Solving Einstein's Equations the Generalized Harmonic Way
Solving Einstein's Equations the Generalized Harmonic Way
Solving Einstein's Equations the Generalized Harmonic Way
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Constraint Damping <strong>Generalized</strong> <strong>Harmonic</strong> System<br />
Pretorius (based on a suggestion from Gundlach, et al.) modified<br />
<strong>the</strong> GH system by adding terms proportional to <strong>the</strong> gauge<br />
constraints:<br />
[<br />
0 = R ab − ∇ (a C b) + γ 0 n (a C b) − 1 2 ψ ab n c C c<br />
],<br />
where n a is a unit timelike vector field. Since C a = H a + Γ a<br />
depends only on first derivatives of <strong>the</strong> metric, <strong>the</strong>se additional<br />
terms do not change <strong>the</strong> hyperbolic structure of <strong>the</strong> system.<br />
Lee Lindblom (Caltech) GH Einstein CCRG-RIT – 10/17/2008 10 / 34