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  1. NTU Theses and Dissertations Repository
  2. 理學院
  3. 天文物理研究所
請用此 Handle URI 來引用此文件: http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/52000
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dc.contributor.advisor陳丕燊(Pisin Chen)
dc.contributor.authorChih-Ching Chenen
dc.contributor.author陳志清zh_TW
dc.date.accessioned2021-06-15T14:02:15Z-
dc.date.available2015-08-25
dc.date.copyright2015-08-25
dc.date.issued2015
dc.date.submitted2015-08-20
dc.identifier.citation[1] K. Greisen, Phys. Rev. Lett. 16 (1966) 748; G. T. Zatsepin and V. A. Kuzmin, JETP. 4 (1966) 114.
[2] R. U. Abbasi et al., Phys. Rev. Lett. 100 (2008) 101101.
[3] Yamamoto, T., International Cosmic Ray Conference 4 (2008) 335.
[4] P. Chen and K. D. Hoffman, U.S. Astronomy Decadal Survey (2010- 2020) Science White Paper (2009), arXiv:0902.3288.
[5] Askaryan, G. A., Zh. Eksp. Teor. Fiz. 41 (1961) 616 [Soviet Physics JETP 14 (1962) 441].
[6] D. Saltzberg, P. Gorham, D. Walz, et al., Phys. Rev. Lett. 86 (2001) 2802.
[7] P. W. Gorham, D. Saltzberg, R. C. Field, et al., Phys. Rev. D 72 (2005) 023002.
[8] P. Miocinovic, et al., Phys. Rev. D 74 (2006) 043002 .
[9] P. W. Gorham, et al., Phys. Rev. Lett. 99 (2007) 171101.
[10] P. W. Gorham et al., Phys. Rev. Lett. 103 (2009) 051103. 85
[11] P. W. Gorham et al., Astropart. Phys. 32 (2009) 10.
[12] K. Reil and the SalSA collaboration, proceedings for PANIC, 2005.
[13] I. Kravchenkoetal., Phys. Rev. D 73 (2006) 082002.
[14] C. W. James et al., Phys .Rev. D 81 (2010) 042003.
[15] P. W. Gorham et al., Phys. Rev. E 62 (2000) 8590-8605.
[16] Zas, E., Halzen, F., and Stanev, T., Phys. Rev. D 45 (1992) 362.
[17] J. Alvarez-Mun ̃iz, R. A. V ́azquez, and E. Zas, Phys. Rev. D 62 (2000) 063001.
[18] J. Alvarez-Mun ̃iz, E. Marqu ́es, R. A. V ́azquez, and E. Zas, Phys. Rev. D 74 (2006) 023007.
[19] L.D. Landau, I. Ya. Pomeranchuk, Dokl. Akad. Nauk SSSR 92 535 735 (1953); A.B. Migdal, Phys. Rev. 103 (1956) 1811.
[20] S. Klein , Rev. Mod. Phys. 71 (1999) 1501.
[21] V. Niess and V. Bertin Astropart. Phys. 26 (2006) 243.
[22] J. Bolmont et al., Proceedings of the 30th ICRC, July, 2007.
[23] J. Alvarez-Muniz, C. W. James, R. J. Protheroe, and E. Zas, Astropart. Phys. 4 (2009) 100.
[24] R.V. Buniy, J.P. Ralston, Phys. Rev. D 65 (2002) 016003.
[25] J. Alvarez-Mun ̃iz, R.A. Vázquez, E. Zas, Phys. Rev. D 62 (2000) 063001.
86
[26] J. Alvarez-Mun ̃iz, E. Zas, Phys. Lett. B 434 (1998) 396.
[27] S. Bevan et al., Astropart. Phys. 28 (2007) 366.
[28] J. Alvarez-Mun ̃iz, Andres Romero-Wolf, and Enrique Zas, Phys. Rev. D 81, (2010) 123009.
[29] K. S . Yee, IEEE Trans. Antennas Propagat., vol. AP-14, pp. 302-307, May 1966.
[30] R. Courant, K. Friedrichs and H. Lewy, IBM Journal, March 1967, pp. 215-234
[31] A. Taflove and S. C. Hangess: Computational Electrodynamics, The Finite-Difference Time- Domain Method, Third Edition, (Artech House, London, 2005).
[32] K. Greisen, in: Prog. of Cosmic Ray Phys., Ed. J.G. Wilson, Vol. III, (North-Holland Publ. Co., Amsterdam, 1956) p. 1; K. Kamata, J. Nishimura, Prog. Tbeor. Phys. (Kyoto) Suppl. 6 (1958) 93.
[33] Anderson, J.A., Lorenz, C.D., Travesset, A., J. Comput. Phys. 227 (10) (2008) 5342.
