Hi Pete:
I am not sure how to define the beginning and end of the radiation epoch, but I will take a crack at it.
The beginning
The radiation epoch must come after the inflation epoch ends, since the scale factor during inflation is
a ≈ et.
Here is a quote from Wikipedia:
You are correct that the radiation epoch is characterized by
a ≈ t1/2.
The end
I don't think there is a well defined criterion for this. The end will occur before ρ
r, the mass-energy density of radiation (photons) equals the mass-energy density of matter ρ
m. The problem is deciding on the value of the ratio
R = ρr : ρm > 1
to use for the end of the radiation epoch and the start of the transition to the matter epoch. When that transition ends, the matter epoch is characterized by
a ≈ t2/3.
If you specify the value you want to use for R, it is easy to calculate the value of a which corresponds to this R value. Calculating the corresponding value for t is more difficult.
Regards,
Buzz