Undergrad Exceptions to the postulate of equal a priori probabilities?

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SUMMARY

The discussion centers on the fundamental postulate of equal a priori probabilities in statistical physics, which asserts that all accessible microstates in an ensemble occur with equal probability. It highlights significant exceptions, particularly in systems like coupled oscillators that can become "stuck" in metastable states, where energy does not distribute evenly across degrees of freedom immediately. The conversation emphasizes that while equal a priori probabilities are often assumed for practical purposes, they must be derived from the system's dynamics, especially in integrable systems where non-trivial initial conditions do not lead to thermal states.

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  • Understanding of statistical physics principles
  • Familiarity with microcanonical and canonical ensembles
  • Knowledge of metastable states and their implications
  • Basic concepts of dynamical systems and integrable systems
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  • Research the Fermi–Pasta–Ulam–Tsingou problem and its implications for statistical mechanics
  • Study the derivation of equal a priori probabilities from dynamical systems
  • Explore the characteristics of thermal states in closed chaotic systems
  • Investigate the differences between microcanonical and canonical ensembles in detail
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AndreasC
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Not sure if this is the appropriate forum for this, hopefully if it isn't someone can move it to a more appropriate place.

The fundamental postulate of equal a priori probabilities in statistical physics asserts that all accessible microstates states in an ensemble happen with equal probability. It is an important assumption for proving a number of important results, like the form of the partition functions in microcanonical and canonical ensembles etc. My question is, are there any significant cases that statistical physics still deals with where equal a priori probabilities can not be assumed and other assumptions have to be made?
 
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For instance, there's this system of coupled oscillators that can get "stuck" in some part of energy-allowed phase space and the energy doesn't partition to all degrees of freedom until some time has passed.

https://en.wikipedia.org/wiki/Fermi–Pasta–Ulam–Tsingou_problem

But this kind of things are something that would probably be called "metastable states" in statistical physics terminology.
 
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In general, equal apriori probabilities are not a postulate but must be derived from the dynamics. However, in all but the most simple cases, this is mathematically very difficult and rarely of practical importance. Thus, this problem is usually sidestepped and the probabilities are just postulated. This is fine in practice, but you have to keep in mind that such a postulate is not independent of the dynamics and could in principle contradict it. Integrable systems are a typical example for this situation. E.g., in the two-body problem, no non-trivial set of initial conditions will lead to a thermal state if you just wait long enough.
 
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Nullstein said:
This is fine in practice, but you have to keep in mind that such a postulate is not independent of the dynamics and could in principle contradict it.
Yeah, this has been my understanding so far, that's why I was interested in examples where this can't be assumed.
Nullstein said:
no non-trivial set of initial conditions will lead to a thermal state if you just wait long enough.
How is a thermal state defined? Furthermore, can equal probabilities be assumed in all such states?
 
AndreasC said:
How is a thermal state defined? Furthermore, can equal probabilities be assumed in all such states?
Typically, a closed, sufficiently chaotic system is expected to have a microcanonical ensemble as equilibrium distribution, which is just an equal probability distribution on a constant energy surface (or constant integrals of motion surface, more generally). An open subsystem that can exchange energy will then typically end up in a canonical ensemble. The canonical ensemble has this constant energy only on avergage, with configurations closer to this constant energy surface being more likely.
 
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Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?

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