[34] E. Gaburov, S. Harfst, and S. Portegies Zwart., New Astron. 14 (2009) 630.
[35] Belleman, R.G., Bedorf, J., Portegies Zwart, S.F., New Astron. 13 (2008) 103.
87
[36] Hsi-Yu Schive, Yu-Chih Tsai, and Tzihong Chiueh, ApJS. 186 (2010) 457.
[37] Ting-Wai Chiu et al., PoS LAT2009:034, 2009
[38] T. Plewa, T. J. Linde and V. G. Weirs: Adaptive Mesh Refinement - Theory And Applications (Springer, 2003).
[39] Yamamoto, T. 2008, International Cosmic Ray Conference, 4, 335
[40] ANITA Collab. (P. Gorham), Phys. Rev. Lett. 103, 051103 (2009).
[41] ARA Collab. (P. Allison et al.), Astropart. Phys. 35, 457 (2012).
[42] S. W. Barwick, J. Phys. Conf. Ser. 60, 276 (2007).
[43] U. F. Katz, Nucl. Inst. Meth. 567, 457 (2006).
[44] D. Heck et al., OCORSIKA: A Monte Carlo Code to Simulate 1 Exten-
sive Air Showers, 2 Report FZKA, 6019, (1998).
[45] C.-Y. Hu, C.-C. Chen and P. Chen, Astropart. Phys. 35, 397 (2012), arxiv:1001.2543
[46] J. Alvarez-Mun ̃iz, R. A. V ́azquez, and E. Zas, Phys. Rev. D 61, 023001 (1999).
[47] Maxwell, James Clerk, “A Dynamical Theory of the Electromagnetic Field”, Philosophical Transactions of the Royal Society of London 155, 459-512 (1865).
[48] A.H. Guth, Phys. Rev. D23, 347 (1981). 88
[49] P.A.M. Dirac, Proc. Roy. Soc. London A133, 60 (1931).
[50] P.B. Price, E.K. Shirk, W.Z. Osborne, and L.S. Pinsky, Phys. Rev. Lett.
35, 487 (1975).
[51] B. Cabrera, Phys. Rev. Lett. 48, 1378 (1982).
[52] A.D. Caplin, M. Hardiman, M. Koratzinos, and J.C. Schouten, Nature 321, 402 (1986).
[53] P.B. Price, E.K. Shirk, W.Z. Osborne, and L.S. Pinsky, Phys. Rev. D18, 1382 (1978).
[54] M.E. Huber, B. Cabrera, M.A. Taber, and R.D. Gardner, Phys. Rev. Lett. 64, 835 (1990).
[55] E.N. Parker, Astrophys. J. 160, 383 (1970).
[56] M. Ambrosio et al. (MACRO Collaboration), Eur. Phys. J. C25, 511
(2002).
[57] H. Wissing, for the IceCube Collaboration, in Proceedings of the 30th
International Cosmic Ray Conference (ICRC), Merida, Mexico, 2007.
[58] V. Aynutdinov et al. (Baikal Collaboration), in Proceedings of the 29th
International Cosmic Ray Conference (ICRC), Pune, India, 2005.
[59] The flux limit from Baikal assumes an initial monopole energy of 1012 − 1015 GeV, lower than the initial energy assumed in this study. Therefore, the Baikal limit shown in Fig. 3.8 should be regarded as a function of the indicated mass but not necessarily the indicated γ.
89
[60] S. Balestra et al. (SLIM Collaboration), Eur. Phys. J. C55, 57 (2008).
[61] F.C. Adams, M. Fatuzzo, K. Freese, G. Tarl ́e, R. Watkins, and M.S. Turner, Phys. Rev. Lett. 70, 2511 (1993); astrophysical limits tabulated in [?]
[62] S.D. Wick, T.W. Kephart, T.J. Weiler, and P.L. Biermann, Astropart. Phys. 18, 663 (2003).
[63] J.D. Jackson, Classical Electrodynamics (Wiley, New York, 1962).
[64] P. W. Gorham et al. (ANITA Collaboration), Astropart. Phys. 32, 10 (2009).
[65] D.P. Hogan et al., Phys. Rev. D78, 075031 (2008).
[66] A. Vilenkin and E.P.S. Shellard, Cosmic Strings and Other Topological
Defects (Cambridge University, Cambridge, 1994).
[67] ARA Collaboration: P. Allison et. al arxiv:1507.08991
[68] K. Greisen, Phys. Rev. Lett. 16, 748 (1966); G. Zatsepin and V. Kuzmin, Pis’ma Zh. Eksp. Teor. Fiz. 4, 114 (1966); JETP Lett. 4, 78 (1966).
[69] P. W. Gorham et al. (ANITA Collaboration), Phys. Rev. Lett 103, 051103 (2009).
