The Laplacian Commutes with Isometries

A short proof using naturality of the exterior derivative and Hodge star.

This short note proves the following theorem relating the laplacian on a Riemannian manifold and its isometries:

Theorem

Let (M,g)(M,g) be a Riemannian manifold and Φ ⁣:MM\Phi\colon M\to M an isometry. Then for any F ⁣:MRF\colon M\to\RR Δ(FΦ)=(ΔF)Φ\Delta(F\circ \Phi)=(\Delta F)\circ \Phi

Here’s the main idea: the composition FΦF\circ \Phi is the pullback of FF by Φ\Phi, FΦ=ΦFF\circ\Phi = \Phi^\ast F And the laplacian is a repeated composition of hodge stars and exterior derivatives. So, we just need to commute each one with the pullback, one at a time. We record each of these as a lemma below:

LemmaExterior Derivative Commutes with Pullbacks

Let α\alpha be a kk-form on MM and Φ ⁣:MM\Phi\colon M\to M. Then d(Φα)=Φ(dα)d(\Phi^\ast \alpha)=\Phi^\ast(d\alpha)

Proof

Note this first result is completely general and does not care that Φ\Phi is an isometry (as one expects, since dd does not know about the metric structure). However the hodge dual is defined in terms of the metric (indirectly through the volume form) so the isometry is crucial below.

LemmaHodge Star Commutes with Pullbacks

Let (M,g)(M,g) be a Riemannian manifold and Φ\Phi an orientation preserving isometry of MM. Then if α\alpha is a kk-form, (Φα)=Φ(α)\star (\Phi^\ast \alpha)=\Phi^\ast(\star \alpha)

Proof

Now we can prove the main theorem by a short computation:

Δ(FΦ)=Δ(ΦF)=dd(ΦF)=dΦ(dF)=dΦ(dF)=Φ(ddF)=Φ(ddF)=ΦΔF=(ΔF)Φ\begin{align} \Delta(F\circ \Phi) &=\Delta(\Phi^\ast F)\\ &= \star d\star d(\Phi^\ast F)\\ &=\star d\star \Phi^\ast (d F)\\ &= \star d\,\Phi^\ast(\star dF)\\ &= \star\, \Phi^\ast(d\star dF)\\ &= \Phi^\ast(\star d\star d F)\\ &= \Phi^\ast \Delta F\\ &= (\Delta F)\circ \Phi \end{align}

This computation goes through exactly if Φ\Phi is orientation preserving. If it is orientation reversing, then we need to modify the argument for the Hodge star, and see that in fact commuting introduces a minus sign. But the Laplacian uses the hodge star twice, so these cancel and the final result holds for any isometry of MM.

This is one of the two ingredients (along with the chain rule) in the spherically symmetric fundamental solution, where it is what forces Δr\Delta r to be constant on the geodesic spheres about OO.

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