Condensing Matters:
A Summary Derivation of the Planck Formula for Black Body Radiation


PRL gif

ω is a chosen angular frequency of light.
τ is temperature, c the speed of light.
uω is energy per unit volume per unit frequency range.

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Introduction
My experience of thermodynamics might have begun with Rudy Marcus if I had managed to attend more of his lectures. Sleep contends with ambition in and out of the lecture hall I suppose. Instead my proper introduction to thermodynamics began with a book (fairly remarkable): Professors Kittel and Kroemer's Thermal Physics published 1980. It was such a good introduction that I feel it worth a revisit. The first 90 pages cover important foundational ideas of thermodynamics and conclude with a derivation of the Planck formula for black body radiation. This derivation ends with the words "This result is the Planck radiation law; it gives the frequency distribution of thermal radiation. Quantum theory began here."

So that's it: Where the river begins. All I need do is follow that 90-page derivation to arrive at the PRL and from there continue downstream into the rest of quantum mechanics. In fact these 90 pages include other ideas; it's a matter of following the central thread based on a fundamental premise: All accessible states of a closed system are equally likely.

Historical note: Planck found the PRL using ideas about Harmonic Oscillators and it was Einstein in 1905 who started the shift towards connecting oscillators to quantized energy and hence light as energy corpuscles (photons). The derivations have the same form but the physical ideas had evolved in Einstein's 1905 contribution. In any event the point of this page is to condense K&K's derivation into a review-derivation of the PRL "the easy/modern way".

Chapter 1 of Kittel and Kroemer: States of a Model System
Examination of an idealized system of many constitutive elements, all identical, all capable of occupying one of two states.

The 'model system' states are taken to be spin-up or spin-down. The system consists of N sites where N is an even number for convenience. Rather than start with all-up or all-down, start with half-up and half-down and consider variations where s sites flip over from - to + giving a spin excess of +2s . That is, when s = 0 the total spin is zero. When s = 1 the total spin is 2, and when s=19 the total spin is 38. Suppose (N/2 + s) magnets are up; how many ways can these be distributed? We use the Combination idea "N-choose-(N/2 + s)" from the binomial theorem to arrive at the multiplicity function g(N,s). This tells us how many different states are available with spin excess s.

g(N, s) = (N N/2+s).


This multiplicity function becomes important when the system has a total energy U attached. The example given is the application of an external magnetic field, in which case the little magnets contribute to or detract from the total system energy. The sum of the magnetic spins is important but their ordering is not; the multiplicity function accounts for just this.


Chapter 2 of Kittel and Kroemer: Entropy and Temperature
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Chapter 3 of Kittel and Kroemer: Boltzmann Distribution and Helmholtz Free Energy
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Chapter 4 of Kittel and Kroemer: Thermal Radiation and Planck Distribution
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Concluding Thoughts
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