Alignment of the CMS silicon tracker during commissioning with cosmic rays

被引:81
作者
Chatrchyan, S. [1 ]
Khachatryan, V. [1 ]
Sirunyan, A. M. [1 ]
Adam, W. [2 ]
Arnold, B. [2 ]
Bergauer, H. [2 ]
Bergauer, T. [2 ]
Dragicevic, M. [2 ]
Eichberger, M. [2 ]
Eroe, J. [2 ]
Friedl, M. [2 ]
Fruehwirth, R. [2 ]
Ghete, V. M. [2 ]
Hammer, J. [2 ]
Haensel, S. [2 ]
Hoch, M. [2 ]
Hoermann, N. [2 ]
Hrubec, J. [2 ]
Jeitler, M. [2 ]
Kasieczka, G. [2 ]
Kastner, K. [2 ]
Krammer, M. [2 ]
Liko, D. [2 ]
de Abril, I. Magrans [2 ]
Mikulec, I. [2 ]
Mittermayr, F. [2 ]
Neuherz, B. [2 ]
Oberegger, M. [2 ]
Padrta, M. [2 ]
Pernicka, M. [2 ]
Rohringer, H. [2 ]
Schmid, S. [2 ]
Schoefbeck, R. [2 ]
Schreiner, T. [2 ]
Stark, R. [2 ]
Steininger, H. [2 ]
Strauss, J. [2 ]
Taurok, A. [2 ]
Teischinger, F. [2 ]
Themel, T. [2 ]
Uhl, D. [2 ]
Wagner, P. [2 ]
Waltenberger, W. [2 ]
Walzel, G. [2 ]
Widl, E. [2 ]
Wulz, C. -E. [2 ]
Chekhovsky, V. [3 ]
Dvornikov, O. [3 ]
Emeliantchik, I. [3 ]
Litomin, A. [3 ]
机构
[1] Yerevan Phys Inst, Yerevan 375036, Armenia
[2] Inst Hochenergiephys OeAW, Vienna, Austria
[3] Natl Ctr Particle & High Energy Phys, Minsk, BELARUS
[4] Res Inst Nucl Problems, Minsk, BELARUS
[5] Res Inst Appl Phys Problems, Minsk, BELARUS
[6] Univ Antwerp, B-2020 Antwerp, Belgium
[7] Vrije Univ Brussel, Brussels, Belgium
[8] Univ Libre Bruxelles, Brussels, Belgium
[9] Univ Ghent, B-9000 Ghent, Belgium
[10] Catholic Univ Louvain, B-3000 Louvain, Belgium
[11] Univ Mons, B-7000 Mons, Belgium
[12] Ctr Brasileiro Pesquisas Fis, Rio De Janeiro, Brazil
[13] Univ Estado Rio de Janeiro, BR-20550011 Rio De Janeiro, Brazil
[14] Univ Estadual Paulista, Inst Fis Teor, BR-01405 Sao Paulo, Brazil
[15] Bulgarian Acad Sci, Inst Nucl Res & Nucl Energy, Sofia, Bulgaria
[16] Univ Sofia, BU-1126 Sofia, Bulgaria
[17] Inst High Energy Phys, Beijing 100039, Peoples R China
[18] Univ Los Andes, Bogota, Colombia
[19] Tech Univ Split, Split, Croatia
[20] Univ Split, Split, Croatia
[21] Rudjer Boskovic Inst, Zagreb, Croatia
[22] Univ Cyprus, Nicosia, Cyprus
[23] NICPB, Tallinn, Estonia
[24] Helsinki Inst Phys, Helsinki, Finland
[25] Lappeenranta Univ Technol, Lappeenranta, Finland
[26] CNRS, IN2P3, Lab Annecy Le Vieux Phys Particules, Annecy Le Vieux, France
[27] CEA Saclay, DSM, IRFU, Gif Sur Yvette, France
[28] Ecole Polytech, CNRS, Lab Leprince Ringuet, IN2P3, F-91128 Palaiseau, France
[29] Univ Haute Alsace Mulhouse, Inst Pluridisciplinaire Hubert Curien, Univ Strasbourg, Strasbourg, France
[30] Univ Lyon 1, CNRS, IN2P3, Inst Phys Nucl Lyon, F-69622 Villeurbanne, France
[31] Georgian Acad Sci, E Andronikashvili Inst Phys, GE-380060 Tbilisi, Georgia
[32] Tbilisi State Univ, Inst High Energy Phys & Informatizat, GE-380086 Tbilisi, Georgia
[33] Rhein Westfal TH Aachen, Inst Phys 1, Aachen, Germany
[34] Rhein Westfal TH Aachen, Inst Phys 3, Aachen, Germany
[35] Rhein Westfal TH Aachen, Inst Phys B 3, Aachen, Germany
[36] Deutsch Elekt Synchrotron, Hamburg, Germany
[37] Univ Hamburg, Hamburg, Germany
[38] Univ Karlsruhe, Inst Expt Kernphys, D-7500 Karlsruhe, Germany
[39] Inst Nucl Phys Demokritos, Aghia Paraskevi, Greece
[40] Univ Athens, Athens, Greece
[41] Univ Ioannina, GR-45110 Ioannina, Greece
[42] KFKI Res Inst Particle & Nucl Phys, Budapest, Hungary
[43] Inst Nucl Res ATOMKI, Debrecen, Hungary
[44] Univ Debrecen, H-4012 Debrecen, Hungary
[45] Panjab Univ, Chandigarh 160014, India
[46] Univ Delhi, Delhi 110007, India
[47] Bhabha Atom Res Ctr, Mumbai 400085, Maharashtra, India
[48] Tata Inst Fundamental Res, EHEP, Mumbai 400005, Maharashtra, India
[49] Tata Inst Fundamental Res, HECR, Mumbai 400005, Maharashtra, India
[50] Inst Studies Theoret Phys & Math IPM, Tehran, Iran
基金
芬兰科学院; 巴西圣保罗研究基金会;
关键词
Large detector systems for particle and astroparticle physics; Particle tracking detectors (Solid-state detectors);
D O I
10.1088/1748-0221/5/03/T03009
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
The CMS silicon tracker, consisting of 1440 silicon pixel and 15 148 silicon strip detector modules, has been aligned using more than three million cosmic ray charged particles, with additional information from optical surveys. The positions of the modules were determined with respect to cosmic ray trajectories to an average precision of 3-4 microns RMS in the barrel and 3-14 microns RMS in the endcap in the most sensitive coordinate. The results have been validated by several studies, including laser beam cross-checks, track fit self-consistency, track residuals in overlapping module regions, and track parameter resolution, and are compared with predictions obtained from simulation. Correlated systematic effects have been investigated. The track parameter resolutions obtained with this alignment are close to the design performance.
引用
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页数:41
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