Development of a New Class of Scintillating Fibres with Very Short Decay Time and High Light Yield

被引:18
作者
Borshchev, O. [1 ]
Cavalcante, A. B. R. [2 ]
Gavardi, L. [3 ]
Gruber, L. [4 ]
Joram, C. [4 ]
Ponomarenko, S. [1 ]
Shinji, O. [5 ]
Surin, N. [1 ]
机构
[1] Russian Acad Sci, Enikolopov Inst Synthet Polymer Mat, Moscow 117393, Russia
[2] CBPF, Rio De Janeiro, Brazil
[3] Tech Univ Dortmund, D-44221 Dortmund, Germany
[4] CERN, PH Dept, CH-1211 Geneva 23, Switzerland
[5] Kuraray CO LTD, Methacrylate Dev Dept, Tokyo 1008115, Japan
基金
欧盟地平线“2020”;
关键词
Scintillators; scintillation and light emission processes (solid; gas and liquid scintillators); Calorimeters; Particle tracking detectors; Timing detectors;
D O I
10.1088/1748-0221/12/05/P05013
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
We present first studies of a new class of scintillating fibres which are characterised by very short decay times and high light yield. The fibres are based on a novel type of luminophores admixed to a polystyrene core matrix. These so-called Nanostructured Organosilicon Luminophores (NOL) have high photoluminescense quantum yield and decay times just above 1 ns. A blue and a green emitting prototype fibre with 250 mu m diameter were produced and characterised in terms of attenuation length, ionisation light yield, decay time and tolerance to x-ray irradiation. The well-established Kuraray SCSF-78 and SCSF-3HF fibres were taken as references. Even though the two prototype fibres mark just an intermediate step in an ongoing development, their performance is already on a competitive level. In particular, their decay time constants are about a factor of two shorter than the fastest known fibres, which makes them promising candidates for time critical applications.
引用
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页数:15
相关论文
共 21 条
[1]   The KLOE electromagnetic calorimeter [J].
Adinolfi, M ;
Ambrosino, F ;
Antonelli, A ;
Antonelli, M ;
Anulli, F ;
Barbiellini, G ;
Bencivenni, G ;
Bertolucci, S ;
Bini, C ;
Bloise, C ;
Bocci, V ;
Bossi, F ;
Branchini, P ;
Cabibbo, G ;
Caloi, R ;
Campana, P ;
Casarsa, M ;
Cataldi, G ;
Ceradini, F ;
Cervelli, F ;
Ciambrone, P ;
De Lucia, E ;
De Sinione, P ;
De Zorzi, G ;
Dell'Agnello, S ;
Denig, A ;
Di Domenico, A ;
Di Donato, C ;
Di Falco, S ;
Doria, A ;
Erriquez, O ;
Farilla, A ;
Ferrari, A ;
Ferrer, ML ;
Finocchiaro, G ;
Forti, C ;
Franceschi, A ;
Franzini, P ;
Gao, ML ;
Gatti, C ;
Gauzzi, P ;
Giannasi, A ;
Giovannella, S ;
Graziani, E ;
Han, HG ;
Han, SW ;
Huang, X ;
Incagli, M ;
Ingrosso, L ;
Keeble, L .
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2002, 482 (1-2) :364-386
[2]   Galaxy dynamics predictions in the nonsymmetric gravitational theory [J].
Moffat, JW ;
Sokolov, IY .
PHYSICS LETTERS B, 1996, 378 (1-4) :59-67
[3]   Development of VUV wavelength shifter for the use with a visible light photodetector in noble gas filled detectors [J].
Akimov, D. Yu ;
Akindinov, A. V. ;
Alexandrov, I. S. ;
Belov, V. A. ;
Borshchev, O. V. ;
Burenkov, A. A. ;
Danilov, M. V. ;
Kovalenko, A. G. ;
Luponosov, Y. N. ;
Ponomarenko, S. A. ;
Stekhanov, V. N. ;
Surin, N. M. ;
Zav'yalov, S. A. ;
Yablokov, M. Yu .
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2012, 695 :403-406
[4]  
Alfieri C., EXPT SET MEASURE LIG
[5]  
Alfieri C., SET MEASURE OPTICAL
[6]  
[Anonymous], ORG PHOTON PHOTOVOLT
[7]  
[Anonymous], ARXIV13016113
[8]  
[Anonymous], CERNLHCC2014001 LHCB
[9]   The Mu3e Experiment [J].
Berger, Niklaus .
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 2014, 248 :35-40
[10]  
Gavardi L., SETUP PERFORM X RAY