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Solving Einstein's Equations for Binary Black Hole Spacetimes

Solving Einstein's Equations for Binary Black Hole Spacetimes

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Comparing Different Numerical Methods<br />

Wave propagation with second-order finite difference method:<br />

3.0<br />

3.0<br />

3.0<br />

N=200<br />

N=200<br />

N=200<br />

2.5<br />

t=0.0<br />

2.5<br />

t=100.0<br />

2.5<br />

t=200.0<br />

2.0<br />

2.0<br />

2.0<br />

U(x,t)<br />

1.5<br />

U(x,t)<br />

1.5<br />

U(x,t)<br />

1.5<br />

1.0<br />

1.0<br />

1.0<br />

0.5<br />

0.5<br />

0.5<br />

0.0<br />

0 π/2 π 3π/2 2π<br />

x<br />

0.0<br />

0 π/2 π 3π/2 2π<br />

x<br />

0.0<br />

0 π/2 π 3π/2 2π<br />

x<br />

Figures from Hesthaven, Gottlieb, & Gottlieb (2007).<br />

Lee Lindblom (Caltech) <strong>Binary</strong> <strong>Black</strong> <strong>Hole</strong>s UW Milwaukee 10/14/2011 19 / 32

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