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Modern Engineering Thermodynamics

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758 CHAPTER 18: Introduction to Statistical <strong>Thermodynamics</strong><br />

EXAMPLE 18.10 (Continued )<br />

Exercises<br />

28. Note that the only property of a polytropic Maxwell-Boltzmann gas that depends on pressure is entropy. Compute the<br />

entropy for the carbon dioxide in Example 18.10 if the pressure is increased from 1.00 to 10.0 atm. Assume all other<br />

variables remain unchanged. Answer: s = 5.68 kJ/kg·K (s trans = 3.68 kJ/kg·K, s rot = 1.47 kJ/kg·K, s vib = 0.528 kJ/kg·K).<br />

29. Recompute the specific internal energy, enthalpy, and entropy of the carbon dioxide in Example 18.10 when the<br />

temperature is lowered from 1000. K to 300. K but the pressure remains constant at 1.00 atm. Answer: u = 841 kJ/kg<br />

(u trans = 85.0 kJ/kg, u rot = 56.7 kJ/kg, u vib = 699 kJ/kg); h = 898 kJ/kg; s = 4.86 kJ/kg·K (s trans = 3.55 kJ/kg·K,<br />

s rot = 1.24 kJ/kg·K, s vib = 0.0694 kJ/kg·K).<br />

30. Determine the specific internal energy, enthalpy, and entropy of the carbon dioxide in Example 18.10 for a temperature<br />

of 5000. K and a pressure of 0.100 atmosphere. Answer: u = 6190 kJ/kg (u trans = 1420 kJ/kg, u rot = 945 kJ/kg, u vib =<br />

3832 kJ/kg); h = 7138 kJ/kg; s = 8.72 kJ/kg·K (s trans = 5.31 kJ/kg·K, s rot = 1.78 kJ/kg·K, s vib = 1.64 kJ/kg·K).<br />

The nonlinear polyatomic molecule has 3 translational degrees of freedom, 3 rotational degrees of freedom, and<br />

3b−6 degrees of vibrational freedom. Thus, it has the same equations for the translational molecular energy as<br />

in the linear polyatomic case, but the rotational and vibrational contribution equations are different. In this<br />

case,<br />

u rot = h rot = 3 2 RT<br />

(18.57a)<br />

ðc v Þ rot = ðc p Þ rot = 3 2 R<br />

n<br />

s rot = R ln½T/ðσ Θ r ÞŠ+ 3 o<br />

2<br />

(18.57b)<br />

(18.57c)<br />

and<br />

u vib = ðu o Þ vib<br />

+ R∑ 3b−6<br />

i=1<br />

h vib = u vib = ðu o Þ vib<br />

+ R∑ 3b−6<br />

ðc v Þ vib = R∑ 3b−6<br />

i=1<br />

Θ vi / ½expðΘ vi /TÞ−1Š (18.58a)<br />

i=1<br />

Θ vi / ½expðΘ vi /TÞ−1Š (18.58b)<br />

ðΘ vi /TÞ 2 ½expðΘ vi /TÞŠ/ ½expðΘ vi /TÞ−1Š 2 (18.58c)<br />

and<br />

ðc p Þ vib<br />

= ðc v Þ vib<br />

+ R∑ 3b−6<br />

i=1<br />

ðΘ vi /TÞ 2 ½expðΘ vi /TÞŠ/ ½expðΘ vi /TÞ−1Š 2 (18.58d)<br />

s vib = R∑ 3b−6<br />

i=1<br />

<br />

ln ½1 − expð−Θ vi /TÞŠ −1 + ðΘ vi /TÞ½expðΘ vi /TÞ−1<br />

where the vibrational internal energy at absolute temperature is now found from<br />

Š −1<br />

(18.58e)<br />

3b−6<br />

ðu o Þ vib = ∑ RΘ vi /2 (18.59)<br />

since the nonlinear polyatomic molecule has 3b−6 characteristic vibrational temperatures Θ vi .<br />

SUMMARY<br />

The subject of statistical thermodynamics is inherently mathematically complex and conceptually difficult. It is<br />

often the subject of an entire advanced engineering course, usually at the graduate level. The material presented<br />

in this chapter is intended only as an introduction to this subject.<br />

i=1

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