Table of Contents
10 Easy? Steps to Model a Black Hole
The 10 Steps
Step 0: Motivation
0: Background: Binary Black Hole Grand Challenge
0:astrophysical Sources of Gravitational Waves
0:Gravitational Wave Detectors
1: What Are Black Holes?
1:Event Horizons
1:Apparent Horizons
2:Einstein Field Equations
3: 3+1 Decomposition of Spacetime
3: ADM 3+1 Form
3:ADM 3+1 form (cont.)
3:Casual differencing
3:Description of causal differencing
3:Description of CD (continued)
4: Computational Solutions
4:Computational Solutions
4:Computational Solutions (cont.)
4:Computational Solutions (cont.)
5: Modeling Black Holes
5:Modeling Black Holes
5: Modeling black holes (picture)
5: Modeling black holes (picture)
6: The Inner Boundary
6: The Inner Boundary (cont.)
6: The inner boundary+causal differencing
6: Inner boundary + causal differencing
6: The Inner Boundary
7:Outer Boundary
7:Blended Dirchlet Outer boundary
8: Putting it together
8:Non-Moving Black Holes (Centered)
8:Non-Moving Black Holes (Centered)
8:Non-Moving Black Holes (Centered)
8:Non-Moving Black Holes (Centered)
8:Boosted Black Holes
8:Boosted Black Holes
9:Elliptic Problems
10:Computational Infrastructure
10: DAGH
10: Visualization Software (Ki, Klasky)
10: SV2 System Architecture
Major Obstacles
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Author: Scott A. Klasky
Email: gcf@npac.syr.edu
Home Page: http://www.npac.syr.edu
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