[70] P. W. Gorham et al. (ANITA Collaboration), Phys. Rev. D82, 022004 (2010), and erratum (arXiv:1011.5004).
[71] S. Hoover et al. (ANITA Collaboration), arXiv:1003.2961, submitted to Phys. Rev. Lett. (2010)
90
[72] S. Iyer Dutta, M.H. Reno, I. Sarcevic, and D. Seckel, Phys. Rev. D63, 094020 (2001); D. Seckel, M.H. Reno, I. Sarkevic, and S. Iyer Dutta, in Proceedings of the 27th International Cosmic Ray Conference (ICRC), Hamburg, Germany, 2001.
[73] The loss symbol β should cause no confusion with the velocity β.
[74] L. D. Landau and I. J. Pomeranchuk, Dokl. Akad. Nauk. SSSR 92, 535 (1953), 92, 735 (1953); A. B. Migdal, Phys. Rev. 103, 1811 (1956). J. Alvarez-Mun ̃iz, R.A. V ́azquez and E. Zas, Phys. Rev. D61, 023001 (1999).
[75] A.M. Dziewonski and D.L. Anderson, Phys. Earth Planet In. 25, 297 (1981).
[76] I. Kravchenko et al. (RICE Collaboration), Phys. Rev. D73, 082002 (2006).
[77] D. Saltzberg et al., Phys. Rev. Lett. 86, 2802 (2001).
[78] P. Gorham et al.Phys. Rev. D72, 023002 (2005).
[79] V. S. Beresinsky, G. T. Zatsepin, Phys. Lett. B 28, 423 (1969).
[80] ANITA Collab.: P. W. Gorham et al., Phys. Rev. Lett. 103, 051103 (2009).
[81] ANITA Collab.: P. W. Gorham et al., Astropart. Phys. 32, 10 (2009).
[82] S. Hoover et al. Phys. Rev. Lett. 105, 151101
[83] S. Barwick et al., J. Glaciol. 51, 231 (2005). 91
[84] G. A. Askaryan, JETP 14, 441 (1962); JETP 21, 658 (1965).
[85] J. Alvarez-Muniz, E. Zas, Phys. Lett. B 411, 218 (1997).
[86] D. Saltzberg et al., Phys. Rev. Lett., 86, 2802 (2001).
[87] ANITA Collab.: P. W. Gorham et al., Phys. Rev. Lett. 99, 171101 (2007).
[88] H. Schoorlemmeret al., arxiv:1506.05396
[89] R. Engel, D. Seckel, T. Stanev, Phys. Rev. D 64, 093010 (2001).
[90] A. Vieregg, UCLA Ph.D. Dissertation (2010).
[91] BEDMAP Consortium: M. B. Lythe, D. G. Vaughan et al., J. Geophys. Res. 106, B6, 11335 (2001).
[92] ANITA Collab: S. Hoover et al., To be submitted to Phys. Rev. Lett., arXiv:1005.0035.
[93] G. Feldman, R. Cousins, Phys. Rev. D 57, 3873 (1998);
[94] P. W. Gorham et al. Phys. Rev. D 82, 022004 J. Conrad, et al., Phys. Rev. D 67, 012002 (2003).
[95] M. Detrixhe et al. (ANITA Collaboration) Phys. Rev. D 83, 023513
[96] Gandhi et al., Astropart. Phys., 5, 81 (1996).
[97] L. A. Anchordoqui et al., Phys. Rev. D 66, 103002 (2002).
[98] N. Lehtinen et al., Phys. Rev. D 69, 013008 (2004).
92
[99] S. Hoover, UCLA Ph.D. Dissertation (2010).
[100] IceCube Collab.: M. Ackermann et al. Ap. J. 675, 1014 (2008).
[101] P.W. Gorhamet al. Phys. Rev. D 85, 049901(E) (2012)
[102] I. Kravchenko, et al., Phys. Rev. D 73, 082002 (2006).
[103] Pierre Auger Collab.: J. Abraham et al., Phys. Rev. Lett. 100, 211101 (2008).
[104] HiRes Collab.: R. U. Abbassi et al., Ap. J. 684, 790 (2008). [105] R. J. Protheroe, P. A. Johnson, Astropart. Phys. 4, 253 (1996). [106] O. E. Kalashev et al., Phys. Rev. D 66, 063004 (2002).
[107] O. E. Kalashev et al., Phys. Rev. D 65, 103003 (2002).
[108] C. Aramo, et al., Astropart. Phys. 23, 65 (2005).
[109] M. Ave et al., Astropart. Phys. 23, 19 (2005).
[110] V. Barger, P. Huber, D. Marfatia, Phys. Lett. B 642, 333 (2006). [111] T. Stanev et al., Phys. Rev. D 73, 043003 (2006).
