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 />
At 1PN order, <strong>the</strong> radiative self-force is<br />
determined from a scalar <strong>and</strong> a vector radiationreaction<br />
potentials:<br />
Burke-Thorne<br />
Potential<br />
V RR (t, x) = − 1 5 xij M (5)<br />
ij (t) + 1<br />
189 xijk M (7)<br />
ijk (t)<br />
− 1 70 x2 x ij M (7)<br />
ij (t) ,<br />
V i RR (t, x) = 1 21 ˆxijk M (6)<br />
jk (t) − 4 45 ijkx jl S (5)<br />
kl (t) ,<br />
2nd Iberian Gravitational Wave Meeting [February 16th, 2012] 26
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