Hmm...I'm not sure what you mean. I know there are a couple of ways to treat Compton scattering. The first way involves finding the frequency (or wavelength) shift in the Compton-scattered photon. This can be done by imposing momentum and energy conservation on the system as well as the following relations for the photon:
[tex]E = hf[/tex]
[tex]E = pc[/tex]
That's where you get the following equation:
[tex]\lambda' - \lambda = \dfrac{h}{mc}(1-cos(\theta))[/tex]
The energy-frequency relation for a photon is basically how we relate the wave and particle theories of light. The energy-momentum relation is pretty much just relativity with the understanding that the photon is a massless particle. So I guess that even here we're using "classical" and "photon" models. Depending on your definition of quantum mechanics though, even treating the photon as a particle is still "classical physics."
Now you can also use quantum field theory to write out the Feynman diagram for Compton scattering (since it's a quantum electrodynamic process). That's how you can calculate the scattering cross-section for this process. It's pretty important for us in astrophysics, since scattering works differently in the Thompson regime (low energy) and Klein-Nishina regime (high energy). I don't know if you're supposed to worry about that though.
You could probably work out the energy change in a photon by treating it as simple classical scattering. But to turn that into a frequency you'd need to use the "photon model."