東華大學圖書館 |

Language: English

Help

回圖書館首頁

手機版館藏查詢

Back

Switch To: Labeled | MARC Mode | ISBD

Development and application of numer...

White, Christopher Joseph.

Linked to FindBook

Google Book

Amazon

博客來

Development and application of numerical techniques for general-relativistic magnetohydrodynamics simulations of black hole accretion.

Record Type:	Electronic resources : Monograph/item
Title/Author:	Development and application of numerical techniques for general-relativistic magnetohydrodynamics simulations of black hole accretion./
Author:	White, Christopher Joseph.
Published:	Ann Arbor : ProQuest Dissertations & Theses, : 2016,
Description:	160 p.
Notes:	Source: Dissertation Abstracts International, Volume: 78-04(E), Section: B.
Contained By:	Dissertation Abstracts International78-04B(E).
Subject:	Astrophysics. -
Online resource:	http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=10167562
ISBN:	9781369219104

Development and application of numerical techniques for general-relativistic magnetohydrodynamics simulations of black hole accretion.
White, Christopher Joseph.

Development and application of numerical techniques for general-relativistic magnetohydrodynamics simulations of black hole accretion. - Ann Arbor : ProQuest Dissertations & Theses, 2016 - 160 p.

Source: Dissertation Abstracts International, Volume: 78-04(E), Section: B.

Thesis (Ph.D.)--Princeton University, 2016.

We describe the implementation of sophisticated numerical techniques for general-relativistic magnetohydrodynamics simulations in the Athena++ code framework. Improvements over many existing codes include the use of advanced Riemann solvers and of staggered-mesh constrained transport. Combined with considerations for computational performance and parallel scalability, these allow us to investigate black hole accretion flows with unprecedented accuracy. The capability of the code is demonstrated by exploring magnetically arrested disks.

ISBN: 9781369219104Subjects--Topical Terms:

535904
Astrophysics.

Development and application of numerical techniques for general-relativistic magnetohydrodynamics simulations of black hole accretion.
LDR:01506nmm a2200289 4500 001 2122500
005 20170922124921.5
008 180830s2016 ||||||||||||||||| ||eng d
020 $a 9781369219104
035 $a (MiAaPQ)AAI10167562
035 $a AAI10167562
040 $a MiAaPQ $c MiAaPQ
100 1 $a White, Christopher Joseph. $3 3284471
245 1 0 $a Development and application of numerical techniques for general-relativistic magnetohydrodynamics simulations of black hole accretion.
260 1 $a Ann Arbor : $b ProQuest Dissertations & Theses, $c 2016
300 $a 160 p.
500 $a Source: Dissertation Abstracts International, Volume: 78-04(E), Section: B.
500 $a Adviser: James M. Stone.
502 $a Thesis (Ph.D.)--Princeton University, 2016.
520 $a We describe the implementation of sophisticated numerical techniques for general-relativistic magnetohydrodynamics simulations in the Athena++ code framework. Improvements over many existing codes include the use of advanced Riemann solvers and of staggered-mesh constrained transport. Combined with considerations for computational performance and parallel scalability, these allow us to investigate black hole accretion flows with unprecedented accuracy. The capability of the code is demonstrated by exploring magnetically arrested disks.
590 $a School code: 0181.
650 4 $a Astrophysics. $3 535904
650 4 $a Theoretical physics. $3 2144760
690 $a 0596
690 $a 0753
710 2 $a Princeton University. $b Astrophysical Sciences. $3 3193121
773 0 $t Dissertation Abstracts International $g 78-04B(E).
790 $a 0181
791 $a Ph.D.
792 $a 2016
793 $a English
856 4 0 $u http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=10167562