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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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Horizon Distortion Maps II<br />

Adjust the placement of grid points near each black hole using a<br />

horizon distortion map that connects grid coordinates x i to points<br />

in the black-hole rest frame ˜x i :<br />

˜θ A = θ A , ˜ϕ A = ϕ A ,<br />

˜r A = r A − f A (r A , θ A , ϕ A )<br />

L∑<br />

l∑<br />

l=0 m=−l<br />

λ lm<br />

A (t)Y lm (θ A , ϕ A ).<br />

Lee Lindblom (Caltech) <strong>Binary</strong> <strong>Black</strong> <strong>Hole</strong>s UW Milwaukee 10/14/2011 23 / 32

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