10.2 Kinetic theory of gases

3 min readjuly 23, 2024

Gases are made up of tiny particles zipping around randomly. Kinetic theory explains how these particles behave, creating pressure and temperature. It's like a microscopic game of bumper cars, where molecules bounce off each other and container walls.

The theory links pressure, volume, and temperature through the law. It also shows how molecular speed relates to temperature. Understanding these connections helps us predict gas behavior in various situations, from weather balloons to car tires.

Kinetic Theory of Gases

Postulates of kinetic theory

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  • Gas consists of a large number of molecules in constant random motion
    • Molecules move rapidly in straight lines until they collide with other molecules or container walls ()
    • Collisions between molecules are perfectly elastic, is conserved during collisions (billiard balls)
  • Molecules are treated as point masses with negligible volume compared to the container
    • The volume occupied by the molecules themselves is much smaller than the volume of the container (ping pong balls in a room)
  • No attractive or repulsive forces exist between molecules, except during collisions
    • Molecules do not exert any long-range forces on each other, they only interact during brief collisions (people in a large crowd)
  • The average kinetic energy of molecules is proportional to the absolute temperature
    • As temperature increases, molecules move faster and have higher average kinetic energy (hot air balloon rising)

Relationships in kinetic theory

  • Pressure is caused by molecular collisions with the container walls
    • P=13nmv2P = \frac{1}{3}nm\overline{v^2}, where nn is the number density, mm is the molecular mass, and v2\overline{v^2} is the average of the square of the molecular velocity
    • More collisions or higher velocity collisions result in higher pressure (tire pressure increasing with temperature)
  • Ideal gas law: [PV = nRT](https://www.fiveableKeyTerm:pv_=_nRT), where PP is pressure, VV is volume, nn is the number of moles, RR is the universal gas constant, and TT is the absolute temperature
    • The ideal gas law relates pressure, volume, temperature, and amount of gas (weather balloon expanding as it rises)
  • Kinetic energy is directly proportional to absolute temperature
    • 12mv2=32kT\frac{1}{2}m\overline{v^2} = \frac{3}{2}kT, where kk is the and TT is the absolute temperature
    • Higher temperature means higher average molecular kinetic energy (faster molecule movement in boiling water vs room temperature water)

Velocity and energy of gas molecules

  • Root mean square (rms) velocity: vrms=v2=3RTMv_{rms} = \sqrt{\overline{v^2}} = \sqrt{\frac{3RT}{M}}, where RR is the universal gas constant, TT is the absolute temperature, and MM is the molar mass
    • RMS velocity is a measure of the average speed of molecules in a gas (speedometer for gas molecules)
  • Average kinetic energy: KE=12mv2=32kT\overline{KE} = \frac{1}{2}m\overline{v^2} = \frac{3}{2}kT, where mm is the molecular mass, kk is the Boltzmann constant, and TT is the absolute temperature
    • The average kinetic energy of gas molecules depends on temperature and mass (heavier molecules move slower at the same temperature)

Maxwell-Boltzmann velocity distribution

  • The describes the probability distribution of molecular velocities in an ideal gas at thermal equilibrium
    • Gives the fraction of molecules with a specific velocity at a given temperature (bell curve of molecular speeds)
  • The distribution depends on temperature and molecular mass
    • Higher temperatures result in a broader distribution and higher average velocities (faster molecules in hot gas)
    • Heavier molecules have a narrower distribution and lower average velocities compared to lighter molecules at the same temperature (oxygen vs hydrogen gas at room temperature)
  • The most probable velocity (vpv_p), average velocity (v\overline{v}), and root mean square velocity (vrmsv_{rms}) can be calculated from the distribution
    1. Most probable velocity: vp=2RTMv_p = \sqrt{\frac{2RT}{M}} (peak of the bell curve)
    2. Average velocity: v=8RTπM\overline{v} = \sqrt{\frac{8RT}{\pi M}} (average of all molecular speeds)
    3. Root mean square velocity: vrms=3RTMv_{rms} = \sqrt{\frac{3RT}{M}} (square root of the average of the squared velocities)

Key Terms to Review (16)

