Density distributions add by convolution, and the result is also a density distribution. So writing this in the time domain, w.l.o.g., the question becomes how do we take a faster gamma distribution:
${\mathrm{GD_{fast}}}\left(\mathrm{a} ;\ \mathrm{b}; \tau \right)=\left\{\begin{array}{cc}\hfill \frac{{\mathrm{b}}^{\mathrm{a}}}{\Gamma \left(\mathrm{a}\right)}{\tau}^{\mathrm{a}-1}{e}^{-\mathrm{b}\kern0.1em \tau },\hfill & \hfill \tau\ \ge\ 0\hfill \\ {}\hfill \kern2.75em 0\kern1.5em ,\hfill & \hfill \tau <0\hfill \end{array}\right.,$
where $\tau $ is time, and add it to a slower one:
${\mathrm{GD}}_{\mathrm{slow}}\left(\alpha; \beta; \tau \right)=\left\{\begin{array}{cc}\hfill \frac{\beta^{\kern0.1em \alpha }}{\Gamma \left(\alpha \right)}{\tau}^{\alpha -1}{e}^{-\beta\;\tau },\hfill & \hfill \tau \ge 0\hfill \\ {}\hfill \kern3em 0\kern1.2em ,\hfill & \hfill \kern1.4em \tau <0\hfill \end{array}\right.,$
The notation here assigns the rate scalar $\beta=\frac{1}{\theta}$, where $\theta$ is the time scalar. Both parameterizations are in common use. Thus, when we require $b>\beta$, we are requiring that $\text{GD(b)}$ to be faster (e.g., lighter right-tailed) than $\text{GD}(\beta)$. The solution is well known for the simpler case when $\mathrm{b}=\beta$; it is also a gamma distribution. But what we (Q1) want is a general closed form convolution solution for the sum of two gamma distributions: a gamma distribution convolution of the type
$\mathrm{GDC}\left(\mathrm{a}\kern0.1em ,\mathrm{b},\alpha, \beta; \tau \right)={\mathrm{GD_{fast}}}\left(\mathrm{a},\mathrm{b};\;\tau \right)\otimes {\mathrm{GD_{slow}}}\left(\alpha, \beta; \tau \right),$
Finally, we (Q2) want some indication of whether this can be used to form reasonable models, and whether or not it has found practical applications.