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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FZ flux - Radiative Multipoles<br />
Follow<strong>in</strong>g Thorne (1980), the expression for the 3PN<br />
accurate far zone energy flux <strong>in</strong> terms of symmetric<br />
trace-free (STF) radiative multipole moments read as<br />
dE<br />
dt<br />
<br />
far−zone<br />
= G<br />
c5 <br />
1<br />
5<br />
(1) (1)<br />
U ij U ij<br />
+ 1<br />
c2 <br />
1<br />
189<br />
+ 1<br />
c4 <br />
1<br />
9072<br />
+ 1<br />
c6 <br />
1<br />
594000<br />
<br />
+O(8) .<br />
(1) (1)<br />
U ijk U ijk<br />
+ 16<br />
45<br />
(1) (1)<br />
U ijkmU ijkm<br />
V (1)<br />
ij<br />
+ 1<br />
84<br />
(1) (1)<br />
U ijkmnU ijkmn<br />
<br />
(1)<br />
V ij<br />
V (1)<br />
ijk<br />
<br />
(1)<br />
V ijk<br />
4 (1) (1)<br />
+ V ijkmV ijkm<br />
14175<br />
<br />
BRI-IHP06-I – p.21/??
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