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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Introduction to IMRIs <strong>and</strong> EMRIs<br />
Astrophysical Mechanisms for IMRIs:<br />
Dense clusters <strong>of</strong> stars -> Runaway Collisions <strong>and</strong> IMBH<br />
formation. IMRIs come from capture <strong>of</strong> stellar objects.<br />
Gravitational collapse <strong>of</strong> Population III stars at <strong>the</strong> early<br />
universe to form IMBHs.<br />
2nd Iberian Gravitational Wave Meeting [February 16th, 2012] 11
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