Kinetic theory of gases Knowledge-Based Study

Physics · Thermal Physics · Physics · Thermodynamics

Physics topic explanations on Kinetic theory of gases.

Study notes

  1. Basic Postulates of Ideal Gases

    The kinetic theory of gases describes the macroscopic properties of gases—such as pressure and temperature—by considering their molecular composition and motion. The model of an ideal gas relies on several core postulates:

    • Point particles: A gas consists of a vast number of identical particles (atoms or molecules) whose individual volumes are negligible compared to the total volume occupied by the gas.
    • Continuous random motion: Particles move continuously in straight paths at varying speeds and in random directions, obeying Newton's laws of motion.
    • Negligible intermolecular forces: There are no attractive or repulsive forces between particles, except during brief collisions.
    • Elastic collisions: All collisions between particles and with the container walls are perfectly elastic; total kinetic energy and linear momentum are conserved.
    • Duration of collisions: The time duration of any collision is negligible compared to the time spent between collisions.

    How Molecular Collisions Produce Pressure

    Macroscopic pressure arises from the continuous impacts of gas particles against the walls of their container. When a particle of mass mm moving with velocity component vxv_x strikes a perpendicular wall elastically, its velocity reverses to −vx-v_x.

    The change in linear momentum per collision is:

    Δpx=−mvx−mvx=−2mvx\Delta p_x = -mv_x - mv_x = -2mv_x

    By Newton's third law, the impulse delivered to the wall is +2mvx+2mv_x. Summing the collisions of NN particles in a volume VV over time and taking the isotropic average of velocities in three dimensions (v2‾=vx2‾+vy2‾+vz2‾=3vx2‾\overline{v^2} = \overline{v_x^2} + \overline{v_y^2} + \overline{v_z^2} = 3\overline{v_x^2}), the macroscopic pressure PP is expressed as:

    P=13NmVv2‾=13ρv2‾P = \frac{1}{3}\frac{N m}{V}\overline{v^2} = \frac{1}{3}\rho \overline{v^2}

    where ρ\rho is the gas density and v2‾\overline{v^2} is the mean square speed of the particles.

    Thermal Energy at the Molecular Scale

    Combining the microscopic pressure relation with the ideal gas law PV=NkBTPV = N k_B T establishes a direct link between absolute temperature and the average translational kinetic energy of gas molecules:

    PV=13Nmv2‾=NkBTPV = \frac{1}{3} N m \overline{v^2} = N k_B T

    Multiplying both sides by 32N\frac{3}{2N} yields the average translational kinetic energy per particle, Ek‾\overline{E_k}:

    Ek‾=12mv2‾=32kBT\overline{E_k} = \frac{1}{2}m\overline{v^2} = \frac{3}{2}k_B T

    Here, kBk_B is the Boltzmann constant (1.38×10−23 J/K1.38 \times 10^{-23}\text{ J/K}) and TT is the absolute temperature in kelvins. This fundamental result reveals that absolute temperature is a direct measure of the average translational kinetic energy of the molecules, independent of the chemical identity or mass of the gas.

    Root-Mean-Square Speed

    Because particles within a gas collide continuously, their speeds are distributed across a wide range described by the Maxwell-Boltzmann distribution. To represent the typical speed of a particle, physics commonly employs the root-mean-square speed (vrmsv_{\text{rms}}), defined as the square root of the mean squared speed:

    vrms=v2‾=3kBTm=3RTMv_{\text{rms}} = \sqrt{\overline{v^2}} = \sqrt{\frac{3k_B T}{m}} = \sqrt{\frac{3RT}{M}}

    where RR is the universal gas constant (8.314 J/(mol⋅K)8.314\text{ J/(mol}\cdot\text{K)}) and MM is the molar mass of the gas in kilograms per mole.

    Key implications include:

    • At a given temperature, gases with lower molar mass (e.g., helium or hydrogen) have significantly higher vrmsv_{\text{rms}} than heavier gases (e.g., oxygen or carbon dioxide).
    • Doubling the absolute temperature increases vrmsv_{\text{rms}} by a factor of 2≈1.41\sqrt{2} \approx 1.41, not by a factor of two.

    Internal Energy and Departures from Ideal Behavior

    For a monatomic ideal gas, intermolecular potential energy is zero. Consequently, the total internal energy UU consists entirely of the translational kinetic energy of all nn moles of gas:

    U=N(32kBT)=32nRTU = N \left(\frac{3}{2}k_B T\right) = \frac{3}{2}nRT

    For polyatomic gases, internal energy also includes rotational and vibrational modes according to the equipartition theorem.

    When Does the Ideal Gas Model Break Down?

    Real gases deviate noticeably from kinetic theory predictions under conditions of:

    • High pressure: The volume occupied by the molecules themselves is no longer negligible compared to the container volume.
    • Low temperature: Molecular speeds decrease, making attractive intermolecular forces significant enough to pull molecules together, eventually leading to liquefaction.