Explain why a gas that obeys the proportionality p V ∝ T (with T the thermodynamic temperature) is described as an ideal gas, and show how this leads to the ideal‑gas equation p V = n R T.
| Quantity | Symbol | Definition | SI Unit |
|---|---|---|---|
| Pressure | p | Force per unit area | Pa (N m⁻²) |
| Volume | V | Space occupied by the gas | m³ |
| Thermodynamic temperature | T | Absolute temperature | K |
| Amount of substance | n | Number of moles | mol |
| Universal gas constant | R | R = 8.314 J mol⁻¹ K⁻¹ = 0.08206 L atm mol⁻¹ K⁻¹ | J mol⁻¹ K⁻¹ |
| Avogadro’s constant | NA | Number of particles per mole | 6.022 × 10²³ mol⁻¹ |
| Boltzmann constant | kB | Energy per particle per kelvin | 1.381 × 10⁻²³ J K⁻¹ |
1 mol = 6.022 × 10²³ particles. The total number of particles in a sample is N = n NA. Because R = NAkB, the macroscopic constant R links the microscopic kinetic‑theory expression to the ideal‑gas law.
The ideal‑gas law is a model that simplifies the behaviour of real gases by adopting three explicit assumptions:
These assumptions allow a simple relationship between the macroscopic variables p, V, T and the amount of substance n. The model works well at moderate pressures (≤ 1 atm) and temperatures (≈ 300 K – 1000 K), which covers the majority of Cambridge AS & A‑Level exam questions.
Consider N identical particles of mass m moving randomly with average squared speed ⟨c²⟩. Kinetic theory gives
\$pV = \frac{1}{3}\,N\,m\,\langle c^{2}\rangle\$
Equipartition of energy states that the average translational kinetic energy of one particle is
\$\frac{1}{2}m\langle c^{2}\rangle = \frac{3}{2}k_{\mathrm{B}}T\$
Substituting the second expression into the first yields
\$pV = N k_{\mathrm{B}} T\$
Since N = nN{A} and R = N{A}k_{B}, we obtain the macroscopic ideal‑gas law
\$\boxed{pV = nRT}\$
For a fixed amount of gas (n constant) the equation can be rearranged as needed:
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