簡易檢索 / 詳目顯示

研究生: 李漢昇
Li, Han-Sheng
論文名稱: 阿法質譜探測儀上, 粒子軌跡演算法以及 0.5-500 GeV 之初級宇宙射線正電子比測量
The new tracking Algorithm and Measurement of Positron Fraction with the AMS-02 Experiment
指導教授: 楊毅
Yang, Yi
學位類別: 碩士
Master
系所名稱: 理學院 - 物理學系
Department of Physics
論文出版年: 2017
畢業學年度: 105
語文別: 英文
論文頁數: 86
中文關鍵詞: Cosmic raysAMS-02Dark matterPositron fraction
外文關鍵詞: Cosmic rays, AMS-02, Dark matter, Positron fraction
相關次數: 點閱:129下載:5
分享至:
查詢本校圖書館目錄 查詢臺灣博碩士論文知識加值系統 勘誤回報
  • 阿法質譜探測儀(AMS-02)是安裝在國際太空站上的粒子物理探
    測器, AMS-02 的主要目的是解開自然界中重要的問題, 像是物質與反
    物質不對稱性以及暗物質的存在。AMS-02 從2011 年5 月開始運作, 到
    現在已經收集了超過90 億個宇宙射線事件。在這篇論文中, 我們將提
    出一個在AMS-02 上新的粒子軌跡演算法模型, 以及展示0.5 - 500 GeV
    之初級宇宙射線正電子比測量的結果, 這個結果顯示我們正在接近新物
    理的邊緣。

    The Alpha Magnetic Spectrometer (AMS-02) is a general purpose particle physics detector installed on the International Space Station. The main purpose of AMS-02 is to answer the most important questions in Nature, for example the matter-antimatter asymmetry and the origin of dark matter.
    AMS-02 detector has collected more than 90 billion cosmic rays since May 2011. In this study, we present a new tracking algorithm for AMS-02, and show the precision measurement of the positron fraction in primary cosmic rays in the energy range from 0.5 to 500 GeV. This result indicates that we are at the corner of finding new physics.

    Abstract in Chinese . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . i Abstract in English . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . ii Acknowledgements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . iii Contents . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . iv List of Tables . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . vii List of Figures . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . viii 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1 2 Theoretical review . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3 2.1 Cosmic rays . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3 2.1.1 Antimatter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5 2.2 Dark matter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6 3 AMS-02 experiment . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10 3.1 International Space Station (ISS) . . . . . . . . . . . . . . . . . . . . . . . 10 3.2 AMS-02 Detector . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11 3.2.1 Transition Radiation Detector . . . . . . . . . . . . . . . . . . . . 12 3.2.2 Permanent magnet . . . . . . . . . . . . . . . . . . . . . . . . . . 13 3.2.3 Time of Flight system . . . . . . . . . . . . . . . . . . . . . . . . 15 3.2.4 Silicon tracker . . . . . . . . . . . . . . . . . . . . . . . . . . . . 16 3.2.5 Ring Image Cherenkov detector . . . . . . . . . . . . . . . . . . . 17 3.2.6 Electromagnetic Calorimeter . . . . . . . . . . . . . . . . . . . . . 18 4 New Tracking Method . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20 4.1 Motivation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20 4.2 Magnetic and Material effects . . . . . . . . . . . . . . . . . . . . . . . . 21 4.3 Performance in Toy MC simulations . . . . . . . . . . . . . . . . . . . . . 30 4.3.1 Energy loss distribution . . . . . . . . . . . . . . . . . . . . . . . 30 4.3.2 The change of particle directions and positions . . . . . . . . . . . 32 4.4 Track model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34 4.4.1 Performance of track model . . . . . . . . . . . . . . . . . . . . . 34 5 Positron Fraction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 39 5.1 Data Sample and Selections . . . . . . . . . . . . . . . . . . . . . . . . . . 39 5.2 Selection Variables for Positron Fraction Analysis . . . . . . . . . . . . . . 42 5.3 Particle templates and Iteration Method . . . . . . . . . . . . . . . . . . . 45 5.3.1 Particle templates . . . . . . . . . . . . . . . . . . . . . . . . . . . 45 5.3.2 Iteration Method . . . . . . . . . . . . . . . . . . . . . . . . . . . 49 5.4 Charge Confusion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 53 5.5 Uncertainties . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 54 5.5.1 Statistical Uncertainty . . . . . . . . . . . . . . . . . . . . . . . . 54 5.5.2 Systematic Uncertainties . . . . . . . . . . . . . . . . . . . . . . . 54 5.6 Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 60 6 Conclusion and Future Work . . . . . . . . . . . . . . . . . . . . . . . . . . . . 68 6.1 Conclusion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 68 6.2 Future Work . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 69 6.2.1 Truth and reconstructed photon in MC . . . . . . . . . . . . . . . . 70 References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73 Appendix A The comparisons of parameters between official MC and Toy MC . . . 76 A.1 The multiple scattering parameter . . . . . . . . . . . . . . . . . . . . . . 76 A.2 The ionization energy loss parameter . . . . . . . . . . . . . . . . . . . . . 77 Appendix B Iteration method on real data . . . . . . . . . . . . . . . . . . . . . . . 78 B.1 Negative charge data . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 78 B.2 Positive charge data . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82 Appendix C Truth and reconstructed photon in MC . . . . . . . . . . . . . . . . . . 85 C.1 The difference of angle between primary and reconstructed photon . . . . . 85 C.2 The opening angle between electron and positron . . . . . . . . . . . . . . 86

