Mean free path

Mean free path

Vishal kumarUpdated on 02 Jul 2025, 06:35 PM IST

The mean free path is a fundamental concept in physics that describes the average distance a particle travels before colliding with another particle. This concept is crucial in understanding the behaviour of gases, where molecules are in constant motion and frequently collide with one another. In simpler terms, the mean free path helps us predict how far a molecule can move freely without interruption. In real life, the mean free path can be related to everyday experiences, such as walking through a crowded room. Imagine navigating through a bustling crowd; the distance you can move freely before bumping into someone is akin to the mean free path. Similarly, in the air we breathe, the molecules of gases like oxygen and nitrogen move in all directions, with their paths continuously interrupted by collisions, determining the overall properties of the gas, such as pressure and temperature. Understanding the mean free path is essential for applications ranging from designing efficient engines to predicting atmospheric phenomena.

This Story also Contains

  1. Mean Free Path
  2. Solved Examples Based on Mean Free Path
  3. Summary

Mean Free Path

On the basis of the kinetic theory of gases, it is assumed that the molecules of a gas are continuously colliding against each other. So, the distance travelled by a gas molecule between any two successive collisions is known as the free path.

There are assumptions for this theory that during two successive collisions, a molecule of a gas moves in a straight line with constant velocity. Now, let us discuss the formula of the mean free path.

Let $\lambda_1, \lambda_2 \ldots \ldots \lambda_n$ be the distance travelled by a gas molecule during n collisions respectively, then the mean free path of a gas molecule is defined as

$\lambda=\frac{\text { Total distance travelled by a gas molecule between successive collisions }}{\text { Total number of collisions }}$

Here, $\lambda$ is the mean free path.

It can also be written as $\lambda=\frac{\lambda_1+\lambda_2+\lambda_3+\ldots+\lambda_n}{n}$

Now, let us take d = Diameter of the molecule,
N = Number of molecules per unit volume.

Also, we know that, PV = nRT

So, Number of moles per unit volume = $\frac{n}{V}=\frac{P}{R T}$

Also, we know that the number of molecules per unit mole $=N_A=6.023 \times 10^{23}$

So, the number of molecules in 'n' moles = nNA

So the number of molecules per unit volume is $N=\frac{P N_A}{R T}$
So, $\lambda=\frac{\text { RT }}{\sqrt{2} \pi \mathrm{d}^2 \mathbf{P N}_{\mathrm{A}}}=\frac{\mathrm{kT}}{\sqrt{2} \pi \mathrm{d}^2 \mathbf{P}}$

If all the other molecules are not at rest then, $\quad \lambda=\frac{1}{\sqrt{2} \pi N d^2}=\frac{R T}{\sqrt{2} \lambda d^2 \mathrm{PN}_{\mathrm{A}}}=\frac{\mathrm{kT}}{\sqrt{2} \pi \mathrm{d}^2 \mathrm{P}}$

Now, if $\lambda=\frac{1}{\sqrt{2} \pi N d^2}$ and m = mass of each molecule then we can write $\lambda=\frac{1}{\sqrt{2} \pi N d^2}=\frac{m}{\sqrt{2} \pi(m N) d^2}=\frac{m}{\sqrt{2} \pi d^2 \rho}$

So, $\lambda \propto \frac{1}{\rho}$ and $\lambda \propto m$

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Solved Examples Based on Mean Free Path

Example 1: For a diatomic gas, the ratio of two specific heat Cp/Cv is equal to

1) 1.66

2) 1.4

3) 1.28

4) 2

Solution:

Value of degree of freedom for diatomic gas

$
f=5
$

So
$
\begin{aligned}
& \frac{C_p}{C_v}=1+\frac{2}{f} \\
& \frac{C_p}{C_v}=1+\frac{2}{5}=\frac{7}{5}
\end{aligned}
$

Hence, the answer is the option (2).

Example 2: The molecules of an ideal gas at 270 C have a mean velocity $v$. At what temperature (in oC) will the mean velocity be $\frac{3}{2} v$?

1) 350

2) 450

3) 402

4) 315

Solution:

The mean velocity of the gas molecule is

$
\bar{v}=\sqrt{\frac{8 R T}{\pi M}}
$
for same gas
$
\begin{aligned}
& \bar{v}=\sqrt{T} \\
& \frac{\overline{v_1}}{\overline{v_2}}=\sqrt{\frac{T_1}{T_2}}=\sqrt{\frac{(273+27)}{T_2}} \\
& \frac{2 v}{3 v}=\sqrt{\frac{300}{T_2}} \Rightarrow \frac{300}{T_2}=\frac{4}{9} \\
& \quad T_2=\frac{2700}{4}=675 \mathrm{~K} \\
& 675-373=402^{\circ} \mathrm{C}
\end{aligned}
$

Hence, the answer is the option (3).

Example 3: For a triatomic ( non-linear) gas, the total no. of degrees of freedom is

1) 4

2) 6

3) 7

4) 5

Solution:

Value of degree of freedom for triatomic gas

$f=6$

A triatomic gas can have three translational degrees of freedom and three rotational degrees of freedom.

