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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Modeling <strong>of</strong> IMRI/EMRIs<br />
Whereas BH + IMBH systems will be practically circular,<br />
eccentricity may play an important role in IMBH+MBH<br />
systems.<br />
Some very good news (K is <strong>the</strong> periastron advance):<br />
The PN <strong>and</strong> EOB results<br />
are valid at 3PN order.<br />
The shaded area marks<br />
<strong>the</strong> error margin <strong>of</strong><br />
<strong>the</strong> NR data.<br />
[Le Tiec et al. PRL 107, 141101(2011)]<br />
2nd Iberian Gravitational Wave Meeting [February 16th, 2012] 18