3+1 formalism and bases of numerical relativity - LUTh ...
3+1 formalism and bases of numerical relativity - LUTh ...
3+1 formalism and bases of numerical relativity - LUTh ...
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4.4 The Cauchy problem 63<br />
hightest degree (two in the present case). We get, denoting by “· · ·” everything but a second<br />
order derivative <strong>of</strong> γij:<br />
Rij = ∂Γkij ∂xk − ∂Γk ik + · · ·<br />
∂xj = 1 ∂<br />
2 ∂xk <br />
γ kl<br />
<br />
∂γlj ∂γil ∂γij<br />
+ −<br />
∂xi ∂xj ∂xl <br />
− 1 ∂<br />
2 ∂xj <br />
γ kl<br />
<br />
∂γlk<br />
∂x ∂x<br />
= 1<br />
2 γkl<br />
<br />
∂2γlj Rij = − 1<br />
2 γkl<br />
<br />
∂2γij ∂xk∂xl + ∂2γkl ∂xi∂xj − ∂2γlj ∂xi∂xk − ∂2γil ∂xj∂xk <br />
+ Qij<br />
∂γil ∂γik<br />
+ − i k<br />
∂xk∂xi + ∂2γil ∂xk∂xj − ∂2γij ∂xk∂xl − ∂2γlk ∂xj∂xi − ∂2γil ∂xj∂xk + ∂2γik ∂xj∂xl γkl, ∂γkl<br />
∂x m<br />
∂xl <br />
+ · · ·<br />
<br />
+ · · ·<br />
<br />
, (4.86)<br />
where Qij(γkl,∂γkl/∂x m ) is a (non-linear) expression containing the components γkl <strong>and</strong> their<br />
first spatial derivatives only. Taking the trace <strong>of</strong> (4.86) (i.e. contracting with γij ), we get<br />
<br />
. (4.87)<br />
Besides<br />
R = γ ik γ jl ∂2γij ∂xk∂xl − γijγ kl ∂2γij ∂xk + Q<br />
∂xl Dj(γ jk ˙γki) = γ jk Dj ˙γki = γ jk<br />
<br />
∂ ˙γki<br />
= γ jk ∂2γki ∂xj <br />
+ Qi<br />
∂t<br />
γkl, ∂γkl<br />
∂x m<br />
∂x j − Γl jk ˙γli − Γ l ji ˙γkl<br />
γkl, ∂γkl ∂γkl<br />
∂xm, ∂t<br />
<br />
<br />
, (4.88)<br />
where Qi(γkl,∂γkl/∂x m ,∂γkl/∂t) is some expression that does not contain any second order<br />
derivative <strong>of</strong> γkl. Substituting Eqs. (4.86), (4.87) <strong>and</strong> (4.88) in Eqs. (4.83)-(4.85) gives<br />
− ∂2 <br />
γij ∂2γij + γkl<br />
∂t2 ∂xk∂xl + ∂2γkl ∂xi∂xj − ∂2γlj ∂xi∂xk − ∂2γil ∂xj∂xk <br />
= 8π [(S − E)γij − 2Sij]<br />
<br />
+Qij γkl, ∂γkl<br />
<br />
∂γkl<br />
∂xm, (4.89)<br />
∂t<br />
γ ik γ jl ∂2γij ∂xk∂xl − γijγ kl ∂2γij ∂xk <br />
= 16πE + Q γkl,<br />
∂xl ∂γkl<br />
<br />
∂γkl<br />
∂xm, (4.90)<br />
∂t<br />
γ jk ∂2γki ∂xj∂t − γkl ∂2γkl ∂xi∂t = −16πpi<br />
<br />
+ Qi γkl, ∂γkl<br />
<br />
∂γkl<br />
∂xm, . (4.91)<br />
∂t<br />
Notice that we have incorporated the first order time derivatives into the Q terms.<br />
Equations (4.89)-(4.91) constitute a system <strong>of</strong> PDEs for the unknowns γij. This system is <strong>of</strong><br />
second order <strong>and</strong> non linear, but quasi-linear, i.e. linear with respect to all the second order<br />
derivatives. Let us recall that, in this system, the γ ij ’s are to be considered as functions <strong>of</strong> the<br />
γij’s, these functions being given by expressing the matrix (γij) as the inverse <strong>of</strong> the matrix (γij)<br />
(e.g. via Cramer’s rule).<br />
A key feature <strong>of</strong> the system (4.89)-(4.91) is that it contains 6 + 1 + 3 = 10 equations for<br />
the 6 unknowns γij. Hence it is an over-determined system. Among the three sub-systems