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http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/68298完整後設資料紀錄
| DC 欄位 | 值 | 語言 |
|---|---|---|
| dc.contributor.advisor | 闕志鴻(Tzihong Chiueh),蘇游瑄(Sherry Suyu) | |
| dc.contributor.author | James Hung-Hsu Chan | en |
| dc.contributor.author | 詹弘旭 | zh_TW |
| dc.date.accessioned | 2021-06-17T02:16:57Z | - |
| dc.date.available | 2018-01-04 | |
| dc.date.copyright | 2018-01-04 | |
| dc.date.issued | 2017 | |
| dc.date.submitted | 2017-09-19 | |
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| dc.identifier.uri | http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/68298 | - |
| dc.description.abstract | 揭曉暗物質 (dark matter, DM) 的本質在現代宇宙學中是非常重要的 課題。分折暗物質的結構更是對於星系生成及演化和大尺度結構非常 的關鍵。為了完成這個目標，我們同時使用宇宙數值模擬和天文觀測 資料。特別的是，我們使用重力透鏡效應 (grivatational lensing) 去探索 宇宙的黑暗成份。我們發表一套新的工具，CHITAH，去偵測影像巡 天觀測中的重力透鏡系統。CHITAH 已經在超廣角可見光相機巡天計 畫中 (the HSC survey) 尋找到數個有公信力的系統，並有計劃進行後續 觀測。在模擬部份，我們發表了一段有效演化波暗物質 (ψDM) 和星粒 子的工具。我們發現星系中的孤粒子核 (soliton) 會因為星粒子的重力 而吸收約二倍的質量，並滿足比例關係。在未來，使用類星體重力透 鏡系統和宇宙模擬能使我們證實/推翻波暗物質的模型。 | zh_TW |
| dc.description.abstract | Unveiling the nature of dark matter has become the golden question in modern cosmology, and understanding the structure/sub-structure of dark mat- ter in the Universe is important for our understanding of the formation/evolution of galaxies and large-scale structures. To achieve this goal, we conduct both cosmological simulations and astrophysical observations. In particular, we exploit a direct technique, gravitational lensing, to explore the dark side of the Universe. We present a novel algorithm, CHITAH, to classify lens systems in imaging surveys. CHITAH has classified a few promising lens candidates in the Hyper-Surprime Cam (HSC) survey, including lensed quasars and lensed galaxies with follow-up observations planned. In the simulation regime, we present an efficient algorithm for wave-like dark matter (ψDM) model plus stars. We discover that a solitonic core can absorb mass by a factor of 2 from its host halo to satisfy the scaling relation even in the presence of additional star gravity. Using lensed quasars and comparing with simulation results will allow us confirm/disconfirm ψDM model. | en |
| dc.description.provenance | Made available in DSpace on 2021-06-17T02:16:57Z (GMT). No. of bitstreams: 1 ntu-106-D00222002-1.pdf: 8902676 bytes, checksum: 6ef4a2fbe678417878eafc15ff765f3f (MD5) Previous issue date: 2017 | en |
| dc.description.tableofcontents | Contents
Acknowledgements v 摘要 vii Abstract ix 1 Introduction 1 1.1 Shorthistoryofdarkmatter......................... 1 1.2 Thenatureofdarkmatter.......................... 2 1.3 Detectionofdarkmatter .......................... 4 2 Gravitational Lensing 7 2.1 Gravitationallensequation ......................... 9 2.2 Strong gravitational lensing: galaxy-scale lens model . . . . . . . . . . . 13 3 CHITAH: Strong-gravitational-lens hunter in imaging surveys 17 3.1 StrategyofCHITAH ............................ 17 3.1.1 Separationoflensandquasars................... 18 3.1.2 Identifications of quasar image positions and lens center..... 21 3.1.3 Potential quads and doubles via configuration . . . . . ...... 23 3.1.4 Classificationvialensmodelfitting . . . . . . . . . . . . . . . . 23 3.2 SimulationforCHITAH .......................... 25 3.3 TheperformanceofCHITAH........................ 27 3.3.1 SimulationswithGaussianPSF .................. 