3(translational) + 3(rotational) = 6

Hence, the answer is the option (2).

Example 4: For monoatomic gas, the incorrect statement is:

(i) It has all translational degrees of freedom

(ii) examples He, H2, Ne

(iii) It can have a maximum of 6 degrees of freedom 3 translational and 3 rotational

1) Only (ii)

2) only (i)

3) (ii) and (iii)

4) (i) and (iii)

Solution

Value of degree of freedom for monoatomic gas

$f=3$

wherein

A monoatomic gas can only have a translational degree of freedom.

* H2 is an example of a diatomic gas

* monoatomic gas can have a maximum of three degrees of freedom and is all translational.

Hence, the answer is the option of (3).

Example 5: Which statement is true for the term degree of freedom?

(i) Monatomic gas has all translational degrees of freedom

(ii) There can be a maximum of two rotational degrees of freedom

(iii) Total degree of freedom is of three types

1) (i), (ii), (iii)

2) (i) and (ii)

3) (i) and (iii)

4) (ii) and (iii)

Solution:

Degree of freedom

It is the number of directions in which a particle can move freely or the number of independent coordinates required to describe the system completely.

It is denoted by $f$.

$\begin{aligned} & f=3 N-R \\ & N=n o . \text { of particle } \\ & R=\text { no. of relation }\end{aligned}$

* monatomic gas has only three degrees of freedom and is all translational.

* Total degree of freedom is of three types

(i) Translational

(ii) Rotational

(iii) Vibrational

Hence, the answer is the option (3).

Summary

The mean free path is the average distance a gas molecule travels between collisions, crucial in understanding gas behaviour. It is calculated using the formula $\lambda=\frac{\mathrm{RT}}{\sqrt{2} \pi d^2 \mathrm{PN}_A}$, where $\lambda$ is the mean free path, $d$ is the molecule's diameter, and $N$ is the number of molecules per unit volume This concept is foundational in predicting gas properties, like pressure and temperature, and is essential in various scientific and engineering applications.

Frequently Asked Questions (FAQs)

Q: How does the mean free path of gas molecules in the upper atmosphere contribute to the escape of gases from Earth?
A:
In the upper atmosphere, the mean free path becomes very long due to low density. This allows some high-energy molecules, especially of lighter gases like hydrogen and helium, to travel long distances without collisions, potentially reaching escape velocity and leaving Earth's atmosphere, contributing to atmospheric loss over geological time scales.
Q: Can mean free path explain why some gases are more suitable for use in certain types of lasers?
A:
Yes, mean free path is relevant in gas laser design. Gases with appropriate mean free paths allow for efficient excitation and de-excitation processes while maintaining suitable pressure for population inversion. This affects laser power output and efficiency.
Q: How does the concept of mean free path relate to the efficiency of catalytic converters?
A:
In catalytic converters, mean free path influences reaction efficiency. A balance is needed: shorter mean paths increase collision frequency with catalyst surfaces, but extremely short paths may hinder gas flow. Understanding this helps optimize converter design for effective pollutant reduction.
Q: What's the relationship between mean free path and the effectiveness of gas chromatography?
A:
Mean free path affects gas chromatography performance. Longer mean free paths in the carrier gas can lead to better separation efficiency as analyte molecules have more opportunity to interact with the stationary phase between collisions with carrier gas molecules.
Q: How does the mean free path of gas molecules affect the design of vacuum insulated panels?
A:
In vacuum insulated panels, reducing the mean free path of remaining gas molecules is crucial. By lowering pressure and sometimes introducing materials with small pores, the mean free path is decreased to less than the panel thickness, minimizing heat transfer through gas conduction and convection.
Q: What's the significance of mean free path in understanding gas adsorption processes?
A:
In gas adsorption, mean free path affects how gas molecules interact with surfaces. Longer mean free paths can result in fewer collisions with the adsorbent surface, potentially reducing adsorption rates, which is important in applications like gas storage and purification.
Q: Can mean free path explain why some gases are more easily compressed than others?
A:
Yes, mean free path contributes to gas compressibility. Gases with longer mean free paths are generally easier to compress initially because there's more "empty space" between molecules. However, as compression increases, the mean free path decreases, and further compression becomes more difficult.
Q: How does the mean free path of gas molecules affect the formation of shock waves?
A:
Mean free path influences shock wave formation. In regions where the gas velocity changes rapidly over distances comparable to the mean free path, the usual continuum flow assumptions break down, contributing to the formation and structure of shock waves.
Q: How does the concept of mean free path relate to the efficiency of thermal insulation materials?
A:
Mean free path is important in thermal insulation. Materials that effectively reduce the mean free path of gas molecules (like aerogels or foam insulations) are good insulators because they limit heat transfer through the gas phase by increasing the number of collisions required for energy transfer.
Q: Can the mean free path concept help explain the behavior of gases in interstellar space?
A:
Yes, mean free path is crucial in understanding interstellar gas behavior. In the extremely low densities of space, mean free paths can be enormous, leading to unique gas behaviors where collisions are rare and gravitational effects become more significant in determining gas distribution and movement.