Can a Super Grand Canonical Ensemble Exist?

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Discussion Overview

The discussion revolves around the concept of a "Super Grand Canonical Ensemble," which proposes a modification to the traditional grand canonical ensemble by allowing pressure to be a fixed parameter while volume fluctuates. Participants explore the implications and existence of this ensemble within the framework of statistical mechanics.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant suggests defining a "Super Grand Canonical Ensemble" where pressure is the parameter and volume is allowed to fluctuate, questioning the absence of such an ensemble.
  • Another participant claims that this ensemble exists but lacks a widely recognized name, referencing its connection to the Gibbs Duhem relation and mentioning its use in certain texts on statistical mechanics.
  • A different participant points to specific literature, including Mandl's "Statistical Physics" and Landau's work, suggesting that the concept may be present under different terminology.
  • One participant expresses doubt about the existence of the super-grand-potential, arguing that it depends solely on intensive quantities and thus cannot be extensive, leading to the conclusion that it vanishes identically.

Areas of Agreement / Disagreement

Participants express differing views on the existence and terminology of the "Super Grand Canonical Ensemble." While some assert its existence and reference literature, others challenge the concept's validity and argue that it cannot be defined as an extensive quantity.

Contextual Notes

There are unresolved questions regarding the definitions and implications of the proposed ensemble, particularly concerning the nature of extensive versus intensive quantities and the relationship to existing thermodynamic potentials.

qbslug
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Can we take the grand canonical ensemble and then switch the roles of the thermodynamic conjugate variable pair (P, V) making P (pressure) the parameter and V (volume) the variable and allowing it to fluctuate in the system. The macrostate would then be defined by the pressure temperature and chemical potential allowing the variables of energy, number of particles and volume to fluctuate. We can call this the "Super Grand Canonical Ensemble".

Why is there no super grand canonical ensemble? Is it because in the grand canonical ensemble the volume is an imaginary boundary (and thus user defined anyway). Or perhaps the super grand canonical ensemble gives no new information or has no thermodynamic potential to work with? Why no concern for the switching the PV pair?
 
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This ensemble exists, but for some reason, it hasn't got a sticky name. I think it is often abbreviated as J or Omega. It's differential yields the Gibbs Duhem relation, i.e. it vanishes. Abrikosov, Gorkov, Dzyaloshinskii, Quantum field theoretical methods in statistical physics (2ed., Pergamon, 1965) make some use of it and I have it seen discussed also in other texts on statistical mechanics, however I don't remember where.
 
I think you 'll find it in Mandl's "Statistical Physics". Landau also uses Ω=-PV while Pathria sticks to PV.
 
I think I have been wrong. The potential Omega I had in mind is simply the grand potential. I believe the super-grand-potential doesn't exist for the following reason: It depends only on intensive quantities and thus cannot be an extensive quantity. In fact it vanishes identically. E.g. [tex]G=\sum_i \mu_i N_i[/tex] and forming [tex]G-\sum_i \mu_i N_i=0[/tex].
 

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