Kinetic Theory and Pressure
The kinetic theory of gases provides a microscopic explanation for the macroscopic behavior of gases, such as pressure and temperature.
Origin of Pressure in a Gas
- Pressure arises from the collisions of gas molecules with the walls of their container.
- Each collision exerts a force on the wall, and the cumulative effect of countless collisions results in pressure.
Pressure is defined as the force exerted per unit area: $$P = \frac{F}{A}$$
Deriving the Pressure Equation
- To relate pressure to molecular motion, consider a cube of side $L$ containing $N$ molecules, each of mass $m$.
- Assume the molecules move randomly with an average speed $v$.
This derivation assumes an ideal gas, where molecules are point particles that undergo elastic collisions and experience no intermolecular forces.
- Momentum Change in a Collision:
- A molecule moving with velocity $v_x$ along the x-axis collides elastically with a wall.
- Before the collision, its momentum is $mv_x$, after the collision, it is $-mv_x$.
- The change in momentum is $2mv_x$.
- Time Between Collisions:
- The molecule travels a distance $2L$ (to the wall and back) in time $t = \frac{2L}{v_x}$.
- Force Exerted by the Molecule:
- The average force exerted on the wall is given by the rate of change of momentum: $$F = \frac{2mv_x}{\frac{2L}{v_x}} = \frac{mv_x^2}{L}$$
- Total Pressure from All Molecules:
- For $N$ molecules, the total pressure is the sum of the forces exerted by each molecule.
- Using the root mean square speed $v_{\text{rms}}$, where $v_{\text{rms}}^2 = \frac{v_1^2 + v_2^2 + \ldots + v_N^2}{N}$, the pressure is: $$P = \frac{1}{3} \rho v_{\text{rms}}^2$$
- Here, $\rho = \frac{Nm}{V}$ is the density of the gas.
The factor $\frac{1}{3}$ arises because the molecules move in three dimensions, and only one-third of their velocity contributes to motion along any single axis.
Internal Energy of an Ideal Gas
Internal energy
Internal energy is the sum of kinetic energy and potential energy of a substance and is the result of the motion of the particles which make up the substance.
The internal energy of an ideal gas is the total kinetic energy of its molecules.
For a monatomic ideal gas, this energy depends only on temperature.
Expression for Internal Energy
The internal energy $U$ of an ideal gas is given by:
$$U = \frac{3}{2} Nk_B T \quad \text{or} \quad U = \frac{3}{2} nRT$$
where:
- $N$ is the number of molecules.
- $n$ is the number of moles.
- $k_B$ is the Boltzmann constant ($1.38 \times 10^{-23} \, \text{J K}^{-1}$).
- $R$ is the universal gas constant ($8.31 \, \text{J K}^{-1} \text{mol}^{-1}$).
- $T$ is the absolute temperature in kelvin.
- In an ideal gas, internal energy is purely kinetic.
- There is no potential energy because intermolecular forces are negligible.
Calculate the internal energy of 2 moles of helium gas at $300 \, \text{K}$.
Solution
Using $U = \frac{3}{2} nRT$:
$$U = \frac{3}{2} \times 2 \, \text{mol} \times 8.31 \, \text{J K}^{-1} \text{mol}^{-1} \times 300 \, \text{K} = 7,479 \, \text{J}$$
Real vs. Ideal Gases
While the ideal gas model is useful, real gases deviate from this behavior under certain conditions.
Conditions for Ideal Gas Behavior
Ideal gases follow the assumptions of the kinetic theory, which include:
- Molecules are point particles with negligible volume.
- No intermolecular forces exist except during collisions.
- Collisions are perfectly elastic.
- Real gases approximate ideal behavior at low pressure and high temperature.
- Under these conditions, molecules are far apart, and intermolecular forces are minimal.
Deviations from Ideal Behavior
Real gases deviate from ideal behavior under high pressure or low temperature.
- High Pressure:
- Molecules are closer together, so their volume becomes significant.
- Intermolecular forces (e.g., van der Waals forces) become more pronounced.
- Low Temperature:
- Molecules move more slowly, increasing the influence of attractive forces.
- Gases may liquefy, violating the ideal gas assumption of no intermolecular forces.
- At very low temperatures, nitrogen gas can liquefy, demonstrating strong deviations from ideal behavior.
- This occurs because the kinetic energy of the molecules is insufficient to overcome intermolecular attractions.
- How does the kinetic theory explain the origin of pressure in a gas?
- What is the relationship between the internal energy of an ideal gas and its temperature?
- Under what conditions do real gases deviate from ideal behavior?