28 3.3.2 SimulationswithMoffatPSF.................... 32 3.4 ApplicationtoCOSMOS5921+0638 ................... 33 3.4.1 ObservationsofCOSMOS5921+0638 . . . . . . . . . . . . . . 34 3.4.2 CHITAHonCOSMOS5921+0638 ................ 35 3.5 SummaryandDiscussions ......................... 37 4 Galaxy-scale gravitational lens candidates from GAMA and HSC 41 4.1 Observation................................. 41 4.1.1 GAMAblendedspectracatalog .................. 41 4.1.2 HSCimaging............................ 42 4.2 Method ................................... 43 4.2.1 Selection via morphology and redshift information . . . . . . . . 43 4.2.2 Lensmodel............................. 44 4.3 GravitationallenscandidatesfromHSCsurvey . . . . . . . . . . . . . . 45 4.3.1 Probablelenscandidates ...................... 46 4.3.2 A promising interacting-galaxy lens candidate from HSC survey . 46 4.4 SummaryandDiscussions ......................... 50 5 Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). I. Automatic search for galaxy-scale strong lenses 53 5.1 Data..................................... 54 5.1.1 HSCphotomerty .......................... 54 5.1.2 BOSSspectroscopyandtargetselection . . . . . . . . . . . . . . 54 5.2 CHITAHforSuGOHI-g .......................... 55 5.3 CandidatesfromHSC+BOSS........................ 56 5.4 Discussion.................................. 57 6 How do stars affect ψDM halos? 63 6.1 Introduction................................. 63 6.2 Simulation.................................. 66 6.2.1 ψDM................................ 66 xii 6.2.2 CDM................................ 67 6.3 FundamentalissuesofψDMhalo...................... 69 6.3.1 Soliton+stars............................ 69 6.3.2 ψDM5.0×109M⊙withstars ................... 70 6.3.3 Solitonmerger ........................... 73 6.4 Results.................................... 75 6.4.1 Initialstellardistribution...................... 75 6.4.2 TestwithψDMandCDMhalos .................. 77 6.5 ConclusionandDiscussion......................... 78 7 A New Method for Computing Self-gravity in an Isolated System 87 7.1 Motivationsofthenewmethod....................... 87 7.2 Detailedcorrectionprocedures ....................... 89 7.3 Numericalexamples ............................ 90 7.4 Discussion.................................. 98 8 Summary and Future Prospects 101 A The possible lens candidates from GAMA in the HSC survey 103 B Template Density-Potential Pairs 107 Bibliography 111 | |
| dc.language.iso | en | |
| dc.subject | 重力透鏡 | zh_TW |
| dc.subject | 暗物質 | zh_TW |
| dc.subject | dark matter | en |
| dc.subject | gravitational lensing | en |
| dc.title | 藉由重力透鏡研究暗物質之結構 | zh_TW |
| dc.title | Studying Dark Matter Structure via Gravitational Lensing | en |
| dc.type | Thesis | |
| dc.date.schoolyear | 106-1 | |
| dc.description.degree | 博士 | |
| dc.contributor.oralexamcommittee | 林彥廷(Yen-Ting Lin),湯姆 布羅姆赫斯特(Tom Broadhurst),奧村哲平(Teppei Okumura) | |
| dc.subject.keyword | 暗物質,重力透鏡, | zh_TW |
| dc.subject.keyword | dark matter,gravitational lensing, | en |
| dc.relation.page | 127 | |
| dc.identifier.doi | 10.6342/NTU201704218 | |
| dc.rights.note | 有償授權 | |
| dc.date.accepted | 2017-09-19 | |
| dc.contributor.author-college | 理學院 | zh_TW |
| dc.contributor.author-dept | 物理學研究所 | zh_TW |
| 顯示於系所單位： | 物理學系 | |
文件中的檔案：
| 檔案 | 大小 | 格式 | |
|---|---|---|---|
| ntu-106-1.pdf 未授權公開取用 | 8.69 MB | Adobe PDF |
系統中的文件，除了特別指名其著作權條款之外，均受到著作權保護，並且保留所有的權利。