How is Work Calculated from Chemical Potential and ΔG in a Two-Chamber System?

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SUMMARY

The discussion focuses on calculating the work that can be harnessed from a two-chamber system with differing solute concentrations (1M and 0.5M) as it reaches equilibrium. The key equation derived is Work = ∫[RTln(C1-n)/(C2+n)]dn, integrated from n=0 to n=0.25, where C1 and C2 represent the initial concentrations. The relationship between chemical potential (μ) and free energy (G) is established through the equation μ = ∂G/∂n, emphasizing that μ is dependent on concentration but not directly on the number of moles when integrated under constant conditions. The discussion clarifies the integration process required to determine the change in free energy as solute moves between chambers.

PREREQUISITES
  • Understanding of chemical potential and its definition (μ = ∂G/∂n).
  • Familiarity with the concept of free energy (G) and its relationship to solute concentration.
  • Knowledge of integration techniques in calculus, particularly in the context of thermodynamic equations.
  • Basic principles of ideal solutions and their behavior in thermodynamics.
NEXT STEPS
  • Study the derivation of the chemical potential for ideal solutions, focusing on μ_i = G_i + RTln(x_i).
  • Learn about the implications of concentration gradients on chemical potential in multi-chamber systems.
  • Explore the mathematical techniques for integrating thermodynamic equations, particularly in relation to free energy changes.
  • Investigate the concept of equilibrium in chemical systems and how it affects work calculations.
USEFUL FOR

Chemistry students, chemical engineers, and researchers in thermodynamics who are looking to deepen their understanding of work calculations in systems with varying solute concentrations.

tahaha
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Homework Statement



Consider a container with two chambers of the same size separated by a fixed membrane in the middle (permeable only to the ideal solute, but not the solvent). One chamber initially contains 1M of solute, and the other contains 0.5M of solute.

Write an equation for the amount of work that could potentially be harnessed when the system goes from the initial condition to equilibrium.


Homework Equations



μ=∂G/∂n at constant temperature and pressure


The Attempt at a Solution



Some confusions that I have:

1. So the definition of the chemical potential of a species at constant temperature, pressure is ∂G/∂n.
When we try to find the total free energy G of the species, we integrate ∫dG=∫μdn. There is then an equation in my textbook saying that G=μn. It kinda makes sense, because it's like summing up the chemical potential (defined as G per molecule or per mole) in the system. But does this imply that μ does not depend on n? How can it depend on concentration while not depending on the number of moles?

2. The answer says Work=∫dG= ∫[RTln(C1-n)/(C2+n)]dn integrated from n=0 to n=0.25, where C1=1M and C2=0.5M.
Apparently, the chemical potential difference between the two chambers changes as the reaction proceeds and is dependent on n. But I don't quite get why we have to integrate it.

Most importantly, can someone please explain in detail the mathematical relationship between chemical potential and free energy (and how to get from one to the other)?
 
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tahaha said:
1. So the definition of the chemical potential of a species at constant temperature, pressure is ∂G/∂n.
When we try to find the total free energy G of the species, we integrate ∫dG=∫μdn. There is then an equation in my textbook saying that G=μn. It kinda makes sense, because it's like summing up the chemical potential (defined as G per molecule or per mole) in the system. But does this imply that μ does not depend on n? How can it depend on concentration while not depending on the number of moles?

∫μdn=μn if the integration path is for constant composition (or concentration c) pressure p and temperature T as μ(c, p,T) does not depend on n.
However, this is not the integration path taken in the second part of your answer.
 
An ideal solution is defined as one in which the chemical potential of each species, by analogy to the chemical potentials of species in an ideal gas, is given by μ_i=G_i+RT\ln x_i, where μi is the chemical potential of species i, Gi is the free energy of species i at the same temperature and pressure as the system, and xi is the mole fraction of species i in the solution. Apparently, there are a significant number of liquid solutions that approach this type of behavior. At final steady state equilibrium, there will be 0.75M solution on both sides of the membrane. Therefore, Δn=0.25 moles per liter will be removed from the high concentration chamber and transferred to the lower concentration chamber. The change in free energy for each chamber is the concentration-dependent chemical potential for that chamber integrated over the change in the moles of solute in that chamber.
 

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