The Simulation of the quenching factor and the channeling effect for the CsI(Tl) and NaI(Tl) crystals Juhee Lee and Sunkee Kim 151-747 Seoul National University.

Slides:



Advertisements
Similar presentations
Fig. 4-1, p Fig. 4-2, p. 109 Fig. 4-3, p. 110.
Advertisements

Studies for a silicon detector in a e/A collider Benedetto Di Ruzza BNL EIC Task Force meeting August 28 th 2014.
Ion Beam Analysis techniques:
Geant4 Low Energy Polarized Compton Processes Gerardo Depaola * Francesco Longo + Francesco Longo + * National University of Córdoba (Argentina) + University.
PET Design: Simulation Studies using GEANT4 and GATE - Status Report - Martin Göttlich DESY.
Tomsk Polytechnic University1 A.S. Gogolev A. P. Potylitsyn A.M. Taratin.
Introducing Channeling Effect
Analysis and Results 3.Gamma-ray Spectra of 134 Cs The background subtracted spectra of 605 keV and 796 keV in multiple hit events, and their coincidence.
P.464. Table 13-1, p.465 Fig. 13-1, p.466 Fig. 13-2, p.467.
Fig. 11-1, p p. 360 Fig. 11-2, p. 361 Fig. 11-3, p. 361.
Tests of scintillators CsI, CsI(Na), BGO, NaI(Tl) CsI(Tl)
Table 6-1, p Fig. 6-1, p. 162 p. 163 Fig. 6-2, p. 164.
Microelectronics Processing
Recent results from CERN NA59 Richard Jones, University of Connecticut GlueX collaboration meetingMay , Bloomington Does the enhancement seen.
Lecture 2-Building a Detector George K. Parks Space Sciences Laboratory UC Berkeley, Berkeley, CA.
ECE/ChE 4752: Microelectronics Processing Laboratory
Workshop on Physics on Nuclei at Extremes, Tokyo Institute of Technology, Institute for Nuclear Research and Nuclear Energy Bulgarian Academy.
Absolute light output determination of crystal scintillators
JSPS Research Fellow / University of Tsukuba T. Horaguchi Oct for HAWAII /10/15HAWAII
Dark Matter Search with Direction sensitive Scintillator Ⅱ Department of Physics, School of Science The University of Tokyo Y. Shimizu, M. Minowa, Y. Inoue.
Experiments on beam deflection by crystals Masataka IINUMA Department of Quantum Matter Graduate School of Advanced Sciences of Matter Hiroshima University.
Space Instrumentation. Definition How do we measure these particles? h p+p+ e-e- Device Signal Source.
Annual Modulation Study of Dark Matter Using CsI(Tl) Crystals In KIMS Experiment J.H. Choi (Seoul National University) SUSY2012, Beijing.
Ion Implantation and Ion Beam Analysis of Silicon Carbide Zsolt ZOLNAI MTA MFA Research Institute for Technical Physics and Materials Science Budapest,
Recent status of dark matter search with ULE-HPGe detector Tsinghua University Qian Yue nd Korea-China Joint Seminar on Dark Matter Search.
Calibration of the new Particle Identification Detector (PID) Tom Jude, Derek Glazier, Dan Watts.
1 Energy loss correction for a crystal calorimeter He Miao Institute of High Energy Physics Beijing, P.R.China.
Meta-stable Sites in Amorphous Carbon Generated by Rapid Quenching of Liquid Diamond Seung-Hyeob Lee, Seung-Cheol Lee, Kwang-Ryeol Lee, Kyu-Hwan Lee, and.
KPS Chonbuk University 2005/10/22 HYUNSU LEE Status of the KIMS dark matter search experiment with CsI(Tl) crystals Hyun Su Lee Seoul National.
1 Experimental particle physics introduction. 2 What holds the world together?
Daily Modulation of the Dark Matter Signal in Crystalline Detectors Nassim Bozorgnia UCLA TexPoint fonts used in EMF. Read the TexPoint manual before you.
Muon flux at Y2L and reconstruction of muon tracks
WIMP search Result from KIMS experiments Kim Seung Cheon (DMRC,SNU)
KIMS Seoul National University Juhee Lee 1 KPS in Changwon.
How to Obtain the Number of Sub-Atomic Particles in an Atom Using a Periodic Table ProtonsNeutronsElectrons Equal to the atomic # on the Periodic Table.
What are ionic bonds? Section 15-5.
Geant4 Tutorial, Oct28 th 2003V. Daniel Elvira Geant4 Simulation of the CMS 2002 Hcal Test Beam V. Daniel Elvira Geant4 Tutorial.
Simultaneous photo-production measurement of the  and  mesons on the nucleons at the range 680 – 1500 MeV N.Rudnev, V.Nedorezov, A.Turinge for the GRAAL.
Acquisition time6 min1 min 12 s Collimator height25 mm (Anger)12 mm (HiSens) Detector1 layer, 1 pixel / hole3 layers, 1 pixel / hole3 layers, 4 pixels.
PyungChang 2006/02/06 HYUNSU LEE CsI(Tl) crystals for WIMP search Hyun Su Lee Seoul National University (For The KIMS Collaboration)
Sep. 22, 2011 Seoul National University Jae Keum Lee KIMS Background 1 China-Korea Workshop 2011 September 22-23, 2011.
Optimization of Scintillators for Stacked-layer Detectors of FNGR 1,2 Jea Hyung Cho, 1,2 Kwang Hyun Kim *, and 3 Young Hyun Jung 1 Biomedical Engineering,
Seoul National University Han-wool Ju CUNPA Kick-off Meeting Aug.22-23, 2013.
1 Semiempirical calculation of quenching factors for ions in scintillators V.I. Tretyak Institute for Nuclear Research, MSP Kyiv, Ukraine AMORE Collaboration.
RAON Simulation Chanyoung Llagi Lee Yonsei HEP.
Optimization of Scintillators for Stacked-layer Detectors of FNGR 1,2 Jea Hyung Cho, 1,2 Kwang Hyun Kim *, and 3 Young Hyun Jung 1 Biomedical Engineering,
A Measurement of the Ultra-High Energy Cosmic Ray Spectrum with the HiRes FADC Detector (HiRes-2) Andreas Zech (for the HiRes Collaboration) Rutgers University.
Characteristics of Miniaturized CsI(Tl) Scintillator for Mobile Radiation Detector Hyunjun Yoo 1, Chankyu Kim 1, Yewon Kim 1, Eunjoong Lee 1, Segyeong.
Yonsei University Combinatorial pair background in the e + e - mass spectra in p+p collisions at √s = 14TeV Yonsei Univ. M. G. Song, D. H. Lee, B. K. Kim,
Status of ULE-HPGe Experiment for WIMP Search in YangYang
V.I. Tretyak Institute for Nuclear Research, MSP Kyiv, Ukraine
Status of 100Mo based DBD experiment
“minimum-ionisation” peak
Sr-84 0n EC/b+ decay search with SrCl2 crystal
Sang-Pil Kim1,2, Kwang-Ryeol Lee1, Jae-Sung Kim3 and Yong-Chae Chung2
PARTICLE FLUX CALCULATION-III
PP-25 Rearrangement Effect of Surface Atoms on the Alternation of Patterning Regime: Incident Energy Effect of Ar Haeri Kim1,2, Sang-Pil Kim1, and Kwang-Ryeol.
Atmospheric Muon This is a muon that was produced naturally from cosmic rays hitting the atmosphere. Only the highest energy muons can penetrate the.
Name That Atom! Use your knowledge of atoms to find the name of each of the following atoms. Use a Periodic Table!
Electron Distribution in Keto-Enol Tautomers
Jing Han, Kristyna Pluhackova, Tsjerk A. Wassenaar, Rainer A. Böckmann 
Two-dimensional Lattice Boltzmann Simulation of Liquid Water Transport
Neutron Beam Test for Measuring Quenching Factor of CsI(Tl) Crystal
Study of e+e- pp process using initial state radiation with BaBar
NKS2 Meeting with Bydzovsky NKS2 Experiment / Analysis Status
Study of Event Reconstruction for Saturated Pulse
Chetan Poojari, Dequan Xiao, Victor S. Batista, Birgit Strodel 
Ion-Induced Defect Permeation of Lipid Membranes
The Selectivity of K+ Ion Channels: Testing the Hypotheses
Update on POLA-01 measurements in Catania
Presentation transcript:

