Helmholtz theorem (classical mechanics) explained

The Helmholtz theorem of classical mechanics reads as follows:

Let $$H(x,p;V)\; =\; K(p)\; +\; \backslash varphi(x;V)$$ be the Hamiltonian of a one-dimensional system, where $$K\; =\; \backslash frac$$ is the kinetic energy and $$\backslash varphi(x;V)$$ is a "U-shaped" potential energy profile which depends on a parameter

V .Let \left\langle ⋅ \right\rangle _{t} denote the time average. Let E = K + \varphi, T = 2 \left\langle K\right\rangle _{t} , P = \left\langle - (\partial \varphi)/(\partial V) \right\rangle _{t} , S(E,V) =log \oint \sqrt{ 2 m\left( E - \varphi \left( x,V\right) \right) }dx.

Then $$dS\; =\; \backslash frac.$$

Remarks

T is given by time average of the kinetic energy, and the entropy S by the logarithm of the action (i.e., $\backslash oint\; dx\; \backslash sqrt$).
The importance of this theorem has been recognized by Ludwig Boltzmann who saw how to apply it to macroscopic systems (i.e. multidimensional systems), in order to provide a mechanical foundation of equilibrium thermodynamics. This research activity was strictly related to his formulation of the ergodic hypothesis.A multidimensional version of the Helmholtz theorem, based on the ergodic theorem of George David Birkhoff is known as the generalized Helmholtz theorem.

Generalized version

The generalized Helmholtz theorem is the multi-dimensional generalization of the Helmholtz theorem, and reads as follows.

Let

p = (p _{1,p} _{2,...,p} _{s),} q = (q _{1,q} _{2,...,q} _{s),} be the canonical coordinates of a s-dimensional Hamiltonian system, and letH( p , q ;V) = K( p ) + \varphi( q ;V)

be the Hamiltonian function, where

K = \sum ^{s} _{i =1} (p ^{2} _{i})/(2 m) ,

is the kinetic energy and

\varphi( q ;V)

is the potential energy which depends on a parameter

V .Let the hyper-surfaces of constant energy in the 2s-dimensional phase space of the system be metrically indecomposable and let \left\langle ⋅ \right\rangle _{t} denote time average. Define the quantities E , P , T , S , as follows:E = K + \varphi ,T = (2)/(s) \left\langle K\right\rangle _{t} ,P = \left\langle - (\partial \varphi)/(\partial V) \right\rangle _{t} ,S(E,V) = log \int _{H(p,q;V)} d ^{spd} ^{s} q .

Then:

dS = (dE + PdV)/(T) .

References

• Helmholtz, H., von (1884a). Principien der Statik monocyklischer Systeme. Borchardt-Crelle’s Journal für die reine und angewandte Mathematik, 97, 111–140 (also in Wiedemann G. (Ed.) (1895) Wissenschafltliche Abhandlungen. Vol. 3 (pp. 142–162, 179–202). Leipzig: Johann Ambrosious Barth).
• Helmholtz, H., von (1884b). Studien zur Statik monocyklischer Systeme. Sitzungsberichte der Kö niglich Preussischen Akademie der Wissenschaften zu Berlin, I, 159–177 (also in Wiedemann G. (Ed.) (1895) Wissenschafltliche Abhandlungen. Vol. 3 (pp. 163–178). Leipzig: Johann Ambrosious Barth).
• Boltzmann, L. (1884). Über die Eigenschaften monocyklischer und anderer damit verwandter Systeme.Crelles Journal, 98: 68–94 (also in Boltzmann, L. (1909). Wissenschaftliche Abhandlungen (Vol. 3, pp. 122–152), F. Hasenöhrl (Ed.). Leipzig. Reissued New York: Chelsea, 1969).
• Gallavotti, G. (1999). Statistical mechanics: A short treatise. Berlin: Springer.
• Campisi, M. (2005) On the mechanical foundations of thermodynamics: The generalized Helmholtz theorem Studies in History and Philosophy of Modern Physics 36: 275–290