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 />
Kerr geodesics +Harmonic Coordinates: An<br />
alternative to this is to use Asymptotically Cartesian<br />
<strong>and</strong> <strong>Mass</strong> Centered coordinates (ACMC) [Thorne<br />
(1980)]<br />
This may be a convenient path to deal with <strong>the</strong> case<br />
in which <strong>the</strong> massive object is not described by <strong>the</strong><br />
Kerr metric.<br />
2nd Iberian Gravitational Wave Meeting [February 16th, 2012] 30
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