| LDR | | 00000nmm u2200205 4500 |
| 001 | | 000000331116 |
| 005 | | 20241108153303 |
| 008 | | 181129s2018 ||| | | | eng d |
| 020 | |
▼a 9780438286030 |
| 035 | |
▼a (MiAaPQ)AAI10837925 |
| 035 | |
▼a (MiAaPQ)asu:18106 |
| 040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 248032 |
| 049 | 1 |
▼f DP |
| 082 | 0 |
▼a 523 |
| 100 | 1 |
▼a Sarmento, Richard John. |
| 245 | 10 |
▼a Following the Cosmic Evolution of the Pristine Gas Pop III Star Formation and the First Galaxies. |
| 260 | |
▼a [S.l.] :
▼b Arizona State University.,
▼c 2018 |
| 260 | 1 |
▼a Ann Arbor :
▼b ProQuest Dissertations & Theses,
▼c 2018 |
| 300 | |
▼a 155 p. |
| 500 | |
▼a Source: Dissertation Abstracts International, Volume: 79-12(E), Section: B. |
| 500 | |
▼a Adviser: Evan Scannapieco. |
| 502 | 1 |
▼a Thesis (Ph.D.)--Arizona State University, 2018. |
| 520 | |
▼a 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 |
| 520 | |
▼a 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 |
| 520 | |
▼a 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. |
| 590 | |
▼a School code: 0010. |
| 650 | 4 |
▼a Astrophysics. |
| 650 | 4 |
▼a Physics. |
| 690 | |
▼a 0596 |
| 690 | |
▼a 0605 |
| 710 | 20 |
▼a Arizona State University.
▼b Astrophysics. |
| 773 | 0 |
▼t Dissertation Abstracts International
▼g 79-12B(E). |
| 773 | |
▼t Dissertation Abstract International |
| 790 | |
▼a 0010 |
| 791 | |
▼a Ph.D. |
| 792 | |
▼a 2018 |
| 793 | |
▼a English |
| 856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T14999595
▼n KERIS |
| 980 | |
▼a 201812
▼f 2019 |
| 990 | |
▼a 관리자
▼b 관리자 |