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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 />

These systems, given that <strong>the</strong>y are defined by mass ratios<br />

beyond 1:100, necessarily must involve Black Holes (BHs).<br />

2nd Iberian Gravitational Wave Meeting [February 16th, 2012] 4

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