請用此 Handle URI 來引用此文件:
http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/21670
完整後設資料紀錄
DC 欄位 | 值 | 語言 |
---|---|---|
dc.contributor.advisor | 朱有花(You-Hua Chu) | |
dc.contributor.author | Li-Hsin Chen | en |
dc.contributor.author | 陳立馨 | zh_TW |
dc.date.accessioned | 2021-06-08T03:41:55Z | - |
dc.date.copyright | 2019-07-04 | |
dc.date.issued | 2019 | |
dc.date.submitted | 2019-06-24 | |
dc.identifier.citation | V. Bromm and N. Yoshida. The First Galaxies. ARA&A, 49:373–407, September 2011. . V. Bromm, P. S. Coppi, and R. B. Larson. The Formation of the First Stars. I. The Primordial Star-forming Cloud. ApJ, 564:23–51, January 2002. .
N. Yoshida, T. Abel, L. Hernquist, and N. Sugiyama. Simulations of Early Structure Formation: Primordial Gas Clouds. ApJ, 592:645–663, August 2003. . T. Abel, G. L. Bryan, and M. L. Norman. The Formation of the First Star in the Universe. Science, 295:93–98, January 2002. . J. H. Wise and T. Abel. Suppression of H2 Cooling in the Ultraviolet Background. ApJ, 671:1559–1567, December 2007. . A. Stacy, T. H. Greif, and V. Bromm. The first stars: mass growth under protostellar feedback. MNRAS, 422:290–309, May 2012. . S. Hirano, T. Hosokawa, N. Yoshida, K. Omukai, and H. W. Yorke. Primordial star formation under the influence of far ultraviolet radiation: 1540 cosmological haloes and the stellar mass distribution. MNRAS, 448:568–587, March 2015. . V. Bromm and R. B. Larson. The First Stars. ARA&A, 42:79–118, September 2004. . P. C. Clark, S. C. O. Glover, R. S. Klessen, and V. Bromm. Gravitational Fragmentation in Turbulent Primordial Gas and the Initial Mass Function of Population III Stars. ApJ, 727:110, February 2011. . T. H. Greif, V. Springel, S. D. M. White, S. C. O. Glover, P. C. Clark, R. J. Smith, R. S. Klessen, and V. Bromm. Simulations on a Moving Mesh: The Clustered Formation of Population III Protostars. ApJ, 737:75, August 2011. . T. Hosokawa, K. Omukai, N. Yoshida, and H. W. Yorke. Protostellar Feedback Halts the Growth of the First Stars in the Universe. Science, 334:1250, December 2011. . A. Stacy and V. Bromm. Constraining the statistics of Population III binaries. MNRAS, 433:1094–1107, August 2013. . H. Susa. The Mass of the First Stars. ApJ, 773:185, August 2013. . H. Susa, K. Hasegawa, and N. Tominaga. The Mass Spectrum of the First Stars. ApJ, 792: 32, September 2014. . S. Hirano, T. Hosokawa, N. Yoshida, H. Umeda, K. Omukai, G. Chiaki, and H. W. Yorke. One Hundred First Stars: Protostellar Evolution and the Final Masses. ApJ, 781:60, February 2014. . T. Hosokawa, S. Hirano, R. Kuiper, H. W. Yorke, K. Omukai, and N. Yoshida. Formation of Massive Primordial Stars: Intermittent UV Feedback with Episodic Mass Accretion. ApJ, 824:119, June 2016. . A. Stacy, V. Bromm, and A. T. Lee. Building up the Population III initial mass function from cosmological initial conditions. MNRAS, 462:1307–1328, October 2016. . A. Heger and S. E. Woosley. The Nucleosynthetic Signature of Population III. ApJ, 567: 532–543, March 2002. . A. Heger and S. E. Woosley. Nucleosynthesis and Evolution of Massive Metal-free Stars. ApJ, 724:341–373, November 2010. . K.-J. Chen, A. Heger, S. Woosley, A. Almgren, and D. J. Whalen. Pair Instability Super- novae of Very Massive Population III Stars. ApJ, 792:44, September 2014. . J. H. Wise, M. J. Turk, M. L. Norman, and T. Abel. The Birth of a Galaxy: Primordial Metal Enrichment and Stellar Populations. ApJ, 745:50, January 2012. . P. F. Hopkins, D. Kereš, J. Oñorbe, C.