Context
The wave equation
$$ \partial_{tt}\psi=v^2\nabla^2 \psi $$
describes waves that travel with frequency-independent speed $v$, ie. the waves are dispersionless. The character of solutions is different in odd vs even number of spatial dimensions, $n$. A point source in odd-$n$ creates a disturbance that propagates on the light cone and vanishes elsewhere: if the point source is a flash of light, an observer sees darkness, then a flash, then darkness. When $n$ is even, a disturbed media never returns to rest: the observer sees darkness, then brightness that lingers for all $t$. This phenomena is known as geometric dispersion.
Question
Is it possible to show that geometric dispersion is predicted by the wave equation, using group theory? For a point source at the origin, we would be searching for spherically symmetric solutions, and the rotation group $SO(n)$ has a different structure depending on whether $n$ is odd or even. In particular, I am interested in doing this without actually solving the wave equation. Unfortunately, I don't know enough group theory to know if this is even possible.
What I know
I can 'show' geometric dispersion by solving the wave equation with an initial condition, or computing the Green's function for the wave equation and noting that it is either supported only on the light cone (odd $n$), or everywhere within the light cone (even $n$).
I know some group theory 'for physicists'.
Related
This unanswered question is similar. I think my question is more specific: I'm asking about a way to predict (rather than explain) geometric dispersion using group theory.
Update: (thanks to comments of Alp Uzman and GiuseppeNegro) It appears to be possible using group theoretic machinery, described in the book Nonabelian harmonic analysis by Howe and Tan. The relevant section is 4.3.1. So an equivalent question becomes: can someone explain the result from Howe and Tan in a more accessible way? The book is beyond my level of group theory at the moment.