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Gravitational Waves from Inspiralling Compact Binaries in ... - LUTH

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3PN accurate conservative dynamics<br />

The angular motion, described <strong>in</strong> terms of φ and ˙ φ, is given by<br />

φ(λ, l) = λ + W (l) ,<br />

λ = (1 + k)l ,<br />

k = 3ξ2/3<br />

1 − e2 ξ<br />

+<br />

t<br />

4/3<br />

4(1 − e2 t )2<br />

<br />

2<br />

78 − 28η + (51 − 26η)et +<br />

ξ2 128(1 − e2 t )3<br />

<br />

18240 − 25376η + 492π 2 η + 896η 2 +<br />

(28128 − 27840η + 123π 2 η + 5120η 2 )e 2 t + (2496 − 1760η + 1040η 2 )e 4 t<br />

+ 1920 − 768η + (3840 − 1536η)e 2 <br />

t 1 − e2 t ,<br />

W (l) = WN + W1PN + W2PN + W3PN ,<br />

WN = v − u + et s<strong>in</strong> u ,<br />

W1PN = 3ξ2/3<br />

1 − e 2 t<br />

(v − u + et s<strong>in</strong> u) ,<br />

BRI-IHP06-I – p.122/??

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