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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/123456789/79997
完整後設資料紀錄
DC 欄位值語言
dc.contributor.advisor闕志鴻(Tzihong Chiueh)
dc.contributor.authorYi-Hsiung hsuen
dc.contributor.author許藝薰zh_TW
dc.date.accessioned2022-11-23T09:20:18Z-
dc.date.available2021-08-10
dc.date.available2022-11-23T09:20:18Z-
dc.date.copyright2021-08-10
dc.date.issued2021
dc.date.submitted2021-07-21
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Journal of High Energy Physics, 2006(06):051–051, jun 2006. [8] Hsi-Yu Schive, Tzihong Chiueh, and Tom Broadhurst. Cosmic structure as the quantum interference of a coherent dark wave. Nature Physics, 10(7):496–499, 2014. [9] Hsi-Yu Schive, Ming-Hsuan Liao, Tak-Pong Woo, Shing-Kwong Wong, Tzihong Chiueh, Tom Broadhurst, and W-Y. Pauchy Hwang. Under- standing the core-halo relation of quantum wave dark matter from 3d simulations. Phys. Rev. Lett., 113:261302, Dec 2014. [10] David J.E. Marsh. Axion cosmology. Physics Reports, 643:1 – 79, 2016. Axion cosmology. [11] Lam Hui, Jeremiah P. Ostriker, Scott Tremaine, and Edward Witten. Ultralight scalars as cosmological dark matter. Phys. Rev. D, 95:043541, Feb 2017. [12] Jens C. Niemeyer. Small-scale structure of fuzzy and axion-like dark matter. Progress in Particle and Nuclear Physics, 113:103787, 2020. [13] Eric Armengaud, Nathalie Palanque-Delabrouille, Christophe Y`eche, David J. E. Marsh, and Julien Baur. Constraining the mass of light bosonic dark matter using SDSS Lyman-α forest. Monthly Notices of the Royal Astronomical Society, 471(4):4606–4614, 07 2017. [14] Takeshi Kobayashi, Riccardo Murgia, Andrea De Simone, Vid Irˇsiˇc, and Matteo Viel. Lyman-α constraints on ultralight scalar dark matter:Implications for the early and late universe. Phys. Rev. D, 96:123514, Dec 2017. [15] David J. E. Marsh and Jens C. Niemeyer. Strong constraints on fuzzy dark matter from ultrafaint dwarf galaxy eridanus ii. Phys. Rev. Lett., 123:051103, Jul 2019. [16] Shu-Rong Chen, Hsi-Yu Schive, and Tzihong Chiueh. Jeans analysis for dwarf spheroidal galaxies in wave dark matter. Monthly Notices of the Royal Astronomical Society, 468(2):1338–1348, 02 2017. [17] Asher Wasserman, Pieter van Dokkum, Aaron J. Romanowsky, Jean Brodie, Shany Danieli, Duncan A. Forbes, Roberto Abraham, Christo- pher Martin, Matt Matuszewski, Alexa Villaume, John Tamanas, and Stefano Profumo. Spatially resolved stellar kinematics of the ultra- diffuse galaxy dragonfly 44. II. constraints on fuzzy dark matter. The Astrophysical Journal, 885(2):155, nov 2019. [18] Hooman Davoudiasl and Peter B. Denton. Ultralight boson dark matter and event horizon telescope observations of M87∗. Phys. Rev. Lett., 123:021102, Jul 2019. [19] Ka-Hou Leong, Hsi-Yu Schive, Ui-Han Zhang, and Tzihong Chiueh. Testing extreme-axion wave-like dark matter using the BOSS Lyman- alpha forest data. Monthly Notices of the Royal Astronomical Society, 484(3):4273–4286, 01 2019. [20] T. S. Li, J. D. Simon, A. Drlica-Wagner, K. Bechtol, M. Y. Wang, J. Garc ́ıa-Bellido, J. Frieman, J. L. Marshall, D. J. James, L. Stri-gari, A. B. Pace, E. Balbinot, Y. Zhang, T. M. C. Abbott, S. Al- lam, A. Benoit-L ́evy, G. M. Bernstein, E. Bertin, D. Brooks, D. L. Burke, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, C. E. Cunha, C. B. D’Andrea, L. N. da Costa, D. L. DePoy, S. Desai, H. T. Diehl, T. F. Eifler, B. Flaugher, D. A. Goldstein, D. Gruen, R. A. Gruendl, J. Gschwend, G. Gutierrez, E. Krause, K. Kuehn, H. Lin, M. A. G. Maia, M. March, F. Menanteau, R. Miquel, A. A. Plazas, A. K. Romer, E. Sanchez, B. Santiago, M. Schubnell, I. Sevilla-Noarbe, R. C. Smith, F. Sobreira, E. Suchyta, G. Tarle, D. Thomas, D. L. Tucker, A. R. Walker, R. H. Wechsler, W. Wester, and B. Yanny and. Farthest neigh- bor: The distant milky way satellite eridanus II. The Astrophysical Journal, 838(1):8, mar 2017. [21] Hsi-Yu Schive, Tzihong Chiueh, and Tom Broadhurst. Soliton random walk and the cluster-stripping problem in ultralight dark matter. Phys. Rev. Lett., 124:201301, May 2020. [22] Tzihong Chiueh. Dynamics of multicomponent, multifield quintessence. Phys. Rev. D, 65:123502, May 2002. [23] Razieh Emami, Tom Broadhurst, George Smoot, Tzihong Chiueh, and Hoang Nhan Luu. Soliton solution for the central dark mass in 47- tuc globular cluster and implications for the axiverse. Phys. Rev. 