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Physics Bootcamp

Section 27.8 Kinetic Theory Bootcamp

Exercises Exercises

Pressure in an Ideal Gas

1. Root Mean Squared Speed of a Helium Molecule.
Follow the link: Example 27.3.
2. Pressure from a Stream of Particles Striking on a Wall.
Follow the link: Example 27.4.
3. Pressure from a Stream of Particles Striking on a Wall and Sticking to the Wall.
Follow the link: Exercise 27.1.3.1.

Internal Energy and Degrees of Freedom

4. Number of Excited Modes in a Water Molecule.
Follow the link: Example 27.16.
5. Internal Energy of Monatomic and Diatomic Ideal Gasses.
Follow the link: Example 27.17.

Maxwell’s Distribution

6. Average Speed and RMS Speed of a Nitrogen Molecule.
Follow the link: Example 27.6.
7. (Calculus) Mean of the Maxwell’s Distribution.
Follow the link: Example 27.8.
8. (Calculus) Exploring Maxwell’s Distribution of Energy of Molecules.
Follow the link: Example 27.9.

Mean Free Path

9. Mean Free Path of an Ideal Gas Illustrated.
Follow the link: Example 27.12.
10. Mean Free Path, Mean Free Time, and Intermolecular Distance in Helium Gas.
Follow the link: Exercise 27.3.1.
11. Variation of Mean Free Path with Pressure, Temperature, Volume, Amount of Gas.
Follow the link: Exercise 27.3.2.
12. (Calculus) Exploring Distribution of Free Lengths.
Follow the link: Exercise 27.3.3.

Effusion

13. (Calculus) Reduction of Pressure in a Container due to Escaping Molecules by Effusion.
Follow the link: Example 27.18.

Water Vapor and Humidity

14. Partial Pressure of Water Vapor from Humidity.
Follow the link: Example 27.21.
15. Plotting Saturated Water Vapor Pressure Versus Temperature.
Follow the link: Exercise 27.7.2.

Miscellaneous

16. Mean Free Path from Distances Between Successive Collisions of a Molecule.
The mean free path is the average distance a molecule travels in-between collisions. In reality a molecule will travel different distances in-between collisions. Suppose a molecule of size 0.3 nm travels the following distances between collisions: 11 nm, 5 nm, 12 nm, 15 nm, 25 nm, 2 nm, 11 nm, 30 nm, 18 nm, 20 nm, 14 nm, 15 nm, 10 nm, 28 nm, 9 nm, 17 nm, 5 nm, 10 nm, 6 nm, 13 nm, 17 nm, 15 nm, 10 nm, 22 nm, 9 nm, 23 nm, 19nm, 4 nm, 15 nm, 12 nm, 10 nm, 16 nm, 11 nm.
(a) Find the mean free path from this data.
(b) What is the standard deviation of space between collisions from the mean free path?
(c) What is the most probable free length?
(d) What is the rms free length?
(e) Supposing, the temperature of the gas is 200 K and the pressure of the gas is 1 atm, what would be the diameter of molecules of the gas
Hint.
Use a data processing sofware such as Mathematica or Excel or Google Sheets.
Answer.
(a) - (d) See solution, (e) \(D = 0.66\text{ nm}\text{.}\)
Solution.
I typed up the data in Mathematica and used their statistical functions. (a) 14 nm, (b) 6.7 nm, (c) Most common function gave two most-commonly occurring number, 10 nm and 15 nm. When I drew the histogram I found that 10 nm has more data points clustered around it than 15 nm points. The most probable length will be 10 nm. (d) 15.4 nm.
(e) Using the formula for the mean free path we get
\begin{equation*} D = \sqrt{ \frac{k_B T}{\sqrt{2}\pi \lambda p}}. \end{equation*}
Now, you can put in the numbers given.
\begin{equation*} T = 200\ \text{K},\ \ p = 1.013\times 10^5\ \text{Pa}. \end{equation*}
This gives \(D = 0.66\text{ nm}\text{.}\)
17. Surface Temperature of a Star for Helium Atoms to Escape Gravitational Pull.
What should be the maximum temperature of a sun-sized star if Helium atoms cannot escape the gravitational pull of the star? Hint: Equate gravitational escape speed with the rms speed.
Hint.
Answer.
Solution.
The escape speed \(v_e\) of a body of mass \(m\) from a body of mass \(M\) and radius \(R\) is given by equating the kinetic energy to the negative of the potential energy.
\begin{equation*} \frac{1}{2} m v_e^2 = G_N \frac{M m}{R}. \end{equation*}
This gives
\begin{equation*} v_e = \sqrt{\frac{2G_N M }{R} }. \end{equation*}
The root-mean square speed of a molecule when in the environment of temperature \(T\) is
\begin{equation*} v_\text{rms} = \sqrt{\frac{3k_B T}{m}} \end{equation*}
Equating the two speeds will give the condition we seek in this problem.
\begin{equation*} \frac{3k_B T}{m} = \frac{2G_N M }{R} \end{equation*}
The temperature will be
\begin{equation*} T =\frac{2G_N Mm }{3 k_B R}. \end{equation*}
Now, we put in the following numbers.
\begin{align*} \amp M = 2\times 10^{30}\ \text{kg}\ \ \text{(Mass of Sun)}\\ \amp m = 4\times 10^{-3}\ \text{kg}/6.022\times 10^{23} \ \ \text{(Mass of one He atom)}\\ \amp R = 7.0\times 10^9 \ \text{m}\ \ \text{(Radius of Sun)}. \end{align*}
These give the following for \(T\text{.}\)
\begin{equation*} T = 9 \times 10^6 \ \text{K}. \end{equation*}
This temperature is much larger than the surface temperature of the Sun.