The Euclidean Laplacian of a scalar function is

Δf=i=1nxi2f.\Delta f=\sum_{i=1}^n\partial_{x_i}^2 f.

For a vector field it acts on Cartesian components: (Δu)i=Δui(\Delta u)_i=\Delta u_i. This convention has Fourier symbol ξ2-|\xi|^2 when derivatives have symbol iξi\xi.

Cylindrical coordinates

For scalar functions on r>0r>0, set

L=r2+r1r+r2θ2+z2.L=\partial_r^2+r^{-1}\partial_r+r^{-2}\partial_\theta^2+\partial_z^2.

Then Δf=Lf\Delta f=Lf. For cylindrical vector components,

(Δu)r=Lurr2ur2r2θuθ,(Δu)θ=Luθr2uθ+2r2θur,(Δu)z=Luz.\begin{aligned} (\Delta u)_r&=Lu_r-r^{-2}u_r-2r^{-2}\partial_\theta u_\theta,\\ (\Delta u)_\theta&=Lu_\theta-r^{-2}u_\theta+2r^{-2}\partial_\theta u_r,\\ (\Delta u)_z&=Lu_z. \end{aligned}

These follow by applying LL to urer+uθeθ+uzezu_r e_r+u_\theta e_\theta+u_z e_z and differentiating the frame. Applying the scalar formula separately to moving components would omit the displayed terms.

References