A hypothetical gas whose behaviour is fully described by the kinetic theory.
Core assumptions:
When a molecule strikes the wall, its perpendicular velocity component reverses.
The momentum change \(\Delta p = 2 m v_x\) pushes the wall; countless such pushes per second create measurable pressure.
Microscopically, pressure depends on how many molecules hit the walls and how hard they hit.
Combining with \(PV = NkT\) gives average kinetic energy \( \frac{3}{2}kT \).
Increasing \( \overline{v^{2}} \) with heat raises pressure at fixed volume.
Ideal gas law relates macroscopic pressure and volume to particle number and absolute temperature.
Kinetic theory links pressure to the average translational kinetic energy of molecules.
Substitute step 2 into step 1 and cancel \(V\) to relate \(T\) to molecular speed.
Solving shows root-mean-square speed rises with temperature and falls with molecular mass.
Temperature is a direct measure of the average kinetic energy of gas particles; higher \(T\) means faster molecules.
Fig 12.1 Compressibility factor Z vs pressure
The flat line at \(Z = 1\) shows an ideal gas.
Real gas curves peel away at high pressure or low temperature because intermolecular forces and molecular volume matter.
For an ideal gas, if the absolute temperature \(T\) is doubled, what happens to the average translational kinetic energy of its molecules?
Use \( