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Following the Cosmic Evolution of the Pristine Gas Pop III Star Formation and the First Galaxies
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| 자료유형 | 학위논문 |
|---|---|
| 서명/저자사항 | Following the Cosmic Evolution of the Pristine Gas Pop III Star Formation and the First Galaxies. |
| 개인저자 | Sarmento, Richard John. |
| 단체저자명 | Arizona State University. Astrophysics. |
| 발행사항 | [S.l.]: Arizona State University., 2018. |
| 발행사항 | Ann Arbor: ProQuest Dissertations & Theses, 2018. |
| 형태사항 | 155 p. |
| 기본자료 저록 | Dissertation Abstracts International 79-12B(E). Dissertation Abstract International |
| ISBN | 9780438286030 |
| 학위논문주기 | Thesis (Ph.D.)--Arizona State University, 2018. |
| 일반주기 |
Source: Dissertation Abstracts International, Volume: 79-12(E), Section: B.
Adviser: Evan Scannapieco. |
| 요약 | The formation of the firsts stars some 100-300 Myr after the Big Bang marked the end of the cosmic darks ages and created the elemental building blocks of not only rocky planets but eventually us. Understanding their formation, lifetimes, and co |
| 요약 | In this work I present an improved model for following the formation of Pop III stars, their effects on early galaxy evolution, and how we might search for them. I make use of a new subgrid model of turbulent mixing to accurately follow the time |
| 요약 | I also implement and track a new "Primordial metals" (PM) scalar that tracks the metals generated by Pop III SNe. These metals are taken up by second generation stars and likely result in a subclass of carbon-enhanced, metal-poor (CEMP) stars. |
| 일반주제명 | Astrophysics. Physics. |
| 언어 | 영어 |
| 바로가기 | 
: 이 자료의 원문은 한국교육학술정보원에서 제공합니다. |