    [1] H. M-H, ``Xinjiang summer program on astroparticle
    physics,' 2016. [Online]. Available: http://www.tir.tw/
    conf/xapp2016/figs/xapp2016-poster.pdf
    [2] Z. Weng, ``Particle identification using transition radiation detector and precision measurement of cosmic ray
    positron fraction with the ams-02 experiment,' 2013. [Online].
    Available: http://zweng.web.cern.ch/zweng/Thesis_ZhiliWeng_ForDefence.pdf
    [3] e. a. Cholis I, ``The pamela positron excess from annihilations into a light boson,' J. Cosmol. Astropart. Phys., 2009.
    [4] S. Ting, ``The first five years of the
    ams-02 on iss,' 2016. [Online]. Available:
    https://indico.cern.ch/event/592392/attachments/1381599/2110332/AMS-CERN-Dec-2016.pdf
    [5] ``The permanent magnet.' [Online]. Available: http://www.
    ams02.org/what-is-ams/tecnology/magnet/pmmagnet/
    [6] ``The time-of-flight.' [Online]. Available: http://www.
    ams02.org/what-is-ams/tecnology/tof/
    [7] H. D, ``The silicon tracker of ams02.' 2004.
    [8] ``The rich.' [Online]. Available: http://www.ams02.org/
    what-is-ams/tecnology/rich/
    [9] ``The eacl.' [Online]. Available: http://www.ams02.org/
    what-is-ams/tecnology/eacl/
    [10] S. Gorbunov and I. Kisel, ``Analytic formula for track extrapolation
    in non-homogeneous magnetic field,' Nuclear
    Instruments and Methods in Physics Research Section
    A, vol. 559, no. 1, pp. 148 -- 152, 2006. [Online].
    Available: http://www.sciencedirect.com/science/article/
    pii/S0168900205022588
    [11] K. Olive and P. D. Group, ``Review of particle physics,'
    Chinese Physics C, vol. 38, no. 9, p. 090001, 2014.
    [Online]. Available: http://stacks.iop.org/1674-1137/38/i=
    9/a=090001
    [12] R. Frühwirth, ``A gaussian-mixture approximation of
    the bethe–heitler model of electron energy loss by
    bremsstrahlung,' Computer Physics Communications,
    vol. 154, no. 2, pp. 131 -- 142, 2003. [Online]. Available: http://www.sciencedirect.com/science/article/pii/S0010465503002923
    [13] J. Myrheim and L. Bugge, ``A fast runge-kutta method for
    fitting tracks in a magnetic field,' Nuclear Instruments and
    Methods, vol. 160, no. 1, pp. 43 -- 48, 1979. [Online].
    Available: http://www.sciencedirect.com/science/article/
    pii/0029554X79901630
    [14] M. Mathis, ``The south atlantic anomaly and the charge
    field.'
    [15] D. F. Smart and M. A. Shea, ``A review of geomagnetic
    cutoff rigidities for earth-orbiting spacecraft.'
    [16] L. Accardo et al., ``High statistics measurement of the
    positron fraction in primary cosmic rays of 0.5-500 gev
    with the alpha magnetic spectrometer on the international
    space station,' Phys. Rev. Lett., vol. 113, p. 121101, Sep 2014. [Online]. Available: http://link.aps.org/doi/10.1103/
    PhysRevLett.113.121101

    無法下載圖示 校內:立即公開
    校外:不公開
    電子論文尚未授權公開,紙本請查館藏目錄
    QR CODE