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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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/??