[112] V. Berezinsky, arXiv: astro-ph/0509675 (2005).
[113] H. Yuksel, M. D. Kistler, Phys. Rev. D 75, 083004 (2007).
[114] S. Yoshida et al., Ap. J. 479, 547 (1997).
[115] E. Waxman, J. Bahcall, Phys. Rev. D 59, 023002 (1999).
dc.identifier.urihttp://tdr.lib.ntu.edu.tw/jspui/handle/123456789/52000-
dc.description.abstract本論文探討應用電波技術在超高能文中子的量測。第一部分研究超高能粒子所產生出的切輪可夫輻射行為,並使用有限元素法研究之。第二部分介紹ANITA實驗所利用的偵測方法、儀器設計及物理結果。第三部份介紹ARA天壇陣列實驗的偵測方法、儀器設計及物理結果。最後探討一種分辨超高能微中子味道的方法。zh_TW
dc.description.abstractIn this thesis we study the Cherenkov radiation pulse from ultra-high energy particle shower by a numerical finite-difference time-domain (FDTD) method. Expounding the work on ANITA experiment include detection method, instrument and operation method. The design concept of Askaryan Radio Array (ARA) experiment and the hardware, deploy and operation. We propose our strategy to identify the neutrino flavor in observing cosmogenic neutrinos by radio neutrino telescopes, such as ARA, ARIANNA.en
dc.description.provenanceMade available in DSpace on 2021-06-15T14:02:15Z (GMT). No. of bitstreams: 1
ntu-104-D97244002-1.pdf: 18639883 bytes, checksum: 7b11c4b22560023df60a774d09c934d4 (MD5)
Previous issue date: 2015
en
dc.description.tableofcontentsContents i
List of Figures iv
List of Tables xiv
1 Introduction 1
2 Radiation 3
2.1 CoherentCherenkovradiationpulses . . . . . . . . . . . . . . 3
2.2 Theoreticalconsiderations .................... 7
2.2.1 The one-dimensional approximation . . . . . . . . . . . 7
2.2.2 Thesqueezingeffect ................... 12
2.3 Numericalmethod ........................ 14
2.3.1 Algorithm......................... 15
2.3.2 Simulationsetup ..................... 17
2.4 Simulations ............................ 20
2.4.1 Towardsmorerealisticcases............... 20
2.5 Summary ............................. 29
3 ANITA 32
3.1 ANITAconcept.......................... 32
3.2 ANITA-IIInstrument....................... 36
3.2.1 RFantenna ........................ 37
3.2.2 Front-endsystem ..................... 37
3.2.3 SURF High Occupancy RF Trigger (SHORT) . . . . . 37
3.2.4 Trigger........................... 38
3.2.5 Digitization ........................ 38 3.2.6 Powersystemanddatatransmission . . . . . . . . . . 39
3.2.7 datatransmission..................... 39
3.3 Dataanalysis ........................... 39
3.3.1 SummaryofANITAmissionstodate . . . . . . . . . . 44
3.4 ANITA-IIresult.......................... 45
3.5 ANITA-IIasacosmicraydetector ............... 45
3.6 ANITA-IIasamonopoledetector................ 51
Askaryan Radio Array 55
4.1 TheARAStation......................... 55
4.2 Generaldesign .......................... 56
4.3 PerformanceoftheARAstationsA2andA3. . . . . . . . . . 62
4.4 The calibration of station geometry and timing . . . . . . . . 64
4.5 Signalchaincalibration...................... 68
4.6 Results............................... 72
5 Discrimination between Flavors for Detection of Cosmogenic Neutrinos 77
5.1 Thestrategyofflavoridentification ............... 77
5.2 Simulationforneutrinoevents.................. 79
5.3 Summary ............................. 84
dc.language.isoen
dc.title利用電波技術量測超高能微中子及宇宙射線zh_TW
dc.titleThe Radio Detection of Ultra High Energy Neutrinos and Cosmic Raysen
dc.typeThesis
dc.date.schoolyear103-2
dc.description.degree博士
dc.contributor.oralexamcommittee黃明輝(Ming-Huey Huang),南智佑(Jiwoo Nam),王明儒(Min-Zu Wang),蕭宇劭(Jerry Shiao),陳勁豪(John Chin-Hao Chen)
dc.subject.keyword微中子,無線電,切倫可夫輻射,計算,超高能粒子,zh_TW
dc.subject.keywordneutrino,radio frequency,Cherenkov radiation,calculation,ultra high energy particle,en
dc.relation.page93
dc.rights.note有償授權
dc.date.accepted2015-08-20
dc.contributor.author-college理學院zh_TW
dc.contributor.author-dept天文物理研究所zh_TW
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