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Homework Statement
Black body radiation inside a cavity at temperature T may be thought of as a gas of photons with an energy distribution given by the function n(E) given by
n(E)dE = A [E^2 / (e^(E/kT) - 1) ] dE
Where A is independent of E and T. (k is Boltzmann constant)
The function n(E) describes the number of photons with energy between E and E + dE. There is no upper limit on E (although n(E) -> 0 as E -> 0)
Show that
a) the total number of photons is proportional to T^3 and
b) the total energy is proportional to T^4
Homework Equations
The Attempt at a Solution
So I'm a bit confused!
To work out the total number of photons, do I just do the integral of n(E)dE with E from 0 to infinity? How is this proportional to T^3?
How do I work out an expression for the total energy (since n(E) just describes the number of the photons..) ?
Thanks