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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Method of variation of constants First construct soln to the ‘unperturbed’ system, defined by ˙x = v , ˙v = A0(x, v). The solution to the exact system ˙x = v , ˙v = A(x, v) , obtained by varying the constants in the generic solutions of the unperturbed system. The method assumes ( true for A conservative 2P N or Aconservative 3P N ) that the unperturbed system admits sufficiently many integrals of motion to be integrable. E.g. if A0 = A2P N, we have four first integrals: the 2PN accurate energy and 2PN accurate angular momentum of the binary written in the 2PN accurate center of mass frame as c1 and ci BRI-IHP06-I – p.102/?? 2:

Method of variation of constants c1 = E(x1, x2, v1, v2)|2(3)PN CM , c i 2 = Ji(x1, x2, v1, v2)|2(3)PN CM , Vectorial structure of c i 2, indicates that the unperturbed motion takes place in a plane. Problem is restricted to a plane even in the presence of radiation reaction. Introduce polar coordinates in the plane of the orbit r and φ such that x = i r cos φ + j r sin φ with, i = p, j = q cos i + N sin i. Functional form for the solution to the unperturbed equations of motion may be expressed as r = S(l; c1, c2) ; ˙r = n ∂S ∂l (l; c1, c2) , φ = λ + W (l; c1, c2) ; ˙ φ = (1 + k)n + n ∂W ∂l (l; c1, c2) , where λ and l are two basic angles, which are 2π periodic and c2 = |c i 2|. BRI-IHP06-I – p.103/??

Method of variation of constants<br />

First construct soln to the ‘unperturbed’ system, def<strong>in</strong>ed by<br />

˙x = v ,<br />

˙v = A0(x, v).<br />

The solution to the exact system<br />

˙x = v ,<br />

˙v = A(x, v) ,<br />

obta<strong>in</strong>ed by vary<strong>in</strong>g the constants <strong>in</strong> the generic solutions of<br />

the unperturbed system. The method assumes ( true for<br />

A conservative<br />

2P N<br />

or Aconservative 3P N ) that the unperturbed system<br />

admits sufficiently many <strong>in</strong>tegrals of motion to be <strong>in</strong>tegrable.<br />

E.g. if A0 = A2P N, we have four first <strong>in</strong>tegrals: the 2PN<br />

accurate energy and 2PN accurate angular momentum of<br />

the b<strong>in</strong>ary written <strong>in</strong> the 2PN accurate center of mass frame<br />

as c1 and ci BRI-IHP06-I – p.102/??<br />

2:

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