What kind sort of impact might intensely blue shifted cosmic microwave background (CMB) photons have on hawking radiation?
short answer: I don't think any..
long answer:
Not sure just what you are getting at here. A distant observer, say on earth, would typically see CMBR as blue shifted approaching a distant black hole. This would be the opposite effect from observing red shifted photons were photons to emerge from a dense gravitational potential. But no black holes are emitting Hawking radiation, insofar as is known, because the universe is warmer than the black holes...so black holes are not currently evaporating.
If Hawking radiation were actually occurring, it would be because the black hole(s) were warmer than surrponding space (our universe)...and we'd observe some photons emerging. A rough analogy is to ask "how do photons from one star interact with those from another?"...in general electromagnetic radiation moves about with little interaction with other electromagnetic.
If you are referring to huge emissions of electromagnetic radiation from the vicintyof black holes, such as the center of aour galaxy, that frictional driven radiation from gas clouds outside the black hole rapidly accelerating in the vicinity of a massive black hole..it's not Hawking radiation which has never been observed.
Could intensely blue shifted CMB photons drive a portion of newly created electrons and positrons into the even horizon before they annihilate giving off gama rays that wouldn't interact with income photons
.
Again, I'm unsure what this means...but I'm not good on particle annihilation...
when a particle and it's antiparticle annihilate in quantum theory no energy is released...and Hawking radiation, when a particle (photon) is observed, it's photons (electromagnetic radiation) not electrons...like black body radiation...
Gamma rays are very high energy electromagnetic radiation, CMBR is low energy...but each is photons (bundles or quanta of electromagnetic radiation) just different frequency and different energy...via E =hf...