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habilitation`a diriger les recherches - LUTH - Observatoire de Paris

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386 Kerr solution in Dirac gauge (Vasset et al. 2009)<br />

the h rr spherical component. Let us note that these relations are more tractable when using a scalar<br />

spherical harmonics <strong>de</strong>composition (introduced in Sec. 13.4.2) for all fields. In<strong>de</strong>ed, an angular Laplace<br />

operator acting on a field reduces then to a simple algebraic operation on every spherical harmonics<br />

component. Inverse relations can also be computed to retrieve the classical components of h ij from<br />

spherical harmonics quantities.<br />

We now <strong>de</strong>rive the main variab<strong>les</strong> related to our study: with the divergence-free <strong>de</strong>composition<br />

h ij = D i V j + D j V i + h ij<br />

T<br />

, and Dih ij<br />

T = 0, a choice for three quantities <strong>de</strong>fined from hij and verifying:<br />

can be expressed as the following scalar fields (see [340]):<br />

h ij<br />

T<br />

C = ∂(h − hrr )<br />

∂r<br />

= 0 ⇒ A = B = C = 0, (13.47)<br />

B = ∂W<br />

∂r<br />

− 3hrr<br />

r<br />

A = ∂X<br />

∂r<br />

µ<br />

− , (13.48)<br />

r<br />

∆θϕW η h − hrr<br />

− − + , (13.49)<br />

2r<br />

<br />

r 4r<br />

<br />

h ∂W W<br />

+ − 2∆θϕ + (13.50)<br />

r ∂r r<br />

These quantities can also be <strong>de</strong>composed onto a scalar spherical harmonics basis. The equivalence<br />

in (13.47) is achieved up to boundary conditions.<br />

To show how the quantities A, B and C behave with respect to the Laplace operator, we shall<br />

suppose in the following that the tensor h ij is the solution of a Poisson equation of the type ∆h ij = S ij .<br />

We can <strong>de</strong>duce a scalar elliptic system verified by A, B and C as:<br />

∆A = AS<br />

∆B − C<br />

= BS<br />

(13.52)<br />

2r2 (13.51)<br />

∆C + 2C 8∆θϕB<br />

+<br />

r2 r2 = CS, (13.53)<br />

Where AS, BS and CS are the corresponding quantities associated with the source Sij . A simple<br />

way of <strong>de</strong>coupling the last two elliptic equations is to <strong>de</strong>fine the variab<strong>les</strong> ˜ B = <br />

l,m ˜ BlmYlm and<br />

˜C = <br />

l,m ˜ ClmYlm with:<br />

˜B lm = B lm + Clm<br />

Thus, we can write an equivalent system for (13.51,13.52,13.53) as:<br />

,<br />

2(l + 1)<br />

(13.54)<br />

˜C lm = C lm − 4lB lm . (13.55)<br />

∆A = AS, (13.56)<br />

˜∆ ˜ B = ˜ BS, (13.57)<br />

∆ ∗ ˜ C = ˜ CS, (13.58)<br />

With the following elliptic operators <strong>de</strong>fined for each spherical harmonic in<strong>de</strong>x l:

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