On the modeling of Intermediate- and Extreme-Mass-Ratio Inspirals
On the modeling of Intermediate- and Extreme-Mass-Ratio Inspirals
On the modeling of Intermediate- and Extreme-Mass-Ratio Inspirals
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A new Method: The Chimera Scheme<br />
The “local” radiative self-force has two pieces:<br />
(i) Gradients <strong>of</strong> <strong>the</strong> potentials [this implies we need<br />
up to eight-order time derivatives <strong>of</strong> <strong>the</strong> trajectory].<br />
(ii) Interaction terms <strong>of</strong> <strong>the</strong> radiative potentials with<br />
<strong>the</strong> near-zone potentials (Kerr gravitational field).<br />
2nd Iberian Gravitational Wave Meeting [February 16th, 2012] 28
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