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Solving Einstein's Equations for Binary Black Hole Spacetimes

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Constraint Damping in Electromagnetism<br />

Electromagnetism is described as the hyperbolic evolution<br />

equation ∇ a ∇ a A b = ∇ b H.<br />

Where have the usual ⃗ ∇ · ⃗E = ⃗ ∇ · ⃗B = 0 constraints gone?<br />

Lee Lindblom (Caltech) <strong>Binary</strong> <strong>Black</strong> <strong>Hole</strong>s UW Milwaukee 10/14/2011 11 / 32

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