Categories:
Physics,
Thermodynamic ensembles,
Thermodynamics.
Grand canonical ensemble
The grand canonical ensemble or μVT ensemble
extends the canonical ensemble
by allowing the exchange of both energy U and particles N
with an external reservoir,
so that the conserved state functions are
the temperature T, the volume V, and the chemical potential μ.
The derivation is practically identical to that of the canonical ensemble.
We refer to the system of interest as A,
and the reservoir as B.
In total, A+B has energy U and population N.
Let cB(UB) be the number of B-microstates with energy UB.
Then the probability that A is in a specific microstate sA is as follows:
p(s)=∑sAcB(U−UA(sA),N−NA(sA))cB(U−UA(sA),N−NA(sA))
Then, as for the canonical ensemble,
we assume UB≫UA and NB≫NA,
and approximate lnp(sA)
by Taylor-expanding lncB around UB=U and NB=N.
The resulting probability distribution is known as the Gibbs distribution,
with β≡1/(kT):
p(sA)=Z1exp(−β(UA(sA)−μNA(sA)))
Where the normalizing grand partition function Z(μ,V,T) is defined as follows:
Z≡sA∑exp(−β(UA(sA)−μNA(sA)))
In contrast to the canonical ensemble,
whose thermodynamic potential
was the Helmholtz free energy F,
the grand canonical ensemble instead
minimizes the grand potential Ω:
Ω(T,V,μ)≡−kTlnZ=⟨UA⟩−TSA−μ⟨NA⟩
So Z=exp(−βΩ).
This is proven in the same way as for F in the canonical ensemble.
References
- H. Gould, J. Tobochnik,
Statistical and thermal physics, 2nd edition,
Princeton.