Canonical ensemble Definition and 58 Threads

In statistical mechanics, a canonical ensemble is the statistical ensemble that represents the possible states of a mechanical system in thermal equilibrium with a heat bath at a fixed temperature. The system can exchange energy with the heat bath, so that the states of the system will differ in total energy.
The principal thermodynamic variable of the canonical ensemble, determining the probability distribution of states, is the absolute temperature (symbol: T). The ensemble typically also depends on mechanical variables such as the number of particles in the system (symbol: N) and the system's volume (symbol: V), each of which influence the nature of the system's internal states. An ensemble with these three parameters is sometimes called the NVT ensemble.
The canonical ensemble assigns a probability P to each distinct microstate given by the following exponential:




P
=

e

(
F

E
)

/

(
k
T
)


,


{\displaystyle P=e^{(F-E)/(kT)},}
where E is the total energy of the microstate, and k is Boltzmann's constant.
The number F is the free energy (specifically, the Helmholtz free energy) and is a constant for the ensemble. However, the probabilities and F will vary if different N, V, T are selected. The free energy F serves two roles: first, it provides a normalization factor for the probability distribution (the probabilities, over the complete set of microstates, must add up to one); second, many important ensemble averages can be directly calculated from the function F(N, V, T).
An alternative but equivalent formulation for the same concept writes the probability as





P
=


1
Z



e


E

/

(
k
T
)


,



{\displaystyle \textstyle P={\frac {1}{Z}}e^{-E/(kT)},}
using the canonical partition function





Z
=

e


F

/

(
k
T
)





{\displaystyle \textstyle Z=e^{-F/(kT)}}
rather than the free energy. The equations below (in terms of free energy) may be restated in terms of the canonical partition function by simple mathematical manipulations.
Historically, the canonical ensemble was first described by Boltzmann (who called it a holode) in 1884 in a relatively unknown paper. It was later reformulated and extensively investigated by Gibbs in 1902.

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  1. M

    How Can I Calculate Internal Energy Using Grand Canonical Ensemble Method?

    Homework Statement To calculate internal energy for a system of non interacting S.H.O's in 1 dimension at constant T & u(chem potential) using grand partition function The Attempt at a Solution L(Grnd prtition fn)= Summation(z^N)*[Z(TVN)] where z = fugacity , Z = partition fn of...
  2. P

    Canonical Ensemble: Partition Function & Free Energy

    Is it true that partition function for canonical ensemble is Z=\sum_{\{states j\}}e^{-\beta E_j}=e^{-\beta F} where F is Helmholtz free energy?
  3. E

    Canonical Ensemble Homework: Equal Probabilities Postulate

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  4. J

    How Does the Grand Canonical Ensemble Determine Site Atom Occupancy?

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  5. T

    Derivation of Grand Canonical Ensemble from scratch?

    I've been studying and thinking about statistical physics for a couple days now... and what bothers me is the grand canonical partition function. Namely that for a system with fixed chemical potential and energy \epsilon_i the probability of having N_i particle in that state is proportional to...
  6. R

    Please help me to derive canonical ensemble

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  7. R

    How to Write a Canonical Ensemble for a System Using the Einstein Model

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  8. S

    When Should You Use the Grand Partition Function in Statistical Mechanics?

    I am taking a statictical mechanics course, and one thing bothers me. I am not sure when we should use the normal partition function (Z) and when the grand partition function (twisty Z). In particular, why can we not use grand partition function when we are considering the following system...
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