A special case of the grand canonical ensemble

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SUMMARY

This discussion focuses on the application of the grand partition function in the context of an Einstein Solid, specifically under conditions where internal energy (U) is constant and the number of particles (N) is large. The participants explore the definitions of chemical potential (μ) and temperature (T) as outlined in equations (1) and (2), and their relevance in calculating the average value of N using the grand partition function. Key equations include the grand partition function Q(α, β) and the expression for μ derived from Schroeder's "An Introduction to Thermal Physics". The final form of μ is established as μ = -kT(q/N), confirming its applicability in this scenario.

PREREQUISITES
  • Understanding of grand canonical ensemble concepts
  • Familiarity with Einstein Solid model and its properties
  • Knowledge of statistical thermodynamics, particularly partition functions
  • Proficiency in mathematical manipulation of thermodynamic equations
NEXT STEPS
  • Study the derivation and applications of the grand partition function in statistical mechanics
  • Explore the implications of the Einstein Solid model on thermodynamic properties
  • Learn about the relationship between chemical potential and temperature in various ensembles
  • Review M. Bellac's "Equilibrium and non-Equilibrium Statistical Thermodynamics" for deeper insights
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Students and researchers in physics, particularly those specializing in statistical mechanics and thermodynamics, as well as educators seeking to enhance their understanding of the grand canonical ensemble and its applications.

Ted Ali
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Homework Statement
Can we consider the internal energy ##U## constant and only allow for the number of particles ##N## to vary, in the grand canonical ensemble?
Relevant Equations
$$\mu = -T \left(\frac{\partial S}{\partial N}\right)_{U,V} \hspace{1cm} (1)$$
$$\frac{1}{T} = \left(\frac{\partial S}{\partial U} \right) \hspace{1cm} (2)$$
In addition to the homework statement and considering only the case where ##U= constant## and ##N = large## : Can we also consider the definition of chemical potential ##\mu## and temperature ##T## as in equations ##(1)## and ##(2)##, and use them in the grand partition function?

More specifically, we can take the case of an Einstein Solid and the Schroeder's definition of internal energy ##U = qhf##. Assuming that ##U## is depending only on a constant number of energy quanta ##q## and allowing only ##N## to vary. Can we use the grand partition function and ##(1), (2)##, for calculating the average value of ##N##? In this case of an Einstein Solid, we also assume that ##N \gg q##.

The grand partition function is given by: $$Q_{(\alpha, \beta)} = \sum_{N=0}^{\infty} e^{\alpha N} Z_{N}(\alpha, \beta) \hspace{1cm} (3)$$
And: $$\bar{N} =\left( \frac{\partial\ln{Q}}{\partial \alpha}\right)_\beta \hspace{1cm} (4)$$
Where: $$\beta = \frac{1}{kT} \hspace{1cm} \alpha = \frac{\mu}{kT} \hspace{1cm} (5)$$
$$Z_1 = 1/ (1 - e^{-\frac{hf}{kT}})\hspace{1cm}(6)$$
And: $$Z_N = (Z_1)^N \hspace{1cm}(7)$$
Under the above conditions and equations:
$$\mu = -kT\frac{q}{N} = \frac{kT}{1 - e^{hf/kT}}\hspace{1cm} (8)$$
 
Last edited:
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Temperature ##T## is given by equation ##(2)##, in the microcanonical ensemble and calculated in Wikipedia (https://en.wikipedia.org/wiki/Einstein_solid). The final result is: $$\frac{q}{N} = \frac{1}{e^{hf/kT} - 1}\hspace{1cm} (9)$$
The chemical potential ##\mu## is given by ##(1)##, when ##U, V## are held constant. The calculation of ##(1)## can be found in the solutions manual of D. Schroeder's book: "An Introduction to Thermal Physics". The final result is $$\mu = -kT\ln(1+ \frac{q}{N})\hspace{1cm} (10)$$ (exercise 3.36).
In the case we examine it is assumed that ##N \gg q## so ##(10)## becomes: $$\mu = -kT\frac{q}{N}\hspace{1cm} (11)$$
From ##(9)## and ##(11)## we have equation ##(8)##, in its final form.
Finally let's comment that in ##(6)##, we have neglected the ground state energy of each one quantum harmonic oscillator of the Einstein solid, in the calculation of the canonical partition function (https://en.wikipedia.org/wiki/Einstein_solid). And that in ##(7)## we have assumed that the oscillators are distinguishable.
Equations ##(3), (4), (5)## come from M. Bellac's book: "Equilibrium and non-Equilibrium Statistical Thermodynamics", pg. 148.
So the "sum" of the questions still remains open: Can we use ##(8)## in the grand partition function?
 
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