scintillator material
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Author(s):  
C. H. Zepeda Fernández ◽  
Hernández Aguilar Javier Efrén ◽  
E. Moreno-Barbosa

The high time resolution detectors are relevant in those experiments or simulations were the particles to detect, have a very short time of flight (TOF), and due this it´s required that the detections times are ranged between ns. & ps.Using Geant4 software, it was made thirty simulations of coupled detectors to plastic scintillators with two silicon photomultipliers (SiPMs) located on the scintillator’s central sides. To characterize the time resolution, it was required to quantify the optical photons that reach the Score in a certain time, which are generated by muons on the surface of the plastic scintillator. Different configurations of muon beams were simulated at energy of 1 GeV, to interact with the configuration of the scintillator material of its corresponding arrangement. The simulations were made varying three parameters: the scintillator material “BC404 & BC422”, its size, and the location of the radiation source. Fifteen simulations correspond to BC404 material & fifteen simulations to BC422 material respectively. The first five simulations consisted in varying the scintillator’s volumetric size and collocate the muons beam guided randomly distributed over it, the next five simulations differentiate from setting up a directly centered beam, and the last five simulations for guide the beam on the left lower corner of each scintillator.The best time resolution achieved was σ= 8.67 +/− 0.26 ps., reported by the detector with BC422 scintillator material which has a volume of 20x20x3 mm3.


2021 ◽  
Vol 13 (1) ◽  
pp. 25-30
Author(s):  
Akmal Ferdiyan ◽  
Urip Nurwijayanto Prabowo

Neutrino can carry information from places that cannot be reached by the usual detection mechanism because it has a very weak interaction with matter. This can be utilized to study the heat flow process inside the earth by using information carried by geoneutrino (electron antineutrino). In this sense, it is important to know the characteristics of neutrino interaction with materials. In this study, the cross-section calculation of the electron antineutrino interaction with Ar-40 and Kr-84 was carried out using computational methods with the help of GENIE software. In the energy range of 0-10 MeV, the dominant interaction between the two materials is the interaction of QES NC and MEC types with an energy threshold of 5,09 MeV. Both Ar-40 and Kr-84 cannot be used as a scintillator material for geoneutrino detection because in the energy range 0-4,4 MeV the cross-sectional value of the CC interaction  is 0.


2019 ◽  
Vol 14 (06) ◽  
pp. P06037-P06037
Author(s):  
K. Mizukoshi ◽  
T. Iida ◽  
I. Ogawa ◽  
K. Shimizu ◽  
S. Kurosawa ◽  
...  

2019 ◽  
Vol 7 (45) ◽  
pp. 14342-14349 ◽  
Author(s):  
Mao-Hua Du ◽  
Hongliang Shi ◽  
S. B. Zhang

First-principles studies of electronic structures, excitons, and defects in Li2B12H12 reveal unique photophysical properties of Li2B12H12 and its potential as a neutron scintillator material.


2018 ◽  
Vol 51 (2) ◽  
pp. 498-504 ◽  
Author(s):  
Drew R. Onken ◽  
Richard T. Williams ◽  
Didier Perrodin ◽  
Tetiana Shalapska ◽  
Edith D. Bourret ◽  
...  

BaBrCl:Eu is a promising scintillator material; however, the crystal growth yield must be improved for it to become commercially viable. This study measures strain accumulations in the crystal lattice which can contribute to cracking during post-growth cooling. Neutron diffraction is used to measure the crystal structure of undoped and 5 mol% europium-doped BaBrCl from 303 to 1073 K, approaching the melting point. Rietveld analysis of these data provides the temperature dependence of the thermal and chemical strain in BaBrCl. In particular, anisotropic thermal expansion is measured, with expansion along thebaxis nearly double the expansion along theaandcaxes. Additionally, the chemical strain from the incorporation of europium atoms peaks around 673 K, explaining cracking frequently observed in that temperature range.


Author(s):  
Martin Pokorný ◽  
Petr Horodyský ◽  
Martin Nikl ◽  
Jindřich Houžvička

2015 ◽  
Vol 157 ◽  
pp. 318-321 ◽  
Author(s):  
Pradeep Kumar ◽  
Agnikumar G. Vedeshwar

2015 ◽  
Vol 10 (04) ◽  
pp. P04007-P04007 ◽  
Author(s):  
B. Játékos ◽  
E. Lőrincz ◽  
A. Barócsi ◽  
G. Erdei

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