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 />
3PN accurate orbital dynamics, namely, r, ˙r, φ, and ˙ φ, explicitly <strong>in</strong> terms of u,<br />
n, and et us<strong>in</strong>g explicit expressions for the PN orbital elements ar, er, eφ, k,<br />
f4φ, f6φ, g4φ, g6φ, i6φ, h6φ, g4t, g6t, f4t, f6t, i6t, and h6t of the GQKR (MGS).<br />
PN orbital elements, given <strong>in</strong> terms of E and L, can easily be expressed <strong>in</strong><br />
terms of n and et with the help of the follow<strong>in</strong>g 3PN accurate relations for<br />
−2E and −2EL2 :<br />
−2E = (GMn) 2/3<br />
ξ 2<br />
5184<br />
<br />
18<br />
<br />
(1 − e 2 t )3/2<br />
1 + ξ2/3<br />
12<br />
(15 − η) + ξ4/3<br />
24<br />
− 4995 − 6075η − 450η 2 − 35η 3 +<br />
<br />
15 − 15η − η 2 +<br />
864<br />
1 − e 2 t<br />
<br />
<br />
2 2<br />
11520 − 15968η + 123π η + 2016η ,<br />
24<br />
1 − e 2 t<br />
(5 − 2η)<br />
(15 + 23η − 20η 2 ) +<br />
<br />
+<br />
BRI-IHP06-I – p.117/??