Boltzmann Constant: The Boltzmann constant is a fundamental physical constant that relates the average kinetic energy of particles in a gas with the temperature of that gas. It plays a crucial role in statistical mechanics, linking macroscopic properties like temperature to microscopic behaviors of particles. This constant is vital in various fields such as kinetic theory, quantum mechanics, and thermodynamics, emphasizing the connection between energy, temperature, and probability distributions.
Brownian motion: Brownian motion refers to the random, erratic movement of microscopic particles suspended in a fluid (liquid or gas) caused by collisions with the fast-moving molecules of the surrounding medium. This phenomenon is significant in understanding the behavior of gases and their molecular interactions, showcasing how temperature and pressure influence particle dynamics and energy distribution.
Diffusion: Diffusion is the process by which particles spread from areas of high concentration to areas of low concentration due to random motion. This phenomenon is a fundamental concept in understanding how substances interact in various systems, impacting energy distribution and equilibrium. The movement of molecules during diffusion occurs until a uniform concentration is achieved, playing a crucial role in gas behavior and non-equilibrium processes.
Effusion: Effusion is the process by which gas particles escape through a tiny hole into a vacuum or another space without collisions between the particles. This phenomenon is closely linked to the kinetic theory of gases, which describes how gas particles are in constant motion and how their speed affects their ability to escape. Understanding effusion helps explain the behavior of gases under different conditions and their rate of escape based on their molecular weight.
Elastic Collisions: Elastic collisions are interactions between particles where both momentum and kinetic energy are conserved. This type of collision is significant in understanding the behavior of gases, as it helps explain how gas molecules interact without losing energy, allowing for predictable outcomes in thermodynamic processes. In these collisions, after the interaction, the total kinetic energy of the system remains the same as before the collision, which is a fundamental principle in the kinetic theory of gases.
Gas particles: Gas particles are the individual molecules or atoms that make up a gas, moving freely and rapidly in all directions. These particles have significant amounts of kinetic energy, which allows them to collide with each other and the walls of their container, influencing the gas's pressure and temperature. Their behavior is fundamental to understanding the kinetic theory of gases, which explains how these particles interact and the resulting macroscopic properties of gases.
Ideal gas: An ideal gas is a theoretical gas composed of many particles that are in constant random motion and interact with one another only through elastic collisions. The behavior of an ideal gas is described by the ideal gas law, which connects pressure, volume, temperature, and number of moles, allowing for predictions of gas behavior under various conditions. The concept of an ideal gas helps simplify the analysis of real gases by providing a baseline model that can be compared against more complex behaviors observed in actual gases.
Kinetic Energy: Kinetic energy is the energy possessed by an object due to its motion, calculated using the formula $$KE = \frac{1}{2}mv^2$$, where $$m$$ is mass and $$v$$ is velocity. This form of energy plays a vital role in understanding how energy is conserved and transferred in systems, impacting the behavior of gases and their interactions.
Maxwell-Boltzmann Distribution: The Maxwell-Boltzmann distribution describes the statistical distribution of speeds of particles in a gas at thermal equilibrium. This distribution illustrates how the velocities of gas molecules are spread out, with most molecules having speeds around the average, while few have very high or very low speeds. Understanding this distribution is crucial for interpreting entropy, explaining gas behavior, and connecting to more complex statistical distributions like the Fermi-Dirac distribution.
Mean free path: Mean free path is the average distance a particle travels between successive collisions with other particles. This concept is central to the kinetic theory of gases, as it helps explain how gas molecules behave and interact with each other under various conditions, such as temperature and pressure. Understanding mean free path provides insight into the properties of gases, including viscosity and thermal conductivity.
Pressure and Volume: Pressure is defined as the force exerted per unit area, while volume refers to the amount of space that a substance occupies. These two terms are deeply interconnected, especially in the context of gases, where changes in one can directly affect the other due to their relationship described by gas laws. Understanding pressure and volume is crucial for grasping how gases behave under different conditions, including changes in temperature and the amount of gas present.
Pv = nRT: The equation $$pv = nRT$$ is known as the ideal gas law, which relates the pressure (p), volume (v), and temperature (T) of an ideal gas, with n representing the number of moles and R being the ideal gas constant. This relationship is fundamental in understanding the behavior of gases under various conditions. The equation provides a way to predict how changing one of these variables will affect the others, thereby giving insights into the kinetic energy and molecular motion of gas particles.
Real gas: A real gas is a gas that does not behave ideally and deviates from the predictions of the ideal gas law due to intermolecular forces and the volume occupied by gas particles. In contrast to an ideal gas, which assumes no interactions between particles and that they occupy no volume, real gases exhibit behaviors influenced by their molecular characteristics, especially under high pressure and low temperature conditions.
Rms speed: Rms speed, or root mean square speed, is a statistical measure of the speed of particles in a gas that reflects their average kinetic energy. It provides an effective means of comparing the speeds of gas molecules, allowing us to understand how temperature and mass influence molecular motion within the framework of kinetic theory.
Temperature and Kinetic Energy: Temperature is a measure of the average kinetic energy of the particles in a substance, reflecting how fast those particles are moving. When we talk about kinetic energy in the context of temperature, we're focusing on the motion of atoms and molecules; higher temperatures indicate greater movement, which means increased kinetic energy. This relationship helps explain the behavior of gases, liquids, and solids as their temperatures change.
Thermal energy: Thermal energy is the internal energy present in a system due to the kinetic energy of its particles. It plays a crucial role in how energy is conserved and transformed within physical systems, influencing everything from temperature changes to phase transitions. Understanding thermal energy helps explain how energy moves and changes forms, as well as the behavior of gases at the molecular level.
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