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The inhomogeneous wave equation $$\left(\frac{1}{c^2} \partial_t^2 - \Delta\right)G(\vec{r},t)=\delta^3(\vec{r})\delta(t) \tag{0}$$ for a point-source in three spatial dimensions can be tackled by means of the Fourier-space, that is writing $$G(\vec{r},t)=\frac{1}{(2\pi)^4} \int {\rm d}^3k \int {\rm d}\omega \, \tilde{G}(\vec{k},\omega) \, e^{i\vec{k}\vec{r}-i\omega t} \\ \delta(\vec{r})\delta(t)=\frac{1}{(2\pi)^4}\int {\rm d}^3k \int {\rm d}\omega \, e^{i\vec{k}\vec{r}-i\omega t} $$ and plugging these into (0), which gives $$\left(k^2-\frac{\omega^2}{c^2}\right)\tilde{G}=1$$ and so $$\tilde{G}=\frac{1}{k^2-\omega^2/c^2} + a_1(\vec{k}) \delta(k-\omega/c) + a_2(\vec{k})\delta(k+\omega/c)$$ with arbitrary functions $a_1$ and $a_2$. These terms actually only give the homogenous solution. The first term is responsible for the inhomogeneity. Then, $$G(\vec{r},t)=\frac{c^2}{(2\pi)^4} \int {\rm d}^3k \int {\rm d}\omega \, \frac{1}{k^2c^2-\omega^2} \, e^{i\vec{k}\vec{r}-i\omega t} \tag{1} \, .$$

For $t>0$, the $\omega$-integral, can be calculated by closing the contour in the lower-half complex plane. A physical causality argument then justifies pushing the poles at $\omega=\pm kc$ in the lower-half complex plane and the residue-theorem then gives $$G(\vec{r},t)=\frac{-ic}{16\pi^3} \int \frac{{\rm d}^3k}{k} \, e^{i\vec{k}\vec{r}} \left( e^{ikct} - e^{-ikct} \right) \, . \tag{2}$$ Evaluating this remaining integral is most easily done in 3d-spherical coordinates with the result $$G(\vec{r},t)=\frac{1}{4\pi r} \, \delta(t-r/c) \,. \tag{3}$$ The result has the interpretation, that an instantaneous perturbation at $t=0$ and $\vec{r}=0$, will only have an effect at $r$ after the retarded time $r/c$.

My question is now with regard to the version in 2+1D. The analysis above holds, except (2) becomes $$G(\vec{r},t)=\frac{-ic}{8\pi^2} \int \frac{{\rm d}^2k}{k} \, e^{i\vec{k}\vec{r}} \left( e^{ikct} - e^{-ikct} \right) \, . \tag{4}$$

With polar-coordinates (4) becomes $$G(\vec{r},t)=\frac{-ic}{8\pi^2} \int_0^{2\pi} {\rm d}\varphi \int_0^\infty {\rm d}k \, e^{ikr\cos\varphi} \left( e^{ikct} - e^{-ikct} \right) \, . $$ where wlog $\vec{r}=r \vec{e}_x$ was assumed. The $k$-integral does not converge, but can be continued analytically by introducing a dampening factor $e^{-ks}$ and taking the limit $s\to 0^+$ with the result $$G(\vec{r},t)=\frac{c}{4\pi^2} \int_0^{2\pi} {\rm d}\varphi \, \frac{ct}{c^2t^2-r^2\cos^2t}. $$ If $r>ct$, then the integral is only defined as a principal value and becomes $0$. It is only non-zero for $r<ct$ and can be done via the residue theorem $$G(\vec{r},t)=\frac{1}{2\pi} \frac{\Theta(ct-r)}{\sqrt{t^2-r^2/c^2}} \, . \tag{5}$$ The fact that $r<ct$ is causally plausible, since an instantaneous perturbation at $t=0$ and $\vec{r}=0$ can not have an effect at $r$ if $ct<r$ i.e. the wave hasn't had the time to travel the distance. But contrary to the 3+1D case, the Greens function in the 2+1D case does not appear to exhibit a sharp response i.e. the instantaneous perturbation at $t=0$ and $\vec{r}=0$ does only act at distance $r$ after the the time $r/c$, but the same position at distance $r$ will be affected at later times as well, after the pulse should have passed already.

Is there a mathematical error, or what is the interpration to this?

Qmechanic
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Diger
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This is correct. Your result is given in Jackson's, Classical Electrodynamics as problem 6.1. Physically, you can imagine that the 2-d source is a line source in 3-d. The radiation from the closest point is the initial effect, and radiation from the rest of the long line source takes longer to get to your observation point. Jackson calls this a "wake".

user200143
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