MARC보기
LDR02259nmm uu200409 4500
001000000330363
00520240805161321
008181129s2018 |||||||||||||||||c||eng d
020 ▼a 9780438260610
035 ▼a (MiAaPQ)AAI10843941
035 ▼a (MiAaPQ)columbia:14846
040 ▼a MiAaPQ ▼c MiAaPQ ▼d 248032
0820 ▼a 520
1001 ▼a Fernandez, Ricardo.
24513 ▼a An Object-Oriented, Python-Based Moving Mesh Hydrodynamics Code Inspired by Astrophysical Problems.
260 ▼a [S.l.] : ▼b Columbia University., ▼c 2018
260 1 ▼a Ann Arbor : ▼b ProQuest Dissertations & Theses, ▼c 2018
300 ▼a 208 p.
500 ▼a Source: Dissertation Abstracts International, Volume: 79-12(E), Section: B.
500 ▼a Adviser: Greg Bryan.
5021 ▼a Thesis (Ph.D.)--Columbia University, 2018.
520 ▼a The role of radiative cooling plays an important role in the formation of structures in collapsing gas. In this dissertation I examine the impact of cooling in two formation scenarios: first, the role of H2 cooling in collapsing gas in primordia
520 ▼a In chapter 2, I examined the proposed mechanism to explain the formation of super-massive black holes through direct collapse. The presence of quasars at redshifts z > 6 indicates the existence of supermassive black holes (SMBHs) as massive as a
520 ▼a In chapter 3, I explore the relative role of small-scale fragmentation and global collapse in low-metallicity clouds, pointing out that in such clouds the cooling time may be longer than the dynamical time, allowing the cloud to collapse globall
520 ▼a Lastly in chapter 4, I describe the structure and implementation of the new open-source parallel moving-mesh hydrodynamic code, Python Hydro-Dynamics (phd). The code has been written from the ground up to be easy to use and facilitate future mod
590 ▼a School code: 0054.
650 4 ▼a Astronomy.
690 ▼a 0606
71020 ▼a Columbia University. ▼b Astronomy.
7730 ▼t Dissertation Abstracts International ▼g 79-12B(E).
773 ▼t Dissertation Abstract International
790 ▼a 0054
791 ▼a Ph.D.
792 ▼a 2018
793 ▼a English
85640 ▼u http://www.riss.kr/pdu/ddodLink.do?id=T14999955 ▼n KERIS
980 ▼a 201812 ▼f 2019
990 ▼a 관리자