches published by D. Mayani.
European Physical Journal C | 2015
E. Aprile; F. Agostini; M. Alfonsi; L. Arazi; K. Arisaka; F. Arneodo; M. Auger; C. Balan; P. Barrow; L. Baudis; B. Bauermeister; A. Behrens; P. Beltrame; Abbe Brown; E. Brown; S. Bruenner; G. Bruno; R. Budnik; Lukas Bütikofer; João Cardoso; Daniel Coderre; A. P. Colijn; H. Contreras; J. P. Cussonneau; M.P. Decowski; A. Di Giovanni; E. Duchovni; S. Fattori; A. D. Ferella; A. Fieguth
The low-background, VUV-sensitive 3-inch diameter photomultiplier tube R11410 has been developed by Hamamatsu for dark matter direct detection experiments using liquid xenon as the target material. We present the results from the joint effort between the XENON collaboration and the Hamamatsu company to produce a highly radio-pure photosensor (version R11410-21) for the XENON1T dark matter experiment. After introducing the photosensor and its components, we show the methods and results of the radioactive contamination measurements of the individual materials employed in the photomultiplier production. We then discuss the adopted strategies to reduce the radioactivity of the various PMT versions. Finally, we detail the results from screening 286 tubes with ultra-low background germanium detectors, as well as their implications for the expected electronic and nuclear recoil background of the XENON1T experiment.
Journal of Instrumentation | 2017
P. Barrow; L. Baudis; D. Cichon; Meike Danisch; D. Franco; F. Kaether; A. Kish; Manfred Lindner; Teresa Marrodán Undagoitia; D. Mayani; L. Rauch; Y. Wei; J. Wulf
The Hamamatsu R11410-21 photomultiplier tube is the photodetector of choice for the XENON1T dual-phase time projection chamber. The device has been optimized for a very low intrinsic radioactivity, a high quantum efficiency and a high sensitivity to single photon detection. A total of 248 tubes are currently operated in XENON1T, selected out of 321 tested units. In this article the procedures implemented to evaluate the large number of tubes prior to their installation in XENON1T are described. The parameter distributions for all tested tubes are shown, with an emphasis on those selected for XENON1T, of which the impact on the detector performance is discussed. All photomultipliers have been tested in a nitrogen atmosphere at cryogenic temperatures, with a subset of the tubes being tested in gaseous and liquid xenon, simulating their operating conditions in the dark matter detector. The performance and evaluation of the tubes in the different environments is reported and the criteria for rejection of PMTs are outlined and quantified.
Journal of Instrumentation | 2013
L. Baudis; A. Behrens; A. D. Ferella; A. Kish; T. Marrodán Undagoitia; D. Mayani; M. Schumann