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Relative velocity of dark matter and baryonic fluids and the formation of the first structures. Phys. Rev. D, 82:083520, Oct 2010. [31] Ben Bar-Or, Jean-Baptiste Fouvry, and Scott Tremaine. Relaxation in a fuzzy dark matter halo. The Astrophysical Journal, 871(1):28, jan 2019. [32] Ran Wang, Jeff Wagg, Chris L. Carilli, Fabian Walter, Lindley Lentati, Xiaohui Fan, Dominik A. Riechers, Frank Bertoldi, Desika Narayanan, Michael A. Strauss, Pierre Cox, Alain Omont, Karl M. Menten, Kirsten K. Knudsen, Roberto Neri, and Linhua Jiang. STAR FOR- MATION AND GAS KINEMATICS OF QUASAR HOST GALAXIES ATz∼ 6: NEW INSIGHTS FROM ALMA. The Astrophysical Journal, 773(1):44, jul 2013. [33] R. Decarli, F. Walter, B. P. Venemans, E. Ban ̃ados, F. Bertoldi, C. Car- illi, X. Fan, E. P. Farina, C. Mazzucchelli, D. Riechers, H. W. Rix, M. A. Strauss, R. Wang, and Y. Yang. Rapidly star-forming galaxies adjacent to quasars at redshifts exceeding 6. Nature, 545(7655):457–461, 2017. [34] Linhua Jiang, Nobunari Kashikawa, Shu Wang, Gregory Walth, Luis C. Ho, Zheng Cai, Eiichi Egami, Xiaohui Fan, Kei Ito, Yongming Liang, Daniel Schaerer, and Daniel P. Stark. Evidence for gn-z11 as a luminous galaxy at redshift 10.957. Nature Astronomy, 2020. [35] Hsi-Yu Schive, Tzihong Chiueh, Tom Broadhurst, and Kuan-Wei Huang. CONTRASTING GALAXY FORMATION FROM QUANTUM WAVE DARK MATTER,ψDM, WITH λCDM, USING PLANCK AND HUB- BLE DATA. The Astrophysical Journal, 818(1):89, feb 2016. [36] Tom Broadhurst, Ivan De Martino, Hoang Nhan Luu, George F. Smoot, and S.-H. Henry Tye. Ghostly galaxies as solitons of bose-einstein dark matter. Phys. Rev. D, 101:083012, Apr 2020.
dc.identifier.urihttp://tdr.lib.ntu.edu.tw/jspui/handle/123456789/79997-
dc.description.abstract本研究目的在理解雙超輕軸子宇宙的線性微擾演化。我們呈現第一個多軸子宇宙的功率譜計算。其中一個特殊結果為以較輕極端軸子與較重自由粒子所組成的情況。此宇宙組成為高紅移星系的形成提供一個可能的解釋。此外,我們的計算保留了各個微擾的速度資訊。這個資訊可以提供未來模擬一個新的方法來建立起始條件。zh_TW
dc.description.provenanceMade available in DSpace on 2022-11-23T09:20:18Z (GMT). No. of bitstreams: 1
U0001-2007202116475300.pdf: 1678170 bytes, checksum: 7112fe9a41089b485473d000851c7392 (MD5)
Previous issue date: 2021
en
dc.description.tableofcontents口試委員審定書 iii 中文摘要 v Abstract vi Chapter 1 Introduction 1 Chapter 2 Timestep Reduction Scheme 5 2.1 Axion Model 6 2.1.1 Full Evolution 6 2.1.2 Axion Background Energy 7 2.1.3 Schrödinger Equation 8 2.1.4 Matching Condition 8 2.2 Photon and Baryon 10 2.2.1 Friction Equations 10 2.2.2 Diffusion Approximation 11 2.2.3 Matching Condition 13 Chapter 3 Single Component Universe 15 3.1 Performance and Validity 15 3.2 Baryon Acoustic Oscillation and Velocity Potential 19 Chapter 4 Two-component Axion Universe 24 Chapter 5 Conclusions 30 Chapter 6 Appendix: Long-wave Issue 32 Bibliography 34
dc.language.isoen
dc.subject波暗物質zh_TW
dc.subject暗物質zh_TW
dc.subjectdark matteren
dc.subjectwave dark matter.en
dc.title雙超輕軸子宇宙的微擾演化及功率譜zh_TW
dc.titleEvolution of perturbation and power spectrum in a two-component ultralight axionic universeen
dc.date.schoolyear109-2
dc.description.degree碩士
dc.contributor.author-orcid0000-0002-4882-8929
dc.contributor.oralexamcommittee薛熙于(Hsin-Tsai Liu),吳建宏(Chih-Yang Tseng)
dc.subject.keyword暗物質,波暗物質,zh_TW
dc.subject.keyworddark matter,wave dark matter.,en
dc.relation.page39
dc.identifier.doi10.6342/NTU202101602
dc.rights.note同意授權(全球公開)
dc.date.accepted2021-07-22
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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