Estimating the final pressure of a transformation

Click For Summary
SUMMARY

The final pressure of 1.0 mol of an ideal gas undergoing a transformation from (1.0 atm, 300 K) to (pfinal, 600 K) is determined to be 4 atm, assuming the Helmholtz Free Energy remains constant. The analysis utilizes the equations A = U - TS and dA = -SdT - pdV, with the initial entropy S0 set to R. The solution confirms that if Cp/R equals 2, the relationship holds, although this ratio is not physically realistic for common gases.

PREREQUISITES
  • Understanding of Helmholtz Free Energy and its implications in thermodynamics
  • Familiarity with the equations A = U - TS and dA = -SdT - pdV
  • Knowledge of ideal gas behavior and the significance of Cp and Cv
  • Basic concepts of entropy and its calculation for ideal gases
NEXT STEPS
  • Explore the derivation of the Helmholtz Free Energy and its applications in thermodynamic processes
  • Study the relationship between Cp, Cv, and the ideal gas law
  • Investigate the implications of constant entropy in thermodynamic transformations
  • Learn about the physical characteristics of mono-atomic and diatomic gases and their specific heat ratios
USEFUL FOR

Students and professionals in thermodynamics, particularly those studying ideal gas behavior, thermodynamic transformations, and the application of the Helmholtz Free Energy in real-world scenarios.

thaalescosta
Messages
11
Reaction score
0

Homework Statement


If the Helmholtz Free Energy remains constant, estimate the final pressure of 1.0mol of an ideal gas in the following transformation: (1.0atm, 300k) → (pfinal, 600k). Given Sgas = R.

Homework Equations


A = U - TS
dA = -SdT - pdV

The Attempt at a Solution


If the Helmholtz Free Energy is constant, then ΔA = 0.

So from dA = -SdT - pdV I'd get that S⋅ΔT = -pΔV.

But I don't see how that helps me figuring out the final pressure.
 
Physics news on Phys.org
I think they meant for you to assume that the initial value of S for the gas is R (S0=R). If this is the case then, in terms of pfinal and ##C_p## what is Sfinal? What is ##\Delta (TS)##? In terms of ##C_p##, what is ##\Delta U##? What is ##\Delta A##?

Is the gas mono-atomic?
 
Last edited:
Chestermiller said:
I think they meant for you to assume that the initial value of S for the gas is R (S0=R). If this is the case then, in terms of pfinal and ##C_p## what is Sfinal? What is ##\Delta (TS)##? In terms of ##C_p##, what is ##\Delta U##? What is ##\Delta A##?

Is the gas mono-atomic?
It did not specify if the gas is mono-atomic nor did it give me the Cp or Cv values.

It only asks me to find the final pressure, which is 4 atm.
 
thaalescosta said:
It did not specify if the gas is mono-atomic nor did it give me the Cp or Cv values.

It only asks me to find the final pressure, which is 4 atm.
OK. Then please set up the equations as I suggested in post #2, and let's see where that takes us. I'm confident that this is the correct approach to use.
 
thaalescosta said:
It did not specify if the gas is mono-atomic nor did it give me the Cp or Cv values.

It only asks me to find the final pressure, which is 4 atm.
My solution to this problem gives 4 atm. if Cp/R=2. This is the same as gamma = 2. It don't think that there are any gases with this ratio, however.

Chet
 
Chestermiller said:
My solution to this problem gives 4 atm. if Cp/R=2. This is the same as gamma = 2. It don't think that there are any gases with this ratio, however.

Chet
You're right.

My solution was making ΔA = 0 and then setting SdT = - pdV.

Since S = R:
- SdT = (1/V)*nRT⋅dV
- dT = (1/V)*nT⋅dV (and n = 1)
- dT/T = (1/V)dV
- ln(T2/T1) = ln(V2/V1)
- ln(2) = ln(V2/V1)
1/2 = V2/V1
V1 = 2V2

(P1⋅V1)/T1 = (P2⋅V2)/T2
(1 atm ⋅2V2)/300 = (P2 ⋅ V2)/600K
P2 = 4 atm
 
I didn't assume that R was constant throughout the change. I assumed that only the initial value of S was equal to R.

For the final entropy I got:
$$S_2=R+C_p\ln(T_2/T_1)-R\ln(P_2/P_1)$$
So, ##\Delta (TS)## was:
$$\Delta (TS)=R(T_2-T_1)+C_pT_2\ln(T_2/T_1)-RT_2\ln(P_2/P_1)$$
For the change in internal energy, I got:$$\Delta U=C_v(T2-T_1)=(C_p-R)(T2-T_1)=C_p(T2-T_1)-R(T2-T_1)$$
So, $$\Delta A=\Delta U-\Delta (TS)=(C_p-2R)(T2-T_1)+C_pT_2\ln(T_2/T_1)-RT_2\ln(P_2/P_1)$$
Setting ##\Delta A## equal to zero and solving for ##\ln(P_2/P_1)##, we get:
$$\ln(P_2/P_1)=\frac{C_p}{R}\ln(T_2/T_1)+\left(2-\frac{C_p}{R}\right)\left[1-\frac{T_1}{T_2}\right]$$
Only if ##\frac{C_p}{R}=2## does the second term on the right vanish, and do we obtain $$\frac{P_2}{P_1}=\left(\frac{T_2}{T_1}\right)^2=4$$
But, even for a mono-atomic gas, ##\frac{C_p}{R}>2##.
Our two analyses are consistent with one another only of ##\frac{C_p}{R}=2##. That's the only way that S can be constant throughout the change.

In my opinion, this is a pretty hinky problem.
 
Last edited:
Here is a simpler analysis of the situation. If the entropy is constant at a value of R, then the change in free energy is given by:
$$\Delta A=C_v(T_2-T_1)-R(T_2-T_1)=(C_v-R)(T_2-T_1)$$
The only way this can be zero is if ##C_v=R##.

The change in entropy for an ideal gas is given by:$$\Delta S=C_p\ln(T_2/T_1)-R\ln(P_2/P_1)$$
But, if ##\Delta S = 0##, we have:
$$C_p\ln(T_2/T_1)=R\ln(P_2/P_1)$$
But, if ##C_v=R##, then ##C_p=2R##
So, $$\ln(P_2/P_1)=2\ln(T_2/T_1)$$
But, for all this to hold together, we must have that ##C_v=R##, which is physically unrealistic.
 

Similar threads

Replies
9
Views
3K
  • · Replies 16 ·
Replies
16
Views
3K
Replies
5
Views
4K
Replies
3
Views
2K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 2 ·
Replies
2
Views
3K
Replies
2
Views
2K
Replies
12
Views
2K
Replies
3
Views
11K