請用此 Handle URI 來引用此文件:
http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/61027
完整後設資料紀錄
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 | |
dc.identifier.citation | [1] A. Aab et al. Probing the radio emission from air showers with polarization mea surements. Phys. Rev. D, 89:052002, Mar 2014. [2] H. Abramowicz and A. Levy. The allm parameterization of sigma tot (gamma ∗ p) an update, 1997. [3] P. Abreu et al. Interpretation of the depths of maximum of extensive air showers measured by the pierre auger observatory. Journal of Cosmology and Astroparticle Physics, 2013(02):026–026, feb 2013. [4] F. Aharonian et al. Energy spectrum of cosmicray electrons at tev energies. Phys. Rev. Lett., 101:261104, Dec 2008. [5] P. Allison, J. Auffenberg, R. Bard, J. Beatty, D. Besson, S. Böser, C. Chen, P. Chen, A. Connolly, J. Davies, M. DuVernois, B. Fox, P. Gorham, E. Grashorn, K. Han son, J. Haugen, K. Helbing, B. Hill, K. Hoffman, E. Hong, M. Huang, M. Huang, A. Ishihara, A. Karle, D. Kennedy, H. Landsman, T. Liu, L. Macchiarulo, K. Mase, T. Meures, R. Meyhandan, C. Miki, R. Morse, M. Newcomb, R. Nichol, K. Rat zlaff, M. Richman, L. Ritter, C. Rott, B. Rotter, P. Sandstrom, D. Seckel, J. Touart, G. Varner, M.Z. Wang, C. Weaver, A. Wendorff, S. Yoshida, and R. Young. Design and initial performance of the askaryan radio array prototype eev neutrino detector at the south pole. Astroparticle Physics, 35(7):457 – 477, 2012. [6] J. AlvarezMuñiz, W. R. Carvalho, K. Payet, A. RomeroWolf, H. Schoorlemmer, and E. Zas. Comprehensive approach to taulepton production by highenergy tau neutrinos propagating through the earth. Phys. Rev. D, 97:023021, Jan 2018. [7] J. AlvarezMuñiz, W. R. Carvalho, A. RomeroWolf, M. Tueros, and E. Zas. Coher ent radiation from extensive air showers in the ultrahigh frequency band. Phys. Rev. D, 86:123007, Dec 2012. [8] J. AlvarezMuniz, M. Risse, G. I. Rubtsov, and B. T. Stokes. Review of the Multi messenger Working Group at UHECR2012. EPJ Web Conf., 53:01009, 2013. [9] J. AlvarezMuñiz, W. R. Carvalho, and E. Zas. Monte carlo simulations of radio pulses in atmospheric showers using zhaires. Astroparticle Physics, 35(6):325 – 341, 2012. [10] G. A. Askar’yan. Excess negative charge of an electronphoton shower and its co herent radio emission. Sov. Phys. JETP, 14(2):441–443, 1962. [Zh. Eksp. Teor. Fiz.41,616(1961)]. [11] S. Barwick, E. Berg, D. Besson, G. Binder, W. Binns, D. Boersma, R. Bose, D. Braun, J. Buckley, V. Bugaev, S. Buitink, K. Dookayka, P. Dowkontt, T. Duffin, S. Euler, L. Gerhardt, L. Gustafsson, A. Hallgren, J. Hanson, M. Israel, J. Kiryluk, S. Klein, S. Kleinfelder, H. Niederhausen, M. Olevitch, C. Persichelli, K. Ratzlaff, B. Rauch, C. Reed, M. Roumi, A. Samanta, G. Simburger, T. Stezelberger, J. Tatar, U. Uggerhoj, J. Walker, G. Yodh, and R. Young. A first search for cosmogenic neu trinos with the arianna hexagonal radio array. Astroparticle Physics, 70:12 – 26, 2015. [12] S. Barwick, E. Berg, D. Besson, E. Cheim, T. Duffin, J. Hanson, S. Klein, S. Kle infelder, T. Prakash, M. Piasecki, K. Ratzlaff, C. Reed, M. Roumi, A. Samanta, T. Stezelberger, J. Tatar, J. Walker, R. Young, and L. Zou. Design and performance of the arianna hexagonal radio array systems. 10 2014. [13] S. Barwick et al. Radio detection of air showers with the arianna experiment on the ross ice shelf. Astroparticle Physics, 90:50 – 68, 2017. [14] J. K. Becker. Highenergy neutrinos in the context of multimessenger physics. Phys. Rept., 458:173–246, 2008. [15] S. F. Berezhnev et al. The primary cr spectrum by the data of the tunka133 array. [16] J. Beringer et al. Review of particle physics. Phys. Rev. D, 86:010001, Jul 2012. [17] S. A. Colgate. The detection of highenergy cosmicray showers by the combined optical and electromagnetic pulse. , 72(19):4869–4879, Oct 1967. [18] W. Commons. File:feynman diagram of decay of tau lepton.svg — wikimedia com mons, the free media repository, 2014. [Online; accessed 10February2020]. [19] W. Commons. File:pair production cartoon.gif — wikimedia commons, the free media repository, 2018. [Online; accessed 10February2020]. [20] W. Commons. File:bremsstrahlung.svg — wikimedia commons, the free media repository, 2019. [Online; accessed 