Question 8.14: An isolated system consists of two rigid subsystems of volum...

An isolated system consists of two rigid subsystems of volumes V_1 and V_2 separated by a rigid and porous membrane. Helium (He) can diffuse through the membrane, but oxygen (O_2) cannot. We label the gases as A for helium and B for oxygen. The whole system is in thermal equilibrium at all times. Each gas can be considered an ideal gas, i.e. they satisfy the equations of state (5.46) and (5.47), namely, p V = NR T and U = c N R T. The gas mixture obeys the ideal mixture relation (8.68), that is,

U = 3 N R T                               (5.46)

p V = N R T                                (5.47)

μ_A (T, p, c_A) = μ_A (T, p) + R T \ln (c_A)                 (8.68)

μ_A (T, p, c_A) = μ_A (T, p) + R T \ln (c_A)

 

μ_B (T, p, c_B) = μ_B (T, p) + R T \ln (c_B)

where μ_A (T, p) and μ_B (T, p) are the chemical potentials of substances A and B when they are pure, c_A and c_B are the concentrations of A and B. Initially, the system contains N_0 moles of helium in subsystem 1, and N_B moles of oxygen in subsystem 2 (Fig. 8.2). The numbers of moles N_0 and N_B are chosen so that the initial pressure p_i is the same in both subsystems. At all times, each subsystem is assumed to be homogeneous. Designate by N_1 and N_2 the number of moles of helium in subsystems 1 and 2, respectively.

a) At equilibrium, show that μ_A (T, p_1) = μ_A (T, p_2, c_A).
b) Deduce from the previous result a relation between the pressures p_1 and p_2 when the two sub-systems reach equilibrium. Express c_A, p_1 and p_2 in terms of N_2. Determine p_1 and p_2 in terms of the initial pressure pi under the condition of equal volume, i.e. V_1 = V_2 = V_0.

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a) Applying Gibbs’ relation (2.12) to the helium in each subsystem yields,

\dot{U} = T \dot{S} – p \dot{V} + \sum\limits_{A=1}^{r}{\mu _A \dot{N}_A }            (2.12)

\dot{U}_1 = T \dot{S}_1 + μ_1 \dot{N}_1       and    \dot{U}_2 = T \dot{S}_2 + μ_2 \dot{N}_2 .

which implies that,

\dot{S} = \dot{S}_1 + \dot{S}_2 = \frac{1}{T} (\dot{U}_1 +\dot{U}_2) – \frac{μ_1}{T}\dot{N}_1 – \frac{μ_2}{T}\dot{N}_2 .

Since the system is isolated \dot{U} = 0 , which implies that \dot{U}_1 = − \dot{U}_2 . The helium conservation law implies that \dot{N}_1 = −\dot{N}_2 . Thus,

\dot{S} = \frac{μ_1 − μ_2}{T} \dot{N}_1 .

and equivalently,

\frac{∂S}{∂N_1} = \frac{μ_1 − μ_2}{T} .

According to the second law, the total entropy S of the system reaches a maximum at equilibrium. Thus, at equilibrium,

\frac{∂S}{∂N_1} = 0 .    (equilibrium)

which implies that μ_1 ≡ μ_A (T, p_1) is equal to μ_2 ≡ μ-A (T, p_2, c_A) ,

μ_A (T, p_1) = μ_A (T, p_2, c_A)          (equilibrium)

b) Using the ideal mixture relation (8.68),

μ_A (T, p, c_A) = μ_A (T, p) + R T \ln (c_A)                 (8.68)

μ_A (T, p_2, c_A) = μ_A (T, p_2) + R T \ln (c_A) .

which implies that at chemical equilibrium,

μ_A (T, p_1) = μ_A (T, p_2) + RT \ln (c_A) .

Moreover, according to relation (8.58),

μ (T, p) = μ (T, p_0) + R T \ln \Bigl(\frac{p}{p_0}\Bigr) .       (8.58)

μ_A (T, p_1) = μ_A (T, p_2) + R T \ln \Bigl(\frac{p_1}{p_2}\Bigr) .

Comparing the two previous relations and using the definition of the concentration c_A ,we obtain,

c_A = \frac{p_1}{p_2}       and      c_A = \frac{N_2}{N_2 + N_0} .

The ideal gas equation of state implies that,

p_1 = \frac{(N_0 − N_2) R T}{V_0}       and    p_2 = \frac{(N_0 + N_2) R T}{V_0} .

Using the last four equations, we obtain,

N_2=\frac{N_0}{2}.

Thus,

p_1 = \frac{N_0 R T}{2 V_0}        and    p_2 = \frac{3 N_0 R T}{2 V_0} .

Moreover, since,

p_i = \frac{N_0 R T}{ V_0} .

we have that,

p_1 = \frac{1}{2} p_i         and      p_2 = \frac{3}{2} p_i .

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