Gravitational Waves from Inspiralling Compact Binaries in ... - LUTH
Gravitational Waves from Inspiralling Compact Binaries in ... - LUTH
Gravitational Waves from Inspiralling Compact Binaries in ... - LUTH
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Complete 3PN energy flux - Mhar<br />
At long last, one can write down the complete 3PN GW<br />
energy flux averaged over an orbit for an ICB mov<strong>in</strong>g <strong>in</strong> an<br />
elliptical orbit by summ<strong>in</strong>g up the averaged <strong>in</strong>stantaneous<br />
contribution and the tail contribution<br />
< ˙<br />
E >MHar = 32ν2 x 5<br />
5<br />
1<br />
(1 − e 2 t ) 7/2<br />
<br />
< ˙<br />
EN >MHar +x < ˙<br />
E1P N >MHar<br />
+x 3/2 < E˙ 3/2P N >MHar +x 2 < E2P<br />
˙<br />
N >MHar<br />
+x 5/2 < ˙<br />
E 5/2P N >MHar +x 3 < ˙<br />
E3P N >MHar<br />
<br />
.<br />
BRI-IHP06-I – p.61/??
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