Boltzmann vs. Gibbs entropy, negative energy

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Discussion Overview

The discussion revolves around the comparison between Boltzmann and Gibbs entropy, particularly in the context of their applicability to different statistical ensembles, including the microcanonical and canonical ensembles. Participants explore the definitions, implications, and potential limitations of these entropy formulations, as well as their relevance to small systems and negative absolute temperatures.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants express skepticism about the dominance of Boltzmann entropy over Gibbs entropy in the physics community, suggesting that Boltzmann's definition has its problems.
  • There is a discussion about the definitions of microcanonical and canonical ensembles, with references to the standard definitions of entropy in these contexts.
  • Participants mention the von Neumann entropy as a quantum generalization of Gibbs entropy, noting that it does not initially involve temperature.
  • Some argue that the Gibbs entropy can be derived from a specific density operator, while others question the equivalence of different definitions of entropy proposed in the literature.
  • Concerns are raised about the applicability of the canonical ensemble to small systems, with references to recent literature suggesting alternative definitions of entropy that may be more suitable.
  • There is a suggestion that the authors of a referenced paper may be proposing a new definition of entropy, termed "Gibbs entropy" or "Hertz entropy," which could address issues faced by the traditional Boltzmann-Gibbs-Shannon-von Neumann entropy.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the superiority or applicability of Boltzmann versus Gibbs entropy. Multiple competing views remain regarding the definitions and contexts in which each entropy is most appropriate, particularly concerning small systems and the implications of negative absolute temperatures.

Contextual Notes

Limitations include unresolved questions about the definitions of entropy in different ensembles and the implications of using various density operators. The discussion also highlights the dependence on specific assumptions regarding system size and energy constraints.

  • #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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