The Simulation of the quenching factor and the channeling effect for the CsI(Tl) and NaI(Tl) crystals Juhee Lee and Sunkee Kim Seoul National University Shillim-dong Kwanak-gu Seoul Korea, Republic of. In the saturation model, the scintillation efficiency can be described by the stopping power of an ion and the concentration of activated ions. It is supported by the experiments for the electron, proton and alpha(fig.1) and can be extended to other ions of higher atomic numbers. With that relation and the simulation tool, we can reproduce the measured energy spectrum of a scintillation detector. We use MARLOWE and TRIM as BC and MD simulation tools respectively. When an ion goes into the symmetric axis or plain, it can interact with only electrons, thus, its penetration and light yield are drastically increased. It is due to the channeling or blocking effect according to the start position of an ion. We can simulate these effects in MARLOWE and estimate the measured energy spectrum with this consideration. Scintillation efficiency Energy loss functions Fig.1 Scintillation efficiency of CsI(Tl) Black ones are experimental results and Red ones from calculation. Fig.1 Scintillation efficiency of CsI(Tl) Black ones are experimental results and Red ones from calculation. Fig.2 The electronic Stopping Power in the amorphous CsI Red line is MARLOWE and Blue line TRIM. Fig.2 The electronic Stopping Power in the amorphous CsI Red line is MARLOWE and Blue line TRIM. 5keV10keV15keV20keV50keV [111] [100] [110] 9.4  7.9  7.2  6.7  Table.1 Comparing of the axial critical angles A Cs ion goes into the symmetric axes of CsI(Tl). Black one is Lindhard ‘s  2, Red one  of Fig6. Table.1 Comparing of the axial critical angles A Cs ion goes into the symmetric axes of CsI(Tl). Black one is Lindhard ‘s  2, Red one  of Fig6. Fig.3 Quenching factors for Cs in CsI(Tl) Fig.3 Quenching factors for Cs in CsI(Tl) Fig.4 Quenching factors for NaI(Tl) Red is for Na ion and Black for I ion. Fig.4 Quenching factors for NaI(Tl) Red is for Na ion and Black for I ion. Fig.9 Measured energy of tail events Fig.9 Measured energy of tail events Fig.7 Penetrations from a lattice point Fig.7 Penetrations from a lattice point 5keV10keV15keV20keV50keV [100] [110] [111] 9.5 · 8.0 · 7.2 · 6.7 · 5.3 · Table.2 Comparing of the critical angles An I ion goes into the symmetric axes of NaI(Tl). Table.2 Comparing of the critical angles An I ion goes into the symmetric axes of NaI(Tl). Fig.6 Initial theta distribution of tail events Fig.6 Initial theta distribution of tail events Fig.8 Initial theta distributions of tail events Red, Black, Blue,Brown Fig.8 Initial theta distributions of tail events Red, Black, Blue,Brown Fig.5 Penetrations from an empty site Red,Blue,Black Fig.5 Penetrations from an empty site Red,Blue,Black