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[Ding<br />
(1983); Abe, Ichinose & Nakanishi(1987)] [See also<br />
Ruiz (1986)]:<br />
Known<br />
t H = t ,<br />
<br />
Function<br />
x H = (r − M • ) 2 + a 2 sin θ cos[φ − Φ(r)] ,<br />
<br />
y H = (r − M • ) 2 + a 2 sin θ sin[φ − Φ(r)] ,<br />
z H = (r − M • ) cos θ .<br />
x α H =0<br />
2nd Iberian Gravitational Wave Meeting [February 16th, 2012] 29
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