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3+1 formalism and bases of numerical relativity - LUTh ...

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9.3 Evolution <strong>of</strong> spatial coordinates 165<br />

<strong>and</strong> QTT ij is both traceless <strong>and</strong> transverse (i.e. divergence-free) with respect to the metric γ:<br />

DjQTT ij = 0. X is then related to the divergence <strong>of</strong> Q by Dj (LX)ij = DjQij. It is legitimate to<br />

relate the TT part to the dynamics <strong>of</strong> the gravitational field <strong>and</strong> to attribute the longitudinal<br />

part to the change in γij which arises because <strong>of</strong> the variation <strong>of</strong> coordinates from Σt to Σt+δt.<br />

This longitudinal part has 3 degrees <strong>of</strong> freedom (the 3 components <strong>of</strong> the vector X) <strong>and</strong> we<br />

might set it to zero by some judicious choice <strong>of</strong> the coordinates (xi ). The minimal distortion<br />

coordinates are thus defined by the requirement X = 0 or<br />

i.e.<br />

Qij = Q TT<br />

ij , (9.51)<br />

D j Qij = 0 . (9.52)<br />

Let us now express Q in terms <strong>of</strong> the shift vector to turn the above condition into an equation<br />

for the evolution <strong>of</strong> spatial coordinates. By means <strong>of</strong> Eqs. (4.63) <strong>and</strong> (9.9), Eq. (9.45) becomes<br />

Qij = −2NKijLβ γij + − 1<br />

<br />

−2NK + 2Dkβ<br />

3<br />

k<br />

γij, (9.53)<br />

i.e. (since Lβ γij = Diβj + Djβi)<br />

Qij = −2NAij + (Lβ)ij, (9.54)<br />

where we let appear the trace-free part A <strong>of</strong> the extrinsic curvature K [Eq. (6.53)]. If we insert<br />

this expression into the minimal distortion requirement (9.52), we get<br />

− 2NDjA ij − 2A ij DjN + Dj(Lβ) ij = 0. (9.55)<br />

Let then use the momentum constraint (4.66) to express the divergence <strong>of</strong> A as<br />

DjA ij = 8πp i + 2<br />

3 Di K. (9.56)<br />

Besides, we recognize in Dj(Lβ) ij the conformal vector Laplacian associated with the metric γ,<br />

so that we can write [cf. Eq. (B.11)]<br />

Dj(Lβ) ij = DjD j β i + 1<br />

3 Di Djβ j + R i j βj , (9.57)<br />

where R is the Ricci tensor associated with γ. Thus we arrive at<br />

DjD j β i + 1<br />

3 Di Djβ j + R i j βj = 16πNp i + 4<br />

3 NDi K + 2A ij DjN . (9.58)<br />

This is the elliptic equation on the shift vector that one has to solve in order to enforce the<br />

minimal distortion.<br />

Remark : For a constant mean curvature (CMC) slicing, <strong>and</strong> in particular for a maximal<br />

slicing, the term D i K vanishes <strong>and</strong> the above equation is slightly simplified. Incidentally,<br />

this is the form originally derived by Smarr <strong>and</strong> York (Eq. (3.27) in Ref. [246]).

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