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| DC 欄位 | 值 | 語言 |
|---|---|---|
| dc.contributor.advisor | 陳丕燊(Pisin Chen) | |
| dc.contributor.author | Chung-Hei Leung | en |
| dc.contributor.author | 梁仲希 | zh_TW |
| dc.date.accessioned | 2021-06-16T10:42:12Z | - |
| dc.date.available | 2020-08-04 | |
| dc.date.copyright | 2020-08-04 | |
| dc.date.issued | 2020 | |
| dc.date.submitted | 2020-07-08 | |
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| dc.identifier.uri | http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/61027 | - |
| dc.description.abstract | 極高能宇宙射線及宇宙微中子的研究已行之有年,而近年來關於無線電波波段的探測方法逐漸地被開發、討論。南極天文粒子地磁同步輻射觀測站 (Taiwan Astroparticle Radio Observatory of GeosynchrotronEmission,簡稱 TAROGEM) 探測無線電波,坐立於南極的墨爾本山上,以 3 支水平及 1 支垂直指向北面的天線來觀測掠過地球的宇宙微中子 (EarthSkimming Neutrino) 。由於墨爾本山是羅斯冰架附近比較高的山,與附近的地形有足夠的距離,容讓從微中子演變的濤子 (Tau lepton) 有足夠的距離發展大氣簇射,與地磁作用並引發足夠的電磁波。借此,TAROGEM 才有能力觀測掠過地球的微中子訊號。本論文就 TAROGEM 的條件進行模擬,探討此系統探測掠過地球的宇宙微中子的可行性,並就 ANITA (ANtarctic Impulse Transient Antenna) 及另一由台大次震宇宙館負責的 ARIANNA-HCR 進行模擬,從而確定模擬的可信性及廣泛性,並比較各實驗對濤子微中子的靈敏度。此外,南極的熱氣球實驗 (ANITA) 從過去三次飛行中獲得豐碩的成果之後,2016 年進行了第四次的飛行。而 ANITA-I 及 ANITA-III 分別各測量到一次異常的訊號。由於目前仍沒有確切的物理背景能解釋這兩個訊號 的來源,世界各地的物理學家都正以不同的理論嘗試了解當中的原因。本論文亦會探討倘若異常訊號的物理過程與濤子微中子一樣的情況下,TAROGE-M 理應接收到多少此等訊號。 | zh_TW |
| dc.description.abstract | The detection of the ultra high energy cosmic rays (UHECRs) and the cosmic neutrinos has been studied for ages. In the past decades, the use of radio frequency waves (RF) to detect UHE cosmic rays and neutrinos has advanced significantly. The Taiwan Astroparticle Radio Observatory of Geosynchrotron Emission Mt. Melbourne (TAROGE-M) detects ultra wide band impulsive radio frequency (RF) signals emitted by the air shower with three horizontal and one vertical antennas pointing to North. It was located on top of Mt. Melbourne in Antarctica. The height of Mt. Melbourne helps the detection of radio signal because the air showers have enough distance to develop and deflect by the geomagnetic field for creating a detectable signal before reaching the detector on the mountain. This thesis I present a comprehensive study of the sensitivity of TAROGE-M to a diffuse tau neutrino flux detected via tau lepton induced air showers with the standard model. Besides, I will present the comparison of experiments, including TAROGE-M, ANtarctic Impulse Transient Antenna (ANITA) and ARIANNA-HCR, with the same simulation in order to show the flexibility and reliability of this simulation. ANITA collaboration has recently reported the observation of two anomalous up-going air shower events with air shower energies of 0.6 EeV, observed during the first and the third flight. Since there is no concrete explanation of these two events, physicists around the world are trying to interpret them with different hypothesis. This thesis would also predict how many same kind of events TAROGE-M should detect, assuming the mechanism of these events and tau neutrino are the same. | en |
| dc.description.provenance | Made available in DSpace on 2021-06-16T10:42:12Z (GMT). No. of bitstreams: 1 U0001-0107202014560600.pdf: 5019245 bytes, checksum: 79d28cfcb0741219eeb0d8ce95c0a9b2 (MD5) Previous issue date: 2020 | en |
| dc.description.tableofcontents | 口試委員會審定書 iii 誌謝 v Acknowledgements vii 摘要 ix Abstract xi 1 Introduction 1 2 UltraHigh Energy Astroparticle Physics 3 2.1 The Cosmic Ray Spectrum 3 2.1.1 The Greisen–Zatsepin–Kuzmin Effect 5 2.2 Neutrinos 6 3 The Standard Model and Neutrino Physics 9 3.1 Differential Cross Section νN scattering 10 3.2 Cross section for νN scattering 10 4 Lepton Physics 13 4.1 Electron 13 4.2 Muon 14 4.2.1 Decay 14 4.2.2 Energy Loss 15 4.3 Tau 18 4.3.1 Decay 18 4.3.2 Energy Loss 19 5 Radio Emission in Ultra-High Energy Particle Showers 23 5.1 Air Shower 23 5.1.1 Electromagnetic shower 23 5.1.2 Hadronic shower 24 5.2 Radio Emission by Particle Cascade 25 5.2.1 Coherence 25 5.3 Emission Mechanism 28 5.3.1 Geomagnetic effect 28 5.3.2 Askaryan effect 30 6 The Antarctic Impulsive Transient Antenna 33 6.1 Detection Concept 33 6.2 Result: Two Anomalous Events 34 7 ARIANNA Horizontal Cosmic Ray 39 7.1 Detection Concept 40 7.2 Cosmic ray search and background rejection 41 8 Taiwan Astroparticle Radio Observatory of Geosynchrotron Emission - MtMelbourne 43 8.1 Detection Concept 43 9 Event Simulation 45 9.1 Geometry Model 45 9.2 Atmosphere Model 47 9.3 SHINIE 48 9.3.1 Isotropy 48 9.3.2 Neutrino Simulation 49 9.3.3 Tau Lepton Propagation 53 9.4 TAUOLA 55 9.4.1 Discussion 58 9.5 CORSIKA and CoREAS 59 9.5.1 Discussion 61 9.6 Detection Model 62 9.6.1 System Response Simulation 62 9.6.2 Parametrization of peak voltage 64 9.6.3 Depth of shower maximum Xmax 72 9.6.4 Monte Carlo simulations 74 10 Verification and validation of the simulation model 75 10.1 Geometry 75 10.2 Verification of SHINIE 76 10.3 Distribution of Tau Energy 77 10.4 Radio Emission Model and Detection Model 77 10.5 Monte Carlo simulation 79 10.6 Reproduce the figure of acceptance 80 11 Result 83 12 Conclusion 87 Bibliography 89 | |
| dc.language.iso | en | |
| dc.subject | 無線電波 | zh_TW |
| dc.subject | 中微子 | zh_TW |
| dc.subject | 宇宙射線 | zh_TW |
| dc.subject | Cosmic ray | en |
| dc.subject | neutrino | en |
| dc.subject | radio wave | en |
| dc.subject | tau | en |
| dc.title | 宇宙微中子之無線電波探測研究 | zh_TW |
| dc.title | Studies of the Radio Wave Detection of Earth-Skimming Tau Neutrinos for TAROGE-M | en |
| dc.type | Thesis | |
| dc.date.schoolyear | 108-2 | |
| dc.description.degree | 碩士 | |
| dc.contributor.advisor-orcid | 陳丕燊(0000-0001-5251-7210) | |
| dc.contributor.coadvisor | 南智祐(Jiwoo Nam) | |
| dc.contributor.oralexamcommittee | 胡德邦(Tak Pong Woo) | |
| dc.subject.keyword | 宇宙射線,中微子,無線電波, | zh_TW |
| dc.subject.keyword | Cosmic ray,neutrino,radio wave,tau, | en |
| dc.relation.page | 96 | |
| dc.identifier.doi | 10.6342/NTU202001239 | |
| dc.rights.note | 有償授權 | |
| dc.date.accepted | 2020-07-08 | |
| dc.contributor.author-college | 理學院 | zh_TW |
| dc.contributor.author-dept | 天文物理研究所 | zh_TW |
| 顯示於系所單位： | 天文物理研究所 | |
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