DOFPro Team

The Enthalpy Games: The Ballad of Integrals and Means discusses how internal energy and enthalpy vary as functions of \(T\) and \(P\).
The Enthalpy Games: Sunrise on the Calculations
does a worked example using nitrogen and data from NIST.
Internal Energy is important for closed systems at constant volume
Enthalpy is important for open systems and closed systems at constant pressure
The ability to evaluate \(\Delta H\) and \(\Delta U\) is important for many 1st-Law problems.
Remember: \(\Delta\) means final – initial or out – in.
State Variable: Value depends only on location or “state.” Does not depend on path.
Common State Variables: \(H\), \(T\), \(U\), \(V\), \(m\), etc.
Path Variable: Value depends only on path. Does not depend on location.
Common Path Variables: \(Q\), \(W\).
Example: Calculate \(\Delta H\) for one mole of ice at \(-5\ ^\circ \mathrm{C}\) and \(1\ \mathrm{bar}\) being changed to steam at \(300\ ^\circ \mathrm{C}\) and \(5\ \mathrm{bar}\) by two different paths.
Path 1:
For the process \(\Delta \hat{H} = \sum\limits_{i=1}^6 \Delta \hat{H}_i\)
Path 2:
For the process \(\Delta \hat{H} = \sum\limits_{i=1}^3 \Delta \hat{H}_i\)
Are the two equal?
Why or why not?
For many chemical engineering processes, work, kinetic energy, and potential energy can be ignored. In such cases the 1st law reduces to:
\(\hspace{160px}Q = \Delta U\) (Closed System)
\(\hspace{160px}\dot{Q} = \Delta \dot{H}\) (Open System)
For a constant volume system we define:
\(\hspace{160px}C_v(T) \equiv \lim\limits_{\Delta T \rightarrow 0} \dfrac{\Delta \hat{U}}{\Delta T} = \dfrac{d\hat{U}}{dT}\)
\(C_v\) is the heat capacity at constant volume.
Rearranging
\(\hspace{160px}d\hat{U} = C_v (T) dT\)
and integrating
\(\hspace{160px}\Delta \hat{U} = \displaystyle\int\limits_{T_1}^{T_2} C_v (T) dT\)
If \(C_v\) does not depend on \(T\), then:
\(\hspace{160px}\Delta \hat{U} = C_v \Delta T\)
What if the volume changes?
For a constant pressure system we define:
\(\hspace{160px}C_p(T) \equiv \lim\limits_{\Delta T \rightarrow 0} \dfrac{\Delta \hat{H}}{\Delta T} = \dfrac{d\hat{H}}{dT}\)
\(C_p\) is the heat capacity at constant pressure. As before
\(\hspace{160px}d\hat{H} = C_p (T) dT\)
and integrating
\(\hspace{160px}\Delta \hat{H} = \displaystyle\int\limits_{T_1}^{T_2} C_p (T) dT\)
If \(C_p\) does not depend on \(T\), then:
\(\hspace{160px}\Delta \hat{H} = C_p \Delta T\)
What if the pressure changes?
In general:
\(\hspace{160px}d\hat{H} = C_p (T) dT + \left[\hat{V} - T \left(\dfrac{\partial \hat{V}}{\partial T}\right)_P\right] dP\)
Ideal Gas:
\(\hspace{160px}\Delta \hat{H} = \displaystyle\int\limits_{T_1}^{T_2} C_p (T) dT\) No pressure dependence
Liquids and Solids:
\(\hspace{160px}\Delta \hat{H} = \displaystyle\int\limits_{T_1}^{T_2} C_p (T) dT + \displaystyle\int\limits_{P_1}^{P_2} \hat{V} dP \approx \displaystyle\int\limits_{T_1}^{T_2} C_p (T) dT + \hat{V} \Delta P\)
How do \(C_p\) and \(C_v\) compare?
Ideal Gas: \(C_p = C_v + R\)
Liquids and Solids: \(C_p \approx C_v\)
How do you evaluate heat capacities?
Mean Heat Capacity
The only reason to calculate an average heat capacity is if someone asks for it.
Definition: \(\bar{C}_p \equiv \dfrac{\hat{H}_2 - \hat{H}_1}{T_2 - T_1}\)
Evaluation:
\[\bar{C}_p = \frac{\int\limits_{T_1}^{T_2}(a + b T + c T^2 + d T^3 + \dfrac{e}{T^2})dT}{T_2 - T_1}\]
which evaluates to
\[\begin{align} \bar{C}_p = a &+ \frac{b}{2} (T_1+T_2) + \frac{c}{3} (T_1^2 +T_1T_2 +T_2^2) \\&+ \frac{d}{4} [(T_1+T_2)(T_1^2+T_2^2)] + \dfrac{e}{T_1T_2} \end{align}\]
It should be obvious that
\(\hspace{80px}\Delta \hat{H} = \bar{C}_p \Delta T\)
but things in thermodynamics rarely are.
The actually useful symbolic integration of the correlations for \(C_p\) is to calculate \(\Delta \hat{H}\) directly.
\[\Delta \hat{H} = \int\limits_{T_1}^{T_2} C_p (T) dT = \int\limits_{T_1}^{T_2} (a + b T + c T^2 + d T^3 + \dfrac{e}{T^2})dT\]
\[\begin{align} \Delta \hat{H}=\ &a (T_2 - T_1) + \frac{b}{2} (T_2^2 - T_1^2) + \frac{c}{3} (T_2^3 - T_1^3) \\&+ \frac{d}{4} (T_2^4 - T_1^4) + e \left(\frac{1}{T_1} - \frac{1}{T_2}\right) \end{align}\]
If you have the formula for \(C_p(T)\) it is much easier to evaluate
\(\hspace{120px}\Delta \hat{H} = \int\limits_{T_1}^{T_2} C_p (T) dT\hspace{80px}\) than to evaluate
\(\hspace{120px}\bar{C}_p = \dfrac{\int\limits_{T_1}^{T_2} C_p (T) dT}{T_2 - T_1}\hspace{80px}\) followed by \(\hspace{80px}\Delta \hat{H} = \bar{C}_p \Delta T\).
\(\hspace{120px}\Delta \hat{U}_\text{ideal gas} = \int\limits_{T_1}^{T_2} \left[C_p (T) - R \right] dT\)
\(\hspace{120px}\Delta \hat{U}_\text{solid,\ liquid} \approx \int\limits_{T_1}^{T_2} C_p (T) dT\)
In The Enthalpy Games: Sunrise on the Calculations, we do a worked example using nitrogen and data from NIST.
Thanks for watching!
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