Development of VUV wavelength shifter for the use with a visible light photodetector in noble gas filled detectors

被引:18
作者
Akimov, D. Yu [1 ]
Akindinov, A. V. [1 ]
Alexandrov, I. S. [1 ]
Belov, V. A. [1 ]
Borshchev, O. V. [2 ]
Burenkov, A. A. [1 ]
Danilov, M. V. [1 ]
Kovalenko, A. G. [1 ]
Luponosov, Y. N. [2 ]
Ponomarenko, S. A. [2 ]
Stekhanov, V. N. [1 ]
Surin, N. M. [2 ]
Zav'yalov, S. A. [3 ]
Yablokov, M. Yu [2 ]
机构
[1] Inst Theoret & Expt Phys, State Sci Ctr Russian Federat, Moscow 117218, Russia
[2] Russian Acad Sci, Enikolopov Inst Synthet Polymer Mat, Moscow 117393, Russia
[3] LY Karpov Phys Chem Res Inst, State Sci Ctr Russian Federat, Moscow 105064, Russia
关键词
VUV detection; Wavelength shifter; Noble gas emission; PHOTOMULTIPLIER TUBES;
D O I
10.1016/j.nima.2011.12.036
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
Development study of a wavelength shifter (WLS) to convert a noble gas emission light from the VUV region to the visible range is presented. The shifter is developed for the use with an array of blue-sensitive multipixel avalanche Geiger photodiodes (MRS APD) to detect Xe 175 nm emission. It was found that a polycrystalline p-terphenyl having an absorption peak at 180 nm with a molar extinction coefficient epsilon of 37500 +/- 5000 mol(-1).1 cm(-1) is well suited for this. To satisfy a requirement of compatibility with an extra pure noble gas detection medium the p-terphenyl layer was coated with an similar to 1 mu m thick poly-para-xylylene protection film. A new WLS with maximum of emission spectrum at 390 nm and at 420 nm is developed on the basis of a nanostructured organosilicon luminophore. (C) 2011 Elsevier B.V. All rights reserved.
引用
收藏
页码:403 / 406
页数:4
相关论文
共 16 条
[1]   The WArP Experiment [J].
Acciarri, R. ;
Antonello, M. ;
Baibussinov, B. ;
Benetti, P. ;
Calaprice, F. ;
Calligarich, E. ;
Cambiaghi, M. ;
Canci, N. ;
Cao, C. ;
Carbonara, F. ;
Cavanna, F. ;
Centro, S. ;
Ceolin, M. B. ;
Chavarria, A. ;
Cocco, A. ;
Di Pompeo, F. ;
Fiorillo, G. ;
Galbiati, C. ;
Grandi, L. ;
Loer, B. ;
Mangano, G. ;
Menegolli, A. ;
Meng, G. ;
Montanari, C. ;
Palamara, O. ;
Pandola, L. ;
Pietropaolo, F. ;
Raselli, G. L. ;
Roncadelli, M. ;
Rossella, M. ;
Rubbia, C. ;
Saldanha, R. ;
Segreto, E. ;
Szelc, A. M. ;
Ventura, S. ;
Vignoli, C. .
TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS (TAUP2009), 2010, 203
[2]   Detection of scintillation light in liquid xenon by multipixel avalanche Geiger photodiode and wavelength shifter [J].
Akimov, D. Yu. ;
Akindinov, A. V. ;
Alexandrov, I. S. ;
Burenkov, A. A. ;
Danilov, M. V. ;
Yablokov, M. Yu. ;
Kovalenko, A. G. ;
Stekhanov, V. N. ;
Surin, N. M. ;
Zav'yalov, S. A. .
JOURNAL OF INSTRUMENTATION, 2010, 5
[3]   First results from the XENON10 dark matter experiment at the Gran Sasso National Laboratory [J].
Angle, J. ;
Aprile, E. ;
Arneodo, F. ;
Baudis, L. ;
Bernstein, A. ;
Bolozdynya, A. ;
Brusov, P. ;
Coelho, L. C. C. ;
Dahl, C. E. ;
DeViveiros, L. ;
Ferella, A. D. ;
Fernandes, L. M. P. ;
Fiorucci, S. ;
Gaitskell, R. J. ;
Giboni, K. L. ;
Gomez, R. ;
Hasty, R. ;
Kastens, L. ;
Kwong, J. ;
Lopes, J. A. M. ;
Madden, N. ;
Manalaysay, A. ;
Manzur, A. ;
McKinsey, D. N. ;
Monzani, M. E. ;
Ni, K. ;
Oberlack, U. ;
Orboeck, J. ;
Plante, G. ;
Santorelli, R. ;
dos Santos, J. M. F. ;
Shagin, P. ;
Shutt, T. ;
Sorensen, P. ;
Schulte, S. ;
Winant, C. ;
Yamashita, M. .
PHYSICAL REVIEW LETTERS, 2008, 100 (02)
[4]   Dark Matter Results from 100 Live Days of XENON100 Data [J].
Aprile, E. ;
Arisaka, K. ;
Arneodo, F. ;
Askin, A. ;
Baudis, L. ;
Behrens, A. ;
Bokeloh, K. ;
Brown, E. ;
Bruch, T. ;
Bruno, G. ;
Cardoso, J. M. R. ;
Chen, W. -T. ;
Choi, B. ;
Cline, D. ;
Duchovni, E. ;
Fattori, S. ;
Ferella, A. D. ;
Gao, F. ;
Giboni, K. -L. ;
Gross, E. ;
Kish, A. ;
Lam, C. W. ;
Lamblin, J. ;
Lang, R. F. ;
Levy, C. ;
Lim, K. E. ;
Lin, Q. ;
Lindemann, S. ;
Lindner, M. ;
Lopes, J. A. M. ;
Lung, K. ;
Undagoitia, T. Marrodan ;
Mei, Y. ;
Fernandez, A. J. Melgarejo ;
Ni, K. ;
Oberlack, U. ;
Orrigo, S. E. A. ;
Pantic, E. ;
Persiani, R. ;
Plante, G. ;
Ribeiro, A. C. C. ;
Santorelli, R. ;
dos Santos, J. M. F. ;
Sartorelli, G. ;
Schumann, M. ;
Selvi, M. ;
Shagin, P. ;
Simgen, H. ;
Teymourian, A. ;
Thers, D. .
PHYSICAL REVIEW LETTERS, 2011, 107 (13)
[5]   Low-temperature study of 35 photomultiplier tubes for the ZEPLIN III experiment [J].
Araújo, HM ;
Bewick, A ;
Davidge, D ;
Dawson, J ;
Ferbel, T ;
Howard, AS ;
Jones, WG ;
Joshi, M ;
Lebedenko, V ;
Liubarsky, I ;
Quenby, JJ ;
Sumner, TJ ;
Neves, F .
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2004, 521 (2-3) :407-415
[6]  
Belogurov S., 1995, NUCL SCI S MED IM 19, V1, P519
[7]  
Benetti P, 2003, NUCL INSTRUM METH A, V505, P89, DOI [10.1016/S0168-9002(03)01027-1, 10.1016/S0168-9002(03)01022-2]
[8]  
Berlman I. B., 1971, HDB FLUORESCENCE SPE
[9]  
Birks J.B., 1964, THEORY PRACTICE SCI, P47
[10]  
Fortin J.B., 2004, CHEM VAPOR DEPOS