A thermodynamic analysis of the harmonic oscillator is presented. The motivation is provided by the blackbody radiation spectrum, because radiation modes take the harmonic-oscillator form. We use the behavior of a thermal harmonic oscillator system under a quasistatic change of oscillator frequency ω to show that the thermodynamic functions can all be derived from a single function of ω/T, analogous to Wien’s displacement theorem. The high- and low-frequency limits yield asymptotic forms involving the temperature T alone or frequency ω alone, corresponding to energy equipartition and zero-point energy. We suggest a natural interpolation between the limiting forms. The Planck spectrum with zero-point energy corresponds to the function satisfying the Wien displacement result which provides the smoothest possible interpolation between energy equipartition at low frequency and zero-point energy at high frequency.

1.
See, for example, M. Planck, The Theory of Heat Radiation (Dover, New York, 1959), pp. 61–63;
R. Becker and G. Leibfried, Theory of Heat (Springer, New York, 1967), 2nd ed., pp. 16 and 17;
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2.
See, for example, E. A. Power, Introductory Quantum Electrodynamics (American Elsevier, New York, 1964), pp. 18–22.
3.
See, for example, M. Planck in Ref. 1, pp. 72–83, or F. K. Richtmyer, E. H. Kennard, and T. Lauritsen, Introduction to Modern Physics (McGraw–Hill, New York, 1955), pp. 113–118;
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4.
See, for example, R. Reif, Fundamentals of Statistical and Thermal Physics (McGraw–Hill, New York, 1965), pp. 55–56, 251–253;
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5.
I do not know of any text where the harmonic oscillator is treated as a thermodynamics system apart from statistical mechanics.
6.
I am not aware of any thermodynamic treatment of the quasistatic change of the harmonic oscillator frequency. The familiar derivations of the Wien law take the Doppler-shift form given in Ref. 3.
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See the discussion of natural units by C. Garrod, Ref. 9, p. 120. The choice ℏ=1 is familiar to particle physicists. The measurement of temperature in energy units is familiar in thermodynamics where our choice corresponds to the use of what is usually termed τ instead of T. See also, for example, C. Kittel, Elementary Statistical Physics (Wiley, New York, 1958), p. 27.
12.
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13.
I am not aware of any textbook treatment of blackbody radiation that mentions zero-point energy as part of the spectrum involved.
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