I'm studying Quantum mechanics by Bransden and Joachain and in the introduction chapter it says:
Wien showed that the spectral distribution function had to be on the form
$$\rho(\lambda,T)=\lambda^{-5}f(\lambda T)$$
where $f(\lambda T)$ is a function of the single variable $\lambda T$. It is a simple matter to show that Wien's law includes Stefan-Boltzmann law $R(T)=\sigma T^4$.
One of the exercises is to show this and I cannot understand how to.
This is what I've tried:
The relationship between spectral emittance and spectral distribution is
$$\rho(\lambda,T)=\frac{4}{c}R(\lambda,T),$$ where c is the speed of light, which inserted in the above equation gives
$$R(\lambda,T)=\frac{c}{4}\lambda^{-5}f(\lambda T).$$
Now, the total spectral emittance is the integral of $R$ over all wavelengths so
$$ R(T)=\frac{c}{4}\int\limits_0^\infty \lambda^{-5}f(\lambda T)d\lambda $$
This is where I'm stuck. Can anyone help me figure this out?