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Remarks

1. Note that ironically, quantum mechanics was discovered via the classical limit of a radiation law! In fact, the Rayleigh-Jeans-law contains no Planck constant $ h$, whereas the parameters $ a$ and $ b$ in the 19th-century `thermodynamic' Wien law contain $ h$ and $ k_B$, both fundamental constants in microscopic theories (although at that time, the deep physical meaning of $ a$ and $ b$ was of course not understood).

2. Nowadays, instead of $ h$ one often uses $ \hbar = h/2\pi$. Instead of the frequency $ \nu$ one often uses the angular frequency $ \omega=2\pi\nu$. If $ \omega$ is used instead of $ \nu$, the spectral energy density $ w(\omega,T)$ is defined as $ w(\omega,T)d\omega = u(\nu,T)d\nu$. Since $ d\omega = 2\pi d\nu$, this gives $ w(\omega,T)=
{\omega^2}/(\pi^2 c^3)\times \hbar\omega /(\exp(\hbar\omega/kT)-1)$. Therefore, be careful when comparing different definitions and doing calculations because a wrong factor $ 2\pi$ gives a result that is wrong by nearly one order of magnitude!

3. Cosmic black body radiation is a consequence of the `Big Bang Model'. Measurements of the cosmic background radiation corresponding to a temperature $ T\approx 2.7$K were performed by R. H. Dicke and co-workers.


next up previous contents
Next: * Math: Density of Up: The Radiation Laws and Previous: The Radiation Laws and   Contents
Tobias Brandes 2004-02-04