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 />
Radiative Self-From from post-Minkowskian<br />
approximation + Asymptotic matched expansions<br />
[Blanchet & Damour (1984); Iyer & Will (1995);<br />
Blanchet (1997)]<br />
2nd Iberian Gravitational Wave Meeting [February 16th, 2012] 24
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