10February2020]. [21] A. Connolly, R. S. Thorne, and D. Waters. Calculation of high energy neutrino nucleon cross sections and uncertainties using the martinstirlingthornewatt par ton distribution functions and implications for future experiments. Phys. Rev. D, 83:113009, Jun 2011. [22] J. W. Cronin, S. P. Swordy, and T. K. Gaisser. Cosmic rays at the energy frontier. Sci. Am., 276:32–37, 1997. [23] K. D. de Vries, O. Scholten, and K. Werner. The air shower maximum probed by Cherenkov effects from radio emission. Astropart. Phys., 45:23–27, 2013. [24] A. M. Dziewonski and D. L. Anderson. Preliminary reference earth model. Physics of the Earth and Planetary Interiors, 25(4):297 – 356, 1981. [25] R. Gandhi, C. Quigg, M. H. Reno, and I. Sarcevic. Ultrahighenergy neutrino inter actions. Astroparticle Physics, 5(2):81 – 110, 1996. [26] D. GarcíaFernández, J. AlvarezMuñiz, W. R. Carvalho, A. RomeroWolf, and E. Zas. Calculations of electric fields for radio detection of ultrahigh energy par ticles. Phys. Rev. D, 87:023003, Jan 2013. [27] P. Gorham et al. The antarctic impulsive transient antenna ultrahigh energy neutrino detector: Design, performance, and sensitivity for the 2006–2007 balloon flight. Astroparticle Physics, 32(1):10 – 41, 2009. [28] P. W. Gorham et al. Characteristics of four upwardpointing cosmicraylike events observed with anita. Phys. Rev. Lett., 117:071101, Aug 2016. [29] P. W. Gorham et al. Observation of an unusual upwardgoing cosmicraylike event in the third flight of anita. Phys. Rev. Lett., 121:161102, Oct 2018. [30] P. W. Gorham et al. Observation of an unusual upwardgoing cosmicraylike event in the third flight of anita. Phys. Rev. Lett., 121:161102, Oct 2018. [31] K. Greisen. End to the cosmicray spectrum? Phys. Rev. Lett., 16:748–750, Apr 1966. [32] B. H., H. W., and D. P. A. Maurice. On the stopping of fast particles and on the creation of positive electrons. Proc. R. Soc. Lond. A, 146, Aug 1934. [33] L. H., K. C. Jezek, B. Li, and Z. Zhao. Radarsat antarctic mapping project digital elevation model, version 2. 400m ramp dem data set. Boulder, Colorado USA. NASA National Snow and Ice Data Center Distributed Active Archive Center., 2015. [34] K. Hagiwara, T. Li, K. Mawatari, and J. Nakamura. Taudecay: a library to simulate polarized tau decays via feynrules and madgraph5. The European Physical Journal C, 73(7):2489, Jul 2013. [35] W. F. Hanlon. Updated Cosmic Ray Spectrum, 2008(accessed 2016). [36] D. Heck, J. Knapp, J. N. Capdevielle, G. Schatz, and T. Thouw. CORSIKA: a Monte Carlo code to simulate extensive air showers., 1998. [37] S.Y. Hsu. Studies of the radio wave detection of cosmic rays and cosmic neutrinos for TAROGE and ANITA. National Taiwan University Master Thesis, pages 1–106, 2016. [38] M.H. Huang. http://pre.tir.tw/096/. [39] M.H. Huang. SHINIE: Simulation of high energy neutrinos interacting with the earth. Nuclear Physics B Proceedings Supplements, 175176:472–475, 01 2008. [40] T. Huege and C. W. James. Full monte carlo simulations of radio emission from extensive air showers with coreas, 2013. [41] S. Iyer Dutta, M. Reno, I. Sarcevic, and D. Seckel. Propagation of muons and taus at high energies. Physical review D: Particles and fields, 63(9), 1 2001. [42] S. Jadach, J. H. Kühn, and Z. Wa̧s. Tauola a library of monte carlo programs to sim ulate decays of polarized τ leptons. Computer Physics Communications, 64(2):275 – 299, 1991. [43] F. D. Kahn and I. Lerche. Radiation from cosmic ray air showers. Proc. R. Soc. Lond. A, 289:206, 1966. [44] K. Kotera, D. Allard, and A. Olinto. Cosmogenic neutrinos: parameter space and detectabilty from PeV to ZeV. Journal of Cosmology and Astroparticle Physics, 2010(10):013–013, oct 2010. [45] K. Kotera and A. V. Olinto. The astrophysics of ultrahighenergy cosmic rays. An nual Review of Astronomy and Astrophysics, 49(1):119–153, 2011. [46] I. Kravchenko, S. Hussain, D. Seckel, D. Besson, E. Fensholt, J. Ralston, J. Taylor, K. Ratzlaff, and R. Young. Updated results from the rice experiment and future prospects for ultrahigh energy neutrino detection at the south pole. Phys. Rev. D, 85:062004, Mar 2012. [47] A. Lagutin, A. Plyasheshnikov, and A. Goncharov. The lateral distribution