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

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Periodic variations<br />

˜cλ = 2ξ5/3 η<br />

45e 2 t<br />

βt = (1 −<br />

<br />

18<br />

χ2 − 56 − 36e2 t<br />

χ3 + 105(1 − e2 t )<br />

χ 4<br />

<br />

1<br />

− e2 t − 144e2 t<br />

χ − 18 − 258e2 t<br />

χ2 + 56 − 92e2 t + 36e4 t<br />

χ3 − 105(1 − e2 t )2<br />

χ4 1<br />

+<br />

2(1 − e2 t )2<br />

134 2<br />

+ 103et − 252e 4 <br />

t 1 − e2 t − 134 − 295e 2 t − 36e4 t<br />

−<br />

ξ 7/3 η<br />

4725e 2 t (1 − e2 t )<br />

+(5400 + 45990η)e 2 t<br />

1 − e 2 t )/et.<br />

21060 − 49770η<br />

1<br />

· · · · · ·<br />

χ2 <br />

+ 48ξ7/3 η<br />

5(1 − e 2 t )<br />

<br />

<br />

1 5<br />

(v − u) −<br />

χ3 χ4 The constant contributions to the time evolution of ˜cl and ˜cλ, appear<strong>in</strong>g <strong>in</strong><br />

are required to guarantee the zero-average behaviour.<br />

We note that the rema<strong>in</strong><strong>in</strong>g <strong>in</strong>tegral <strong>in</strong> Eq. can be numerically evaluated.<br />

<br />

<br />

χ du ,<br />

BRI-IHP06-I – p.142/??

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