Magnetized Accretion onto Inspiraling Binary Black Holes - LUTH
Magnetized Accretion onto Inspiraling Binary Black Holes - LUTH
Magnetized Accretion onto Inspiraling Binary Black Holes - LUTH
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<strong>Accretion</strong> Rate<br />
Figure: (Left) <strong>Accretion</strong> rate through the inner boundary: RunSE (black) and<br />
RunIN (gray). (Right) Time-averaged accretion rate during four equally spaced<br />
segments from t = 30, 000M (black) till the end of RunSE.<br />
Both RunIN and RunSE accretion rate decrease over time.<br />
Decrease due largely to torques. Decrease of RunIN also due to<br />
binary orbital decoupling.<br />
Bruno C. Mundim <strong>Magnetized</strong> <strong>Accretion</strong> <strong>onto</strong> <strong>Inspiraling</strong> BBH 2013-05-23
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