Simple Models of Matter and Boltzmann Factor

Gas Laws

When describing an ideal gas, the following assumptions are made:

  • Gas particles take up negligible volume
  • All collisions between particles and the walls of the container and each other are completely elastic
  • There are negligible forces between particles except during collisions
  • All particles of a particular gas are identical
  • The internal energy of the gas is entirely kinetic
  • Newton's laws of motion apply
  • Gravitational, electrostatic and Van de Waals forces can be ignored
  • The motion of all molecules is random
  • All molecules travel in straight lines
    The top three assumptions in bold are given explicitly in the specification.

Boyle's Law states that for a constant temperature, the volume of a fixed mass of gas is inversely proportional to its pressure:

Avogadro's Law states that for a constant pressure and temperature, the volume of a gas is directly proportional to the number of moles:

Temperature is a measure of the average kinetic energy of the particles in a substance. Due to the random nature of collisions between particles in a gas, there is a distribution of speeds, and therefore kinetic energies of particles. The range of speeds are represented by the Maxwell Boltzmann distribution.

Charles' Law states that for a constant pressure, the volume of a fixed mass of gas is directly proportional to its absolute temperature:

For in Kelvin (K).

By combining these laws, we get:
Where is the ideal gas constant, with a value of .

The Boltzmann Constant is similar to the gas constant, , but only for one particle. It is equal to the gas constant divided by , the Avogadro constant:

By combining with , we get: , so we can rewrite the ideal gas equation as:

At a constant temperature, the distribution of speeds will remain the same, as well as the average speed. The root mean square speed is:

Temperature of a gas is proportional to the average kinetic energy of its particles:

For monatomic particles (and one dimension), a simple estimation is often used:

Gas Law Derivation

Consider a particle of mass moving at velocity in a cubic box with side length .

  • Assume that the particle is moving only perpendicular to a given wall. In general, one third of the total kinetic energy is in each perpendicular direction[1].
  • When the particle collides with a wall, it applies an impulse of .
  • For a given wall, this happens every seconds, so there are collisions with a given wall per second.
  • The force exerted on this wall is equal to the rate of change of impulse, so
  • The pressure is equal to force per unit area, so
  • Rearranging, we find
  • is just the volume, so for a single particle
  • Considering particles each with mean squared speed , we get .

Equating , we find:

  • (cancelling from both sides)
  • (pulling out a factor of for KE)

Specific Heat Capacity

Specific heat capacity is a measure of the energy needed to raise the temperature of of a substance by . The equation for SHC is:

Brownian Motion

Particles in a liquid or gas undergo random motion because fast free-moving molecules move around and collide with each other. The mean free path is the average distance a particle travels before colliding (the size of a 'step'). If a particles takes steps, on average its end point is steps away from its starting point.

Boltzmann Factor

For many physical processes, a certain amount of energy is needed for the process to take place. This is the activation energy E; for example, in chemistry, reagents are often heated so they have enough kinetic energy to react. Other physical processes requiring an activation energy are:

  • Changes of state
  • Thermionic emission, where electrons are emitted from a heated metal surface
  • Ionisation, where electrons are removed from an atom
    • Conduction in semiconductors
  • Viscous flow
  • Nuclear fusion
    The first five of these processes are given explicitly in the specification.
10¡1100101102103104105106107108109101010¡410¡310¡210¡1100101102103104105106Nuclearfusionand¯ssionInner-shellionization/plasmaOuter-shellionizationCovalent,ionic,metallicbondsbrokenHydrogenbondsvanderWaalsforces293KE=kBT;T=293KE=kBTE=15kBTandE=30kBTTemperatureT/KEnergy/eV10¡210¡11101102103104105106107Energy/kJmol¡1

Hope you like this diagram because we used up our entire yearly Tikz diagram budget on it.

Many physical processes require energies between and , for example water evaporation requires around at freezing.


  1. Footnote on kinetic energies in perpendicular directions
    Kinetic energies in perpendicular directions add (by the Pythagorean theorem), so on average a third of the total kinetic energy is in any given direction.↩︎