B.3 Gas lawsIB Physics HL: Revision notes
Section 1
Pressure and amount of substance
Pressure is the force acting perpendicular to a surface per unit area: P = F/A, measured in pascals (1 Pa = 1 N m⁻²).
The amount of substance n, in moles, is n = N/N_A, where N is the number of particles and N_A = 6.02 × 10²³ mol⁻¹ is the Avogadro constant. Keep N (a pure number of molecules) and n (moles) separate: many calculation errors come from swapping them.
Section 2
The empirical gas laws and the ideal gas law
For a fixed mass of gas, three laws were found by experiment:
- Boyle's law (constant T): PV = constant
- Charles's law (constant P): V/T = constant
- pressure law (constant V): P/T = constant
Combining them gives PV/T = constant. Including the amount of gas gives the ideal gas law: PV = nRT or PV = Nk_BT, where R = 8.31 J K⁻¹ mol⁻¹ and k_B = R/N_A = 1.38 × 10⁻²³ J K⁻¹. Temperatures must always be in kelvin.
Using degrees Celsius in PV = nRT. Always add 273 first; a ratio like T₂/T₁ is meaningless in °C.
Section 3
The kinetic model of an ideal gas
An ideal gas is a model: an idealised system used to approximate real gases. Its assumptions are:
- a very large number of identical molecules in random motion with a range of speeds;
- molecular volume is negligible compared with the container;
- no intermolecular forces except during collisions;
- collisions are elastic and last a negligible time.
Every empirical gas law follows from these assumptions.
Section 4
Pressure from molecular collisions
When a molecule rebounds from a wall, its momentum component perpendicular to the wall reverses, a change of 2mv. The wall exerts a force equal to the rate of change of momentum, and the molecule exerts an equal and opposite force on the wall. Averaging over the huge number of collisions gives
P = ⅓ρv²
where ρ is the gas density and v is the root mean square speed. Pressure rises if molecules move faster (more momentum per collision and more frequent collisions) or if there are more of them per unit volume.
Combine P = ⅓ρv² with PV = nRT to show v² ∝ T: doubling the kelvin temperature multiplies the rms speed by √2, not 2.
Section 5
Internal energy of an ideal monatomic gas
In an ideal gas there are no intermolecular forces, so there is no intermolecular potential energy. The internal energy is the total random kinetic energy of the molecules. For a monatomic gas:
U = (3/2)Nk_BT = (3/2)nRT
The mean kinetic energy of one molecule is (3/2)k_BT, so absolute temperature is a measure of the average kinetic energy of the molecules. Because PV = nRT, you can also write U = (3/2)PV.
Section 6
When is a real gas close to ideal?
Real gases behave most like an ideal gas at low pressure, low density and high temperature (well above the temperature at which they liquefy). Then the molecules are far apart, so their volume and the forces between them are negligible.
At high pressure / high density or low temperature, molecules are close and move slowly: attractive forces reduce the pressure below the ideal value, and the molecules' own volume becomes significant. Near liquefaction the ideal model fails completely.
Saying real gases deviate at high temperature. High temperature makes gases more ideal; deviations appear at low temperature and high density.
That's the notes covered.
Carry on to the next subtopic.