Construction and response of a highly granular scintillator-based electromagnetic calorimeter

被引:8
|
作者
Repond, J. [1 ]
Xia, L. [1 ]
Eigen, G. [2 ]
Price, T. [3 ]
Watson, N. K. [3 ]
Winter, A. [3 ]
Thomson, M. A. [4 ]
Carloganu, C. [24 ]
Blazey, G. C. [5 ]
Dyshkant, A. [5 ]
Francis, K. [5 ]
Zutshi, V. [5 ]
Gadow, K. [6 ]
Gottlicher, P. [6 ]
Hartbrich, O. [6 ,25 ]
Kotera, K. [6 ,19 ,26 ,27 ]
Krivan, F. [6 ]
Krueger, K. [6 ]
Lu, S. [6 ]
Lutz, B. [6 ]
Reinecke, M. [6 ]
Sefkow, F. [6 ]
Sudo, Y. [6 ,22 ]
Tran, H. L. [6 ]
Kaplan, A. [7 ]
Schultz-Coulon, H. -Ch. [7 ]
Bilki, B. [8 ,28 ]
Northacker, D. [8 ]
Onel, Y. [8 ]
Wilson, G. W. [9 ]
Kawagoe, K. [10 ,11 ]
Sekiya, I. [10 ,11 ]
Suehara, T. [10 ,11 ]
Yamashiro, H. [10 ,11 ]
Yoshioka, T. [10 ,11 ]
Calvo Alamillo, E. [12 ]
Fouz, M. C. [12 ]
Marin, J. [12 ]
Navarrete, J. [12 ]
Puerta Pelayo, J. [12 ]
Verdugo, A. [12 ]
Chadeeva, M. [13 ,29 ]
Danilov, M. [13 ,29 ,30 ]
Gabriel, M. [14 ]
Goecke, P. [14 ]
Graf, C. [14 ]
Israeli, Y. [14 ]
van der Kolk, N. [14 ]
Simon, F. [14 ]
Szalay, M. [14 ]
机构
[1] Argonne Natl Lab, 9700 S Cass Ave, Argonne, IL 60439 USA
[2] Univ Bergen, Inst Phys, Allegaten 55, N-5007 Bergen, Norway
[3] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
[4] Univ Cambridge, Cavendish Lab, J J Thomson Ave, Cambridge CB3 0HE, England
[5] Northern Illinois Univ, Dept Phys, NICADD, De Kalb, IL 60115 USA
[6] DESY, Notkestr 85, D-22603 Hamburg, Germany
[7] Heidelberg Univ, Fak Phys & Astron, Albert Uberle Str 3-5 2-OG Ost D-69120, Heidelberg, Germany
[8] Univ Iowa, Dept Phys & Astron, 203 Van Allen Hall, Iowa City, IA 52242 USA
[9] Univ Kansas, Dept Phys & Astron, Malott Hall,1251 Wescoe Hall Dr, Lawrence, KS 66045 USA
[10] Kyushu Univ, Dept Phys, Nishi Ku, 744 Motooka, Fukuoka 8190395, Japan
[11] Kyushu Univ, Res Ctr Adv Particle Phys, Nishi Ku, 744 Motooka, Fukuoka 8190395, Japan
[12] Ctr Invest Energet Medioambientales & Tecnol, CIEMAT, Madrid, Spain
[13] Russian Acad Sci, PN Lebedev Phys Inst, GSP-1,B-333, Moscow 117924, Russia
[14] Max Planck Inst Phys & Astrophys, Fohringer Ring 6, D-80805 Munich, Germany
[15] CNRS IN2P3, Lab Accelerateur Lineaire, Ctr Sci Orsay Beitiment 200,BP 34, F-91898 Orsay, France
[16] Univ Paris Sud 11, Ctr Sci Orsay, Batiment 200,BP 34, F-91898 Orsay, France
[17] CNRS IN2P3, Ecole Polytech, LLR, F-91128 Palaiseau, France
[18] Czech Acad Sci, Inst Phys, Na Slovance 2, CZ-182218 Prague 8, Czech Republic
[19] Shinshu Univ, Dept Phys, 3-1-1 Asahi, Nagano 3908621, Japan
[20] Univ Tokyo, ICEPP, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan
[21] Kyungpook Natl Univ, Dept Phys, Taegu 702701, South Korea
[22] Univ Tsukuba, Fac Pure & Appl Sci, Div Phys, Tennoudai 1-1-1, Tsukuba, Ibaraki 3058571, Japan
[23] Berg Univ Wuppertal, Fak Phys 4, Gaussstr 20, D-42097 Wuppertal, Germany
[24] Univ Blaise Pascal, Clermont Univ, Lab Phys Corpusculaire, CNRS IN2P3, BP10448, F-63000 Clermont Ferrand, France
[25] Univ Hawaii Manoa, High Energy Phys Grp, 2505 Correa Rd, Honolulu, HI 96822 USA
[26] Shinshu Univ, Matsumoto, Nagano, Japan
[27] Osaka Univ, Suita, Osaka, Japan
[28] Beykent Univ, Istanbul, Turkey
[29] MEPhI, Moscow, Russia
[30] Moscow Inst Phys & Technol, Dolgoprudnyi, Russia
[31] Okayama Univ, Okayama, Japan
[32] KEK, Tsukuba, Ibaraki, Japan
[33] Islamia Coll Univ, Peshawar, Pakistan
基金
新加坡国家研究基金会; 英国科学技术设施理事会; 美国国家科学基金会; 欧盟地平线“2020”; 加拿大自然科学与工程研究理事会;
关键词
Particle flow; Electromagnetic calorimeter; Scintillator; MPPC; SiPM; Granular; PROTOTYPE;
D O I
10.1016/j.nima.2018.01.016
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
A highly granular electromagnetic calorimeter with scintillator strip readout is being developed for future linear collider experiments. A prototype of 21.5 X-0 depth and 180 x 180 mm(2) transverse dimensions was constructed, consisting of 2160 individually read out 10 x 45 x 3 mm(3) scintillator strips. This prototype was tested using electrons of 2-32 GeV at the Fermilab Test Beam Facility in 2009. Deviations from linear energy response were less than 1.1%, and the intrinsic energy resolution was determined to be (12.5 +/- 0.1(stat.)+/- 0.4(syst.))%/root E[GeV]circle plus (1.2 +/- 0.1(stat.)(-0.7)(+0.6)(syst.))%, where the uncertainties correspond to statistical and systematic sources, respectively. (C) 2018 Elsevier B.V. All rights reserved.
引用
收藏
页码:150 / 168
页数:19
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