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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 />

<strong>Intermediate</strong>- <strong>and</strong> <strong>Extreme</strong> mass ratio inspirals (IMRIs <strong>and</strong><br />

EMRIs) are binary systems whose evolution is driven by<br />

Gravitational-Wave (GW) emission <strong>and</strong> such <strong>the</strong> mass ratio<br />

between <strong>the</strong>ir components is in <strong>the</strong> range:<br />

q = m ∗<br />

M •<br />

=<br />

∼ 10 −7 − 10 −4<br />

∼ 10 −4 − 10 −2<br />

for EMRIs<br />

for IMRIs<br />

2nd Iberian Gravitational Wave Meeting [February 16th, 2012] 3

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