What is the significance of the grand partition function in an Einstein solid?

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The grand partition function for an Einstein solid is expressed as Q(α, β) = ∑(N=0 to ∞) e^(αN) Z_N(α, β), where Z_N is the canonical partition function. In this context, the number of oscillators N and the total quanta of energy q are significant, particularly when q is much greater than N. The calculations indicate that the logarithm of the grand partition function simplifies to ln(Q) ≈ ln(C/q) + ln(N), leading to an average particle number of N̄ = 1. The discussion raises questions about the nature of q as a constant versus a variable, the necessity of an upper bound for N, and the applicability of chemical potential derivations in different statistical ensembles. Overall, the significance of the grand partition function lies in its ability to describe the statistical properties of the system under consideration.
Ted Ali
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Homework Statement
Calculate the average number of oscillators of an Einstein solid, in the grand canonical ensemble, when q>>N. N is the number of oscillators and q the total number of energy quanta.
Relevant Equations
I am quoting from "Equilibrium and non-Equilibrium Statistical Thermodynamics", by M. Bellac.
$$Q_{(\alpha, \beta)} = \sum_{N=0}^{\infty} e^{\alpha N} Z_{N}(\alpha, \beta) \hspace{1cm} (3.127)$$ $$\beta = \frac{1}{kT} \hspace{1cm} \alpha = \frac{\mu}{kT} \hspace{1cm} (3.128)$$ $$\bar{N} = \frac{\partial{\ln Q}}{\partial \alpha} \hspace{1cm} (3.129)$$
$$q >> N \rightarrow q \approx 10^z N, z \geq 2$$
In this case: $$\mu = -kT\ln(\frac{q}{N}) \hspace{1cm} (1)$$ Reference: Daniel V. Schroeder, An Introduction to Thermal Physics,
(Addison-Wesley, 2000) - Problems 3.35 - 3.36.
$$Z_{N} = \frac{N}{2 \sinh(\frac{hf}{2kT})} = N\cdot C \hspace{1cm} (2)$$
$$Q_{(\alpha, \beta)} = \sum_{N=0}^{\infty} e^{\alpha N} Z_{N}(\alpha, \beta) \hspace{1cm} (3.127)$$
Where ##Q## is the grand partition function, ##Z_N## is the canonical partition function and:
$$\beta = \frac{1}{kT} \hspace{1cm} \alpha = \frac{\mu}{kT} \hspace{1cm} (3.128)$$
In the case of an Einstein solid, ##N## is the number of oscillators and ##q## the total quanta of energy. We are interested in the case: $$q >> N \rightarrow q \approx 10^z N, z \geq 2$$ In this case: $$\mu = -kT\ln(\frac{q}{N}) \hspace{1cm} (1)$$ Reference: Daniel V. Schroeder, An Introduction to Thermal Physics,
(Addison-Wesley, 2000) - Problems 3.35 - 3.36.
From https://en.wikipedia.org/wiki/Einstein_solid, we get: $$Z_{N} = \frac{N}{2 \sinh(\frac{hf}{2kT})} = N\cdot C \hspace{1cm} (2)$$
Where $$C = \frac{1}{2\sinh(\frac{hf}{2kT})} \hspace{1cm} (3)$$
##C## depends only on ##\beta##. Substituting in ##(3.127)##, we get:
$$Q = C \cdot \sum_{N=0}^{\infty} e^{\alpha N} \cdot N = C \cdot \sum_{N=0}^{\infty} e^{\ln((\frac{N}{q})^N)} \cdot N = $$ $$ = C \cdot \sum_{N=0}^{\infty} N (\frac{N}{q})^N \hspace{1cm} (4)$$
Since ##q >> N##, (4) becomes:
$$Q \cong \left(C\cdot \frac{N}{q}\right) \Rightarrow$$ $$ \Rightarrow \ln{Q} \cong \ln{\frac{C}{ q}} + \ln{N} \hspace{1cm} (5)$$

Quoting ##(3.129)##: $$\bar{N} = \frac{\partial{\ln{Q}}}{\partial \alpha} = \frac{\partial{\ln{Q}}}{\partial N}\cdot \frac{1}{\frac{\partial \alpha}{\partial N}} = \frac{\frac{1}{N}}{\frac{1}{N}} \Rightarrow$$ $$\Rightarrow \bar{N} = 1 \hspace{1cm} (6)$$
I would like you to let me know of my errors in calculations, comments, etc. If I am correct in my calculations, is it equilibrium or non-equilibrium statistics? How about ##\Delta N##, when we start from ##N \approx 10^{10}##?
 
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The main question is whether ##q## should be considered a constant, or else, dependent on every value ##N## takes, in the sum.
 
Should ##N## have an upper bound other than infinity? Should we consider an interaction between systems (instead of the isolated Einstein solid), governed by the grand canonical ensemble? Is the derivation of the chemical potential ##(\mu)## in the microcanonical ensemble, not applicable in the case of the grand canonical ensemble?
 
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