Describe the pressure and the changes in pressure of a gas in terms of the forces exerted by particles colliding with surfaces, creating a force per unit area

Cambridge IGCSE Physics 0625 – Topic 2.1.2 & 2.1.3: Particle Model and Gas Laws

Objective

Explain the origin of gas pressure and the way pressure changes in terms of the forces exerted by particles when they collide with surfaces – i.e. as a force per unit area (P = F/A).

1. Particle structure of the three states of matter

  • Solids – particles are tightly packed in a regular (often crystalline) arrangement and vibrate about fixed positions.
  • Liquids – particles are close together but not in a fixed lattice; they can slide past one another, giving a definite volume but no fixed shape.
  • Gases – particles are far apart compared with their size, move rapidly in straight lines, and collide elastically with each other and with the walls of the container.

Simple particle diagrams for solids, liquids and gases (as required by the syllabus).

1.1 Atoms, molecules and ions

The particle model uses the term particle to mean any microscopic entity – an atom, a molecule or an ion – that behaves as a single unit in collisions. In a mono‑atomic gas (e.g. He) each particle is an atom; in a di‑atomic gas (e.g. O₂) each particle is a molecule; in an ionised gas (plasma) each particle may be an ion.

2. Relation between particle motion and temperature

The average translational kinetic energy of a particle is proportional to the absolute temperature:

\[

\langle Ek\rangle = \tfrac{3}{2}\,k{\rm B}\,T

\]

where \(k_{\rm B}=1.38\times10^{-23}\,\text{J K}^{-1}\) is Boltzmann’s constant. As temperature rises, particles move faster and collide with the walls more energetically.

3. Evidence for the particle model

  • Brownian motion – the erratic, observable motion of tiny suspended particles (e.g. pollen in water) results from countless collisions with the much smaller molecules of the liquid. This provides direct macroscopic evidence that molecules are in constant motion.
  • Diffusion & effusion – the spontaneous spreading of gases and the escape of gas through a small hole are both explained by random molecular motion.

4. Pressure as a force per unit area

When a gas particle strikes a surface it exerts a force on that surface. The cumulative effect of many collisions over an area \(A\) gives the pressure:

\[

P = \frac{F}{A}

\]

4.1 How a single collision produces force

  1. Consider a particle of mass \(m\) that hits a wall perpendicularly with speed \(v\) and rebounds with the same speed (elastic collision).
  2. The change in momentum is

    \[

    \Delta p = mv - (-mv) = 2mv .

    \]

  3. If the time between successive collisions of that particle with the same wall is \(\Delta t\), the average force contributed by that particle is

    \[

    F_{\text{particle}} = \frac{\Delta p}{\Delta t}.

    \]

4.2 From many particles to macroscopic pressure

  • In a volume containing \(N\) particles, many collisions occur each second on a small surface element \(dA\).
  • The total force on \(dA\) is the sum of the individual forces:

    \[

    F = \sum{i=1}^{N{\text{coll}}} \frac{\Delta pi}{\Delta ti}.

    \]

  • Dividing by the area gives the pressure:

    \[

    P = \frac{F}{A} = \frac{1}{A}\sum \frac{\Delta pi}{\Delta ti}.

    \]

5. Forces and distances between particles (supplementary)

In real gases particles exert short‑range attractive or repulsive forces. The magnitude of these forces depends on the distance between particles:

  • At very short distances (< 0.3 nm) strong repulsive forces dominate (electron cloud overlap).
  • At intermediate distances (≈ 0.3–0.5 nm) weak attractive (Van der Waals) forces act.
  • Beyond ≈ 0.5 nm the forces are negligible, and the gas behaves ideally.

These interactions explain why real gases deviate from the ideal‑gas equation at high pressures (particles forced close together) or low temperatures (attractive forces become significant).