-A. Faucher-Giguère, E. Quataert, N. Murray, and J. S. Bullock. Galaxies on FIRE (Feedback In Realistic Environments): stellar feedback explains cosmologically inefficient star formation. MNRAS, 445:581–603, November 2014. . M. Jeon, A. H. Pawlik, V. Bromm, and M. Milosavljević. Radiative feedback from high-mass X-ray binaries on the formation of the first galaxies and early reionization. MN- RAS, 440:3778–3796, June 2014. . B. D. Smith, J. H. Wise, B. W. O’Shea, M. L. Norman, and S. Khochfar. The first Population II stars formed in externally enriched mini-haloes. MNRAS, 452:2822–2836, September 2015. . M. Jeon and V. Bromm. Signature of the first galaxies in JWST deep field observations. MNRAS, 485:5939–5950, June 2019. . G. L. Bryan, M. L. Norman, B. W. O’Shea, T. Abel, J. H. Wise, M. J. Turk, D. R. Reynolds, D. C. Collins, P. Wang, S. W. Skillman, B. Smith, R. P. Harkness, J. Bordner, J.-h. Kim, M. Kuhlen, H. Xu, N. Goldbaum, C. Hummels, A. G. Kritsuk, E. Tasker, S. Skory, C. M. Simpson, O. Hahn, J. S. Oishi, G. C. So, F. Zhao, R. Cen, Y. Li, and Enzo Collaboration. ENZO: An Adaptive Mesh Refinement Code for Astrophysics. ApJS, 211:19, April 2014. . P. Colella and P. R. Woodward. The Piecewise Parabolic Method (PPM) for Gas- Dynamical Simulations. Journal of Computational Physics, 54:174–201, September 1984. . E. F. Toro, M. Spruce, and W. Speares. Restoration of the contact surface in the HLL- Riemann solver. Shock Waves, 4:25–34, July 1994. . T. Abel, P. Anninos, Y. Zhang, and M. L. Norman. Modeling primordial gas in numerical cosmology. Nature, 2:181–207, August 1997. . P. Anninos, Y. Zhang, T. Abel, and M. L. Norman. Cosmological hydrodynamics with multi-species chemistry and nonequilibrium ionization and cooling. Nature, 2:209– 224, August 1997. . S. C. O. Glover and T. Abel. Uncertainties in H2 and HD chemistry and cooling and their role in early structure formation. MNRAS, 388:1627–1651, August 2008. . S. C. O. Glover and A.-K. Jappsen. Star Formation at Very Low Metallicity. I. Chemistry and Cooling at Low Densities. ApJ, 666:1–19, September 2007. . M. L. Norman. Pop III Stellar Masses and IMF. In D. J. Whalen, V. Bromm, and N. Yoshida, editors, American Institute of Physics Conference Series, volume 1294 of American Institute of Physics Conference Series, pages 17–27, November 2010. . J. H. Wise, M. J. Turk, and T. Abel. Resolving the Formation of Protogalaxies. II. Central Gravitational Collapse. ApJ, 682:745–757, August 2008. . R. Cen and J. P. Ostriker. Galaxy formation and physical bias. ApJL, 399:L113–L116, November 1992. . T. Abel and B. D. Wandelt. Adaptive ray tracing for radiative transfer around point sources. MNRAS, 330:L53–L56, March 2002. . J. H. Wise and T. Abel. ENZO+MORAY: radiation hydrodynamics adaptive mesh refinement simulations with adaptive ray tracing. MNRAS, 414:3458–3491, July 2011. . J. S. Vink, A. de Koter, and H. J. G. L. M. Lamers. Mass-loss predictions for O and B stars as a function of metallicity. A&A, 369:574–588, April 2001. . N. Smith. Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars. ARA&A, 52:487–528, August 2014. . J. F. Navarro, C. S. Frenk, and S. D. M. White. The Structure of Cold Dark Matter Halos. ApJ, 462:563, May 1996. . K.-J. Chen, V. Bromm, A. Heger, M. Jeon, and S. Woosley. Cosmological Impact of Population III Binaries. ApJ, 802:13, March 2015. . S. E. Woosley, A. Heger, and T. A. Weaver. The evolution and explosion of massive stars. Reviews of Modern Physics, 74:1015–1071, November 2002. . E. E. Salpeter. The Luminosity Function and Stellar Evolution. ApJ, 121:161, January 1955. . L. Corlies, K. V. Johnston, and J. H. Wise. Exploring simulated early star formation in the context of the ultrafaint dwarf galaxies. MNRAS, 475:4868–4880, April 2018. . J. A. Turner, S. J. Chapman, A. S. Bhattal, M. J. Disney, H. Pongracic, and A. P. Whit- worth. Binary star formation: gravitational fragmentation followed by capture. MNRAS, 277:705–726, November 1995. . M. J. Turk, T. Abel, and B. O’Shea. The Formation of Population III Binaries from Cos- mological Initial Conditions. Science, 325:601, July 2009. . S. S. R. Offner, K. M. Kratter, C. D. Matzner, M. R. Krumholz, and R. I. Klein. The Formation of Low-mass Binary Star Systems Via Turbulent Fragmentation. ApJ, 725: 1485–1494, December 2010. . A. Stacy, T. H. Greif, and V. Bromm. The first stars: formation of binaries and small multiple systems. MNRAS, 403:45–60, March 2010. . B. Reipurth and S. Mikkola. Formation of the widest binary stars from dynamical unfolding of triple systems. Nature, 492:221–224, December 2012. . URL https: //doi.org/10.1038/nature11662. Michael Ireland, Christoph Federrath, and Rajika L. Kuruwita. Binary star formation and the outflows from their discs. Monthly Notices of the Royal Astronomical Society, 470 (2):1626–1641, 05 2017. ISSN 0035-8711. . URL https://doi.org/10.1093/mnras/ stx1299. H. Sana, S. E. de Mink, A. de Koter, N. Langer, C. J. Evans, M. Gieles, E. Gosset, R. G. Izzard, J.-B. Le Bouquin, and F. R. N. Schneider. Binary Interaction Dominates the Evolution of Massive Stars. Science, 337:444, July 2012. . Beers, T. C. and Christlieb, N. The Discovery and Analysis of Very Metal-Poor Stars in the Galaxy. ARA&A, 43:531–580, September 2005. . A. Frebel. Stellar archaeology: Exploring the Universe with metal-poor stars. Astronomis- che Nachrichten, 331:474–488, May 2010. . T. Hartwig, V. Bromm, R. S. Klessen, and S. C. O. Glover. Constraining the primordial initial mass function with stellar archaeology. MNRAS, 447:3892–3908, March 2015. . K.-J. Chen, D. J. Whalen, K. M. J. Wollenberg, S. C. O. Glover, and R. S. Klessen. How the First Stars Regulated Star Formation. II. Enrichment by Nearby Supernovae. ApJ, 844:111, August 2017a. . K.-J. Chen, A. Heger, D. J. Whalen, T. J. Moriya, V. Bromm, and S. E. Woosley. Low- energy Population III supernovae and the origin of extremely metal-poor stars. MNRAS, 467:4731–4738, June 2017b. . M. N. Ishigaki, N. Tominaga, C. Kobayashi, and K. Nomoto. The Initial Mass Function of the First Stars Inferred from Extremely Metal-poor Stars. ApJ, 857:46, April 2018. . T. Hartwig, N. Yoshida, M. Magg, A. Frebel, S. C. O. Glover, F. A. Gómez, B. Griffen, M. N. Ishigaki, A. P. Ji, R. S. Klessen, B. W. O’Shea, and N. Tominaga. Descendants of the first stars: the distinct chemical signature of second-generation stars. MNRAS, 478:1795–1810, August 2018. . T. Hartwig, M. N. Ishigaki, R. S. Klessen, and N. Yoshida. Fingerprint of the first stars: multi-enriched extremely metal-poor stars in the TOPoS survey. MNRAS, 482:1204– 1210, January 2019. . | |
dc.identifier.uri | http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/21670 | - |
dc.description.abstract | 近代宇宙學模擬成功地呈現了暗物質暈的階級制聚集過程,提供 了足夠的重力位能井,使原始氣體(未受金屬污染的氣體)生成恆星 及星系的形成。宇宙中最重要的天體之一——第一代星系,容納了第 一批恆星在其中,此類星系被視為早期宇宙的基石。為了了解第一代 星系的形成,我們先建立了較簡單的模型,根據不同的第一代恆星質 量分佈,設置了第一代超新星殘骸的初始溫度、密度、金屬比率,及 數量在模擬中。我們設法理解第三類超新星殘骸的聚集過程,以了解 下一代恆星生成的過程。我們根據不同的暗物質暈及不同第三類超新 星殘骸組成建立了十八組模型。從我們的結果發現,在第一代星系中 橫有可能有第三類恆星的生成,這些恆星會產生額外的金屬,並改 變下一代恆星的生成。下一代(第二類)恆星的質量分布可由指數函 數來描述,在十八組模型中,指數 α 的範圍大約落在 1.37-4.76 之間 (Salpeter IMF 的 α = 2.35)。因此,我們的結果提供了一條途徑,來了 解第一代恆星及第一代星系之間的關聯,而第一代星系未來將有可能 被詹姆士偉伯望遠鏡所觀測到。 | zh_TW |
