TY - JOUR
T1 - Test of a SiPM-scintillator-based muon detector at the Gran Sasso National Laboratory
AU - Stark, I.
AU - Könye, V.
AU - Antolini, R.
AU - Arneodo, F.
AU - Boeltzig, A.
AU - Candela, A.
AU - Di Giovanni, A.
AU - Fülöp, Zs
AU - Junker, M.
N1 - Publisher Copyright:
© Published under licence by IOP Publishing Ltd.
PY - 2018/1/31
Y1 - 2018/1/31
N2 - The aim of the present work was to determine the characteristics of a tracking scintillation detector by measuring cosmic muons above- and underground at the Gran Sasso National Laboratory (LNGS). The detector has been designed for demonstrational purposes and had never been involved in scientific research before. It is a compact, layered detector using plastic scintillator bars and silicon photomultipliers (SiPM). In the present setup no energy information is used. In the underground laboratory we had to deal with a very low rate of muons (6 orders of magnitude less than on the surface). For this reason we optimized the trigger configuration. During the evaluation process we designed and optimized a maximum likelihood line fitting method which is able to deal with the high dark count rate and the non optimized detection efficiency of the detector. We also carried out simulations to calculate the actual flux and intensity from the measured ones. Finally, we compared our results with the literature and they were found to be in agreement.
AB - The aim of the present work was to determine the characteristics of a tracking scintillation detector by measuring cosmic muons above- and underground at the Gran Sasso National Laboratory (LNGS). The detector has been designed for demonstrational purposes and had never been involved in scientific research before. It is a compact, layered detector using plastic scintillator bars and silicon photomultipliers (SiPM). In the present setup no energy information is used. In the underground laboratory we had to deal with a very low rate of muons (6 orders of magnitude less than on the surface). For this reason we optimized the trigger configuration. During the evaluation process we designed and optimized a maximum likelihood line fitting method which is able to deal with the high dark count rate and the non optimized detection efficiency of the detector. We also carried out simulations to calculate the actual flux and intensity from the measured ones. Finally, we compared our results with the literature and they were found to be in agreement.
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U2 - 10.1088/1742-6596/940/1/012056
DO - 10.1088/1742-6596/940/1/012056
M3 - Conference article
AN - SCOPUS:85042432775
SN - 1742-6588
VL - 940
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
IS - 1
M1 - 012056
T2 - 7th Nuclear Physics in Astrophysics Conference, NPA 2015
Y2 - 18 May 2015 through 22 May 2015
ER -