I have been trying to solve Poisson's Equation, given by $$\nabla^2\Phi(\vec{r}) = -\frac{\rho(\vec{r})}{\epsilon_0}$$ for the given charge density $$\rho(\vec{r}) = \frac{\rho_0}{m}\frac{e^{-mr}}{r}$$ for positive parameters $\rho_0$ and $m$, subject to the boundary condition that $\Phi(\vec{r})\rightarrow 0$ as $r\rightarrow\infty$. To do this, I did a Fourier Transform of the initial equation, which I then solved for the Fourier Transform of $\Phi(\vec{r})$, $\hat{\Phi}(\vec{k})$ to obtain: $$\hat{\Phi}(\vec{k}) = \frac{4\pi\rho_0}{m\epsilon_0}\frac{1}{m^2 + k^2}$$ When applying the Inverse Fourier Transform, the integral in question arises as the last integral to calculate - $\Phi(\vec{r})$ is given by $$\Phi(\vec{r}) = \frac{\rho_0}{\pi\epsilon_0 mr}\int_{0}^{\infty}dk\frac{\sin(kr)}{k(k^2 + m^2)}$$ I have entered this integral into Wolfram Alpha, which gives me the result $$\Phi(\vec{r}) = \frac{\rho_0}{\epsilon_0 m^3 r}(1 - e^{-mr})$$ This agrees with the result one obtains when calculating $\Phi(\vec{r})$ directly using the formula obtained by using the Green Function of the $\nabla^2$-Operator, so I know that it is correct.
However, I'd still be interested in how one would go about evaluating this integral, because none of the integration techniques that I know seem to work at all.
Any help would be much appreciated.
According to Plancherel's formula \begin{equation*} \int_{-\infty}^{\infty}\overline{f(x)}g(x)\, dx = \dfrac{1}{2\pi}\int_{-\infty}^{\infty}\overline{F(\xi)}G(\xi)\, d\xi \end{equation*} where $f,g\in L_{2}(\mathbb{R})$ and $F(\xi) = \int_{-\infty}^{\infty}f(x)e^{-i\xi x}\, dx$ (Fourier transform).
If $f(x) = \dfrac{\sin(xr)}{x}$ then $F(\xi) = \pi(H(\xi+r)-H(\xi-r))$, where $H$ is the Heaviside step function. Futhermore, if $g(x) = \dfrac{1}{x^2+m^2}$ then $G(\xi) = \dfrac{\pi}{m}e^{-|m\xi|}$.
Thus \begin{equation*} \int_{-\infty}^{\infty}\dfrac{\sin(xr)}{x(x^2+m^2)}\, dx = \dfrac{1}{2\pi}\int_{-r}^{r}\dfrac{\pi^2}{m}e^{-|m\xi|}\, d\xi = \dfrac{\pi}{m}\int_{0}^{r}e^{-m\xi}\, d\xi = \dfrac{\pi}{m^2}(1-e^{-mr}). \end{equation*} Finally \begin{equation*} \Phi = \dfrac{\rho_{0}}{2\epsilon_{0}m^{3}r}(1-e^{-mr}) \end{equation*} with an extra 2 factor.