dc.description.abstract | Modern cosmological simulations successfully demonstrate that the hierarchical assembly of dark matter halos provided the gravitational wells that nurse the primordial gases to form the first stars and galaxies inside them. One of the most significant objects in the universe, the first galaxies, are naturally regarded as the foundation of the early Universe. To examine the effect of Pop III supernova remnants (SNRs) to the first galaxy formation, we perform
high-resolution hydro simulations by considering initial Pop III SNRs from different Pop III initial mass functions (IMFs). We follow the mergers of Pop III SNRs with the primordial gas and study the consequent star formation in the first galaxies. We construct 18 models with different halo properties and Pop III SNR compositions. Our results suggest that it is still possible to form Pop III stars inside the first galaxies after the first supernovae, which inject extra metals and change the subsequent Pop II star formation history. We also find that Pop II stellar mass function in our simulated galaxies can be described by power-laws, dN/dM_star ∝ M_star^α, where the exponent α falls in a wide range of 1.37 – 4.76 (α = 2.35 for the Salpeter IMF). The mass distribution is highly sensitive to the previous Pop III supernovae and the properties of the host halos. Our study can provide a channel to correlate the populations of the first stars and supernovae to star formation inside these first galaxies which may be soon observed by the James Webb Space Telescope. | en |
dc.description.provenance | Made available in DSpace on 2021-06-08T03:41:55Z (GMT). No. of bitstreams: 1 ntu-108-R06244001-1.pdf: 6485577 bytes, checksum: e326ede33bc4d263151c062909ec1b5b (MD5) Previous issue date: 2019 | en |
dc.description.tableofcontents | Contents
誌謝 iii Acknowledgements v 摘要 vii Abstract ix 1 Introduction 1 2 Methods 3 2.1 Star Formation................................ 3 2.1.1 Population III Star Formation ................... 4 2.1.2 Population II Star Formation.................... 5 2.2 Stellar Feedback............................... 6 2.3 Numerical Setup .............................. 6 3 Galaxy Initial Condition 9 4 Results 13 4.1 Gas Dynamics................................ 13 4.2 Star Formation In The First Galaxies.............. 17 5 Discussion 27 5.1 Radial Metallicity Profile.......................... 27 5.2 Parameter Choice Dependence ....................... 27 5.3 Comparison With Previous Works ..................... 30 5.4 Application And Model Refinement .................... 31 6 Conclusion 33 Bibliography 35 | |
dc.language.iso | en | |
dc.title | 第三類超新星殘骸對第一代星系的形成的影響 I. 氣體、 金屬及恆星 | zh_TW |
dc.title | Population III Supernova Remnants on The Formation of The First Galaxies I. Gas, Metals, and Stars | en |
dc.type | Thesis | |
dc.date.schoolyear | 107-2 | |
dc.description.degree | 碩士 | |
dc.contributor.coadvisor | 陳科榮(Ke-Jung Chen) | |
dc.contributor.oralexamcommittee | 平下博之(Hiroyuki Hirashita) | |
dc.subject.keyword | (宇宙學:) 早期宇宙,星系:矮,星系:形成,流體動力學,方法:數值,恆星:第三類, | zh_TW |
dc.subject.keyword | (cosmology:) early universe,galaxies: dwarf,galaxies: formation,hydrodynamics,methods: numerical,stars: Population III, | en |
dc.relation.page | 40 | |
dc.identifier.doi | 10.6342/NTU201900921 | |
dc.rights.note | 未授權 | |
dc.date.accepted | 2019-06-24 | |
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 | |
---|---|---|---|
ntu-108-1.pdf 目前未授權公開取用 | 6.33 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。