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 />
Multipolar Expansion <strong>of</strong> <strong>the</strong> Gravitational<br />
Waveforms [Thorne (1980)]<br />
h TT<br />
ij = 4 r<br />
∞<br />
=2<br />
1<br />
! M() ijI −2<br />
(t − r)N I−2<br />
+<br />
<br />
2<br />
TT<br />
( + 1)! ε kl(i J() (t − r)n<br />
j)kI −1 l N I−2<br />
Here, we also use harmonic coordinates.<br />
2nd Iberian Gravitational Wave Meeting [February 16th, 2012] 31
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