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

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Log terms <strong>in</strong> total energy flux<br />

At the lowest Newtonian order Uij reduces to the second<br />

time derivative of Iij, and where the dots <strong>in</strong>dicate all the<br />

terms which do not depend on r0.<br />

Trivial to deduce that the correspond<strong>in</strong>g dependence of the<br />

tail part of the energy flux on r0 is given by<br />

Ftail = · · · − 428<br />

525 M 2 〈I (4)<br />

ij I(4)<br />

ij 〉 ln r0 + · · · ,<br />

where <strong>in</strong>side the time average operation 〈〉 one can freely<br />

operate by parts the time derivatives. Hence,<br />

〈I (3)<br />

ij I(5) ij 〉 = −〈I(4) ij I(4) ij 〉<br />

Thus, the effect looks like a “quadrupole formula” but where<br />

the third time derivative of the moment is replaced by the<br />

fourth one.<br />

BRI-IHP06-I – p.59/??

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