of the electrons in the electromagnetic air shower. Nuclear Physics B Proceedings Sup plements, 60(3):161 – 167, 1998. [48] L. Landau and I. Pomeranchuk. Electronshowers processes at ultrahigh energies. Dokl.Akad.Nauk.SSSR, 92:735–738, 1953. [49] B. L.B. and B. Eh.V. Nucleon shadowing effects in photonnucleus interactions. Yadernaya Fizika, 33(5):1195–1207, 1981. [50] J. Linsley. private communication by m.hillas, 1988. [51] W. Lohmann, R. Kopp, and R. Voss. Energy loss of muons in the energy range 110000 GeV. CERN Yellow Reports: Monographs. CERN, Geneva, 1985. [52] P. Maestro. Cosmic rays: direct measurements. Proceedings of Science(ICRC2015), 016, 2015. [53] A. B. Migdal. Bremsstrahlung and pair production in condensed media at high en ergies. Phys. Rev., 103:1811–1820, Sep 1956. [54] M. J. Mottram. A Search for UltraHigh Energy Neutrinos and CosmicRays with ANITA2. Springer, Berlin, Heidelberg, 2012. [55] J. Nam et al. Highelevation synoptic radio array for detection of upward moving airshowers, deployed in the Antarctic mountains. PoS, ICRC2019:967, 2019. [56] J. Nam and T. C. Liu. Feasibility of antenna array experiment for Earth skimming tauneutrino detection in Antarctica. PoS, ICRC2017:944, 2018. [57] K. Olive. Review of particle physics. Chinese Physics C, 38(9):090001, aug 2014. [58] A. A. Penzias and R. W. Wilson. A Measurement of Excess Antenna Temperature at 4080 Mc/s. , 142:419–421, Jul 1965. [59] B. Pontecorvo. Mesonium and antimesonium. Zh. Eksp. Teor. Fiz., 33:549–551, 1957. [60] C. Quigg, M. H. Reno, and T. P. Walker. Interactions of ultrahighenergy neutrinos. Phys. Rev. Lett., 57:774–777, Aug 1986. [61] A. RomeroWolf et al. Comprehensive analysis of anomalous ANITA events disfa vors a diffuse tauneutrino flux origin. Phys. Rev. D, 99:063011, Mar 2019. [62] O. Scholten, K. D. de Vries, and K. Werner. Coherent radiation from extensive air showers. Nucl. Instrum. Meth., A662:S80–S84, 2012. [63] H. Schoorlemmer et al. Energy and flux measurements of ultrahigh energy cosmic rays observed during the first anita flight. Astroparticle Physics, 77:32 – 43, 2016. [64] F. G. Schröder. Status of the radio technique for cosmicray induced air showers. Nuclear and Particle Physics Proceedings, 279281:190 – 197, 2016. Proceedings of the 9th Cosmic Ray International Seminar. [65] F. G. Schröder. Radio detection of cosmicray air showers and highenergy neutrinos. Progress in Particle and Nuclear Physics, 93:1 – 68, 2017. [66] T. Serebryakova, A. Goncharov, A. Lagutin, R. Raikin, and A. Misaki. Lateral dis tributions of electrons in air showers initiated by ultrahigh energy gamma quanta taking into account LPM and geomagnetic field effects. Journal of Physics: Con ference Series, 1181:012088, feb 2019. [67] M. W. E. Smith et al. The Astrophysical Multimessenger Observatory Network (AMON). Astropart. Phys., 45:56–70, 2013. [68] T. Stanev, C. Vankov, R. E. Streitmatter, R. W. Ellsworth, and T. Bowen. Develop ment of ultrahighenergy electromagnetic cascades in water and lead including the landaupomeranchukmigdal effect. Phys. Rev. D, 25:1291–1304, Mar 1982. [69] M. Tanabashi et al. Review of particle physics. Phys. Rev. D, 98:030001, Aug 2018. [70] M. Tartare, D. Lebrun, and F. m. c. Montanet. Influence of the photonuclear effect on electronneutrinoinduced electromagnetic cascades under the landaupomeranchuk migdal regime in standard rock. Phys. Rev. D, 86:033005, Aug 2012. [71] S.H. Wang et al. Status, calibration, and cosmic ray detection of ariannahcr station. PoS(ICRC2019), page 462, 2019. [72] E. Zas, F. Halzen, and T. Stanev. Electromagnetic pulses from highenergy showers: Implications for neutrino detection. Phys. Rev. D, 45:362–376, Jan 1992. [73] G. T. Zatsepin and V. A. Kuz’min. Upper Limit of the Spectrum of Cosmic Rays. Soviet Journal of Experimental and Theoretical Physics Letters, 4:78, Aug 1966. [74] 容震軒, C.H. Iong, 林貴林, and G.L. Lin. 淺穿地球之 tau 微中子模擬研究. http://hdl.handle.net/11536/55802, 2003. | |
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.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 |
文件中的檔案:
檔案 | 大小 | 格式 | |
---|---|---|---|
U0001-0107202014560600.pdf 目前未授權公開取用 | 4.9 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。