Peculiarities of intrinsic background in LaBr3: Ce and CeBr3 scintillating crystals

2009 ◽  
Vol 52 (6) ◽  
pp. 774-781 ◽  
Author(s):  
A. F. Iyudin ◽  
V. V. Bogomolov ◽  
S. I. Svertilov ◽  
I. V. Yashin ◽  
N. V. Klassen ◽  
...  
Keyword(s):  
2008 ◽  
Vol 1076 ◽  
Author(s):  
Jerome Moloney ◽  
Joerg Hader ◽  
Stephan W. Koch

ABSTRACTPerformance metrics of every class of semiconductor amplifier or laser system depend critically on semiconductor QW optical properties such as photoluminescence (PL), gain and recombination losses (radiative and nonradiative). Current practice in amplifier or laser design assumes phenomenological parameterized models for these critical optical properties and has to rely on experimental measurement to extract model fit parameters. In this tutorial, I will present an overview of a powerful and sophisticated first-principles quantum design approach that allows one to extract these critical optical properties without relying on prior experimental measurement. It will be shown that an end device L-I characteristic can be predicted with the only input being intrinsic background losses, extracted from cut-back experiments. We will show that textbook and literature models of semiconductor amplifiers and lasers are seriously flawed.


Universe ◽  
2021 ◽  
Vol 7 (11) ◽  
pp. 396
Author(s):  
Minbin Kim ◽  
Jakub Ripa ◽  
Il H. Park ◽  
Vitaly Bogomolov ◽  
Søren Brandt ◽  
...  

We developed an X-ray detector using 36 arrays, each consisting of a 64-pixellated yttrium oxyorthosilicate (YSO) scintillation crystal and a 64-channel multi-anode photomultiplier tube. The X-ray detector was designed to detect X-rays with energies lower than 10 keV, primarily with the aim of localizing gamma-ray bursts (GRBs). YSO crystals have no intrinsic background, which is advantageous for increasing low-energy sensitivity. The fabricated detector was integrated into UBAT, the payload of the Ultra-Fast Flash Observatory (UFFO)/Lomonosov for GRB observation. The UFFO was successfully operated in space in a low-Earth orbit. In this paper, we present the responses of the X-ray detector of the UBAT engineering model identical to the flight model, using 241Am and 55Fe radioactive sources and an Amptek X-ray tube. We found that the X-ray detector can measure energies lower than 5 keV. As such, we expect YSO crystals to be good candidates for the X-ray detector materials for future GRB missions.


2021 ◽  
Vol 60 (03) ◽  
Author(s):  
Ingmar G. E. Renhorn ◽  
Thomas Svensson ◽  
Glenn D. Boreman

2000 ◽  
Vol 106 (1) ◽  
pp. 65-80 ◽  
Author(s):  
J.E Castle ◽  
H Chapman-Kpodo ◽  
A Proctor ◽  
A.M Salvi

2020 ◽  
Vol 31 (10) ◽  
Author(s):  
Hao Cheng ◽  
Bao-Hua Sun ◽  
Li-Hua Zhu ◽  
Tian-Xiao Li ◽  
Guang-Shuai Li ◽  
...  

2011 ◽  
Vol 53 (10) ◽  
pp. 749-762 ◽  
Author(s):  
Geon-Ho Jahng ◽  
Songfan Xu ◽  
Micheal W. Weiner ◽  
Dieter J. Meyerhoff ◽  
Seungjoon Park ◽  
...  

2003 ◽  
Vol 70 (5) ◽  
pp. 317
Author(s):  
S. K. Dvoruk ◽  
I. N. Efimov ◽  
V. N. Kornienko ◽  
I. V. Kochikov ◽  
M. V. Lelkov ◽  
...  

2021 ◽  
Vol 5 (0) ◽  
pp. 0-0
Author(s):  
Anatolii D. Skorbun ◽  
◽  
Gennadii I. Odinokin ◽  
Oleksandr A. Kuchmagra

1984 ◽  
Vol 219 (2) ◽  
pp. 336-338 ◽  
Author(s):  
E.A. Sokol ◽  
Pham Ngoc Chuong ◽  
V.I. Smirnov ◽  
M.P. Ivanov ◽  
G.M. Ter-Akopian ◽  
...  

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