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Blocking effect in CsI(Tl) crystal by neutron
DC Field | Value | Language |
---|---|---|
dc.contributor.advisor | 최선호 | - |
dc.contributor.author | 주한울 | - |
dc.date.accessioned | 2017-07-19T09:16:44Z | - |
dc.date.available | 2017-07-19T09:16:44Z | - |
dc.date.issued | 2013-08 | - |
dc.identifier.other | 000000013711 | - |
dc.identifier.uri | https://hdl.handle.net/10371/131688 | - |
dc.description | 학위논문 (석사)-- 서울대학교 대학원 : 물리·천문학부(물리학전공), 2013. 8. 최선호. | - |
dc.description.abstract | To detect WIMP directly, which is strong candidate for dark matter, KIMS
collaboration used CsI(Tl) crystal as a scintillation detector. To increase the detector`s sensitivity, we studied channeling and blocking effect in the CsI(Tl) crystal, which refer to the orientation dependence of charged ion`s penetration in crystals. It results in modulation of scintillation or ionization yield in the CsI(Tl) crystal. In order to measure the channeling and blocking effect in CsI(Tl) crystal, we used a CsI(Tl) crystal, a neutron generator, and three neutron detectors, with making the directions of recoil ions induced by the neutron-nucleus scatterings to be aligned along one of the symmetry axis or plane in the CsI(Tl) crystal. Also, we did simulations to compare their results with the data obtained from our experimental setup, by two kinds of computer simulations, MARLOWE and Geant4. To confirm the affection of the blocking effect in the CsI(Tl) crystal, we compared the light yields of recoil ions moving along the symmetry axis, [110], and those of recoil ions moving along random directions, and compared mean decay time of signals from each recoil direction. By comparing those from experiments and simulations, we could find a clue for the blocking effect which is expected to result in less scintillation light yields. | - |
dc.description.tableofcontents | 1 Introduction 1
1.1. CsI(Tl) crystal as a dark matter detector . . . . . . . . . . . . . . . . . . 1 1.2. Channeling and Blocking Effect on the CsI(Tl) crystal . . . . . . 3 1.3. Daily and Annual modulation for WIMP research . . . . . . . . . . 5 1.4. Motivation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5 2 Experiment 7 2.1. Goal of this experiment . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7 2.2. Experimental Setup . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8 2.2.1. Neutron Generator . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8 2.2.2. CsI(Tl) crystal . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10 2.2.3. Neutron Detector . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12 2.3. DAQ and event selection . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15 3 Simulation 19 3.1. MARLOWE . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19 3.2. Geant4 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23 4 Data Analysis & result 26 5 Conclusion 37 Bibliography 39 | - |
dc.format | application/pdf | - |
dc.format.extent | 1371109 bytes | - |
dc.format.medium | application/pdf | - |
dc.language.iso | en | - |
dc.publisher | 서울대학교 대학원 | - |
dc.subject | Dark matter | - |
dc.subject | WIMPs | - |
dc.subject | KIMS | - |
dc.subject | CsI(Tl) crystal | - |
dc.subject | Channeling effect | - |
dc.subject | Blocking effect | - |
dc.subject.ddc | 523 | - |
dc.title | Blocking effect in CsI(Tl) crystal by neutron | - |
dc.type | Thesis | - |
dc.description.degree | Master | - |
dc.citation.pages | iv, 40 | - |
dc.contributor.affiliation | 자연과학대학 물리·천문학부(물리학전공) | - |
dc.date.awarded | 2013-08 | - |
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