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 +<br />
Harmonic Coordinates<br />
Radiative Self-Force<br />
from post-Minkowskian<br />
approximation + Asymptotic<br />
matched expansions.<br />
Multipolar Expansion<br />
<strong>of</strong> <strong>the</strong> Gravitational<br />
Waveforms<br />
2nd Iberian Gravitational Wave Meeting [February 16th, 2012] 23
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