This is my first time posting here!
I want to model the photons ejected from a blackbody source at temperature T.
The question I want answered is: given a photon is detected, what is the probability of the photon having a wavelength λ. This amounts to just attaining the probability density function for the different wavelengths.
We normal talk about blackbodies in terms of intensity, or more specifically spectral radiance, but I want to talk about the individual photon wavelength distribution.
My current thoughts are:
Any thoughts on whether this is right?
EDIT: The attached graphs are nothing to do with anything. Apparently they just came along for the ride. Bless 'em.