Boltzmann vs. Gibbs entropy, negative energy

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The discussion centers on the relevance of Gibbs and Boltzmann entropy in statistical mechanics, questioning the notion that the physics community has overlooked Gibbs entropy in favor of Boltzmann's. Participants highlight that while Boltzmann entropy is commonly used, Gibbs' definition is broader and encompasses Boltzmann's. The conversation delves into the applicability of these definitions in both microcanonical and canonical ensembles, noting that the von Neumann entropy serves as a quantum generalization of Gibbs entropy. There is contention over the authors' claims in a referenced paper regarding the validity of their proposed "Gibbs entropy" for small systems, with some asserting that traditional definitions remain more appropriate. The discussion concludes with skepticism about the derivation of the proposed entropy definitions from established principles.
  • #31
This call for universal redefinition of entropy of a closed system seems very strange to me too. For a typical system of thermodynamics enclosed in a box, the area of available phase space hypersurface will grow with energy (think of ideal gas). The old definition of entropy for most many-particle systems seems consistent with classical thermodynamics and is well motivated in probabilistic ideas (accessible states...)

For a system of states whose density of states decreases with energy, this standard definition gives entropy that does not grow with energy. For the authors this is somehow sign of a defect of the concept and they propose another definition of statistical entropy ##S_{new} (E)## that maintains monotonicity, and so they say is generally better.

But there is no theoretical justification for such requirement when the systems have decreasing density of states. It is not clear that such systems fall under the purview of classical thermodynamics at all. If not, it makes no sense to impose requirement of thermodynamic properties upon statistical entropy and it is better to stay with the old definition for its other well-known nice properties.

For example, take multi-level system ##\mu## with decreasing density of states ##D(E)## and highest energy ##E_h##.

The standard statistical entropy ##S(E)## decreases with energy for this system, and when the energy is ##E_h##, it is minimum. Now let us connect ##\mu## thermally to a large system ##B## with ordinary density of states (increasing with energy) and Boltzmann temperature ##T##. Since in equilibrium the total system will have such occupation probabilities as to maximize total multiplicity for total energy of the sum system, the ##\mu## system will most probably transfer some heat to ##B##, and itself fall down to lower average energy (and higher standard entropy).

In other words, the system ##\mu## behaves as universal source of heat, regardless of the temperature ##T## of the receptor. Such systems do not fall under classical thermodynamics. They do not have thermodynamic temperature (in the original sense).

It may be interesting to study such systems with methods of statistical physics, and even define some new statistical entropy concept and new temperature concept for them for convenience. It would not be the first case (consider how many entropies are there already). Perhaps it is even possible to use thermodynamic ##formalism## for closed collection of such systems.

But it seems doubtful that this necessitates change of the standard statistical entropy for systems it was originally designed for.
 

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