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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Energy Flux - Modified Harmonic Coords<br />
Logs can be removed by the follow<strong>in</strong>g shift on the particle world-l<strong>in</strong>es:<br />
ξ i 1 =<br />
22 m<br />
3<br />
2 1m2 c6 r2 ni <br />
r<br />
ln ,<br />
ξ i 2<br />
= − 22<br />
3<br />
Under shift ξ, Accn of First particle shifts by<br />
Rel Accn shifts by<br />
δξa i = − m3 ν<br />
+<br />
r 4<br />
δξa i 1 = ¨ ξ i 1 − ξ j<br />
1<br />
m1m 2 2<br />
c 6 r 2 ni ln<br />
r ′ 1<br />
r<br />
r ′ 2<br />
<br />
− ξj<br />
2 ∂ja i 1 .<br />
<br />
110 ˙r 2 − 22v 2 n i − 44 ˙rv i ln<br />
<br />
− 176<br />
3 ˙r2 + 22<br />
3 v2 − 22<br />
3<br />
m<br />
r<br />
<br />
.<br />
n i + 44<br />
3 ˙rvi<br />
Log dependence <strong>in</strong> the above transformation exactly cancels the log dependence<br />
of the acceleration <strong>in</strong> standard harmonic coord<strong>in</strong>ates. Some 3PN coefficients<br />
<strong>in</strong> the EOM are also modified and the f<strong>in</strong>al result for Accn <strong>in</strong> Modified Harm<br />
Coords. agrees with that displayed <strong>in</strong> e.g. Mora Will<br />
BRI-IHP06-I – p.33/??<br />
r<br />
<br />
r ′ 0