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VUV-Sensitive Silicon Photomultipliers for Xenon Scintillation Light Detection in nEXO
Authors
A Alamre
JB Albert
+151 more
G Anton
IJ Arnquist
I Badhrees
PS Barbeau
D Beck
V Belov
T Bhatta
E Bourque
JP Brodsky
E Brown
T Brunner
A Burenkov
GF Cao
L Cao
WR Cen
C Chambers
SA Charlebois
M Chiu
B Cleveland
M Coon
M Cote
A Craycraft
W Cree
J Dalmasson
T Daniels
L Darroch
SJ Daugherty
J Daughhetee
S Delaquis
R DeVoe
J Dilling
YY Ding
MJ Dolinski
Leonard Douglas
A Dragone
J Echevers
L Fabris
D Fairbank
W Fairbank
J Farine
S Feyzbakhsh
R Fontaine
D Fudenberg
G Gallina
G Giacomini
R Gornea
G Grata
EV Hansen
D Harris
M Hasan
M Heffner
J Hoessl
EW Hoppe
A House
P Hufschmidt
M Hughes
Y Ito
A Iverson
A Jamil
C Jessiman
MJ Jewell
XS Jiang
A Karelin
LJ Kaufman
T Koffas
S Kravitz
R Krucken
A Kuchenkov
KS Kumar
Y Lan
A Larson
G Li
S Li
Z Li
C Licciardi
YH Lin
L Lupin-Jimenez
P Lv
R MacLellan
AD Mesrobian-Kabakian
T Michel
B Mong
DC Moore
K Murray
RJ Newby
Z Ning
O Njoya
F Nolet
O Nusair
K Odgers
A Odian
M Oriunno
JL Orrell
GS Ortega
I Ostrovskiy
CT Overman
S Parent
A Piepke
A Pocar
JE Pratte
D Qiu
V Radeka
E Raguzin
T Rao
S Rescia
F Retiere
A Robinson
T Rossignol
PC Rowson
N Roy
R Saldanha
S Sangiorgio
S Schmidt
J Schneider
A Schubert
D Sinclair
K Skarpaas
AK Soma
G St-Hilaire
V Stekhanov
T Stiegler
XL Sun
M Tarka
J Todd
T Tolba
TI Totev
R Tsang
T Tsang
F Vachon
B Veenstra
V Veeraraghavan
G Visser
JL Vuilleumier
M Wagenpfeil
Q Wang
J Watkins
M Weber
W Wei
LJ Wen
U Wichoski
G Wrede
SX Wu
WH Wu
Q Xia
L Yang
YR Yen
O Zeldovich
X Zhang
J Zhao
Y Zhou
T Ziegler
Publication date
1 November 2018
Publisher
IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC
Abstract
Future ton-scale liquefied noble gas detectors depend on efficient light detection in the vacuum ultraviolet (VUV) range. In the past years, silicon photomultipliers (SiPMs) have emerged as a valid alternative to standard photomultiplier tubes or large-area avalanche photodiodes. The next-generation double-beta decay experiment, nEXO, with a 5-ton liquid xenon time projection chamber will use SiPMs for detecting the 175-nm xenon scintillation light, in order to achieve an energy resolution of sigma/Q(beta beta) = 1%. This paper presents recent measurements of the VUV-HD generation SiPMs from Fondazione Bruno Kessler, Trento, Italy, in two complementary setups. It includes measurements of the photon-detection efficiency (PDE) with gaseous xenon scintillation light in a vacuum setup and dark measurements in a dry nitrogen gas setup. We report improved PDE at 175 nm compared to previous generation devices that would meet the criteria of nEXO. Furthermore, we present the projected nEXO detector light collection and energy resolution that could be achieved by using these SiPMs © 2018 IEEE
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Last time updated on 06/02/2020