- #1
UHECRon
- 4
- 0
I am interested in what the average photon densities are within galactic environments due to non CMB sources. In extra galactic environments, the CMB certainly dominates, however as you enter more dense and luminous areas (e.g. , the galactic disc) broad spectrum photon densities from local sources must climb. My question is how does this compare on average to CMB?
I ask as the answer may have implications on cosmic ray phenomenology.
I ask as the answer may have implications on cosmic ray phenomenology.