6. Factors that change the pressure of a gas (particle‑model view)

VariableWhat changes at the particle level?Resulting effect on pressure
Temperature \(T\)Average speed ↑ → momentum change per collision ↑ and collision frequency ↑Force ↑ → pressure ↑ (Gay‑Lussac’s law)
Volume \(V\)Distance between wall and particle ↓ → particles reach the wall more often (collision frequency ↑)Force ↑ → pressure ↑ (Boyle’s law)
Amount of gas \(n\)Number of particles ↑ → more collisions per unit timeForce ↑ → pressure ↑ (direct proportionality)
Nature of the gasParticle size & intermolecular forces differ → affect how closely particles can be packed and how much kinetic energy is lost in collisionsReal‑gas deviations from ideal behaviour at high \(p\) or low \(T\)

7. Gas laws explained with the particle model

7.1 Boyle’s law (constant \(T\) and \(n\))

\[

pV = \text{constant}

\]

Halving the volume halves the average distance a particle travels before hitting a wall, so the collision frequency doubles; the average force per unit area therefore doubles, giving twice the pressure.

7.2 Charles’s law (constant \(p\) and \(n\))

\[

\frac{V1}{T1} = \frac{V2}{T2}

\]

Raising the temperature increases the average speed of the particles. To keep the pressure unchanged, the container must expand so that the collision frequency per unit area remains the same.

7.3 Gay‑Lussac’s law (constant \(V\) and \(n\))

\[

\frac{p1}{T1} = \frac{p2}{T2}

\]

At a fixed volume, a higher temperature means faster particles and a larger momentum change per collision, so the pressure rises in direct proportion to \(T\).

7.4 Combined gas law (constant \(n\))

\[

\frac{pV}{T} = \text{constant}

\]

7.5 Ideal‑gas equation (core)

\[

pV = nRT

\]

Derivable from the particle model by substituting \(\langle Ek\rangle = \tfrac{3}{2}k{\rm B}T\) into the kinetic‑theory expression for pressure:

\[

p = \frac{1}{3}\frac{N}{V}m\langle v^2\rangle,

\]

where \(N = nN{\!A}\) and \(R = N{\!A}k_{\rm B}\).

8. Worked examples (illustrating pressure changes)

  1. Heating a sealed container

    A 2 L container holds 0.5 mol of an ideal gas at 300 K. It is heated to 600 K while the volume remains fixed.

    Using \(p1/T1 = p2/T2\):

    \[

    p2 = p1\frac{600}{300}=2p_1.

    \]

    The pressure doubles because the average particle speed (and thus momentum change per collision) doubles.

  2. Compressing the gas at constant temperature

    The same gas is now compressed isothermally from 2 L to 1 L.

    From Boyle’s law, \(p1V1 = p2V2\) → \(p2 = p1\frac{2}{1}=2p_1\).

    Halving the volume halves the mean free path, doubling the collision frequency.

  3. Adding more gas at constant \(T\) and \(V\)

    Adding another 0.5 mol (doubling \(n\)) while keeping \(V\) and \(T\) unchanged gives, from the ideal‑gas equation,

    \[

    p2 = 2p1.

    \]

    Twice as many particles mean twice as many collisions per second.

9. Summary

  • Pressure is the macroscopic manifestation of countless microscopic collisions of gas particles with a surface. Each collision changes a particle’s momentum; the total change per unit time gives a force, and pressure is that force divided by the area (P = F/A).
  • Temperature controls particle speed, volume controls collision frequency, and the amount of gas controls the number of colliding particles.
  • Brownian motion provides observable evidence for the particle model, while intermolecular forces become important for real gases at high pressures or low temperatures.
  • The particle‑model explanations naturally lead to the gas laws (Boyle, Charles, Gay‑Lussac, combined) and the ideal‑gas equation, which together describe how pressure, volume, temperature and amount of gas are inter‑related.

Suggested diagram: a rectangular container showing randomly moving particles, arrows indicating collisions with a small surface element, and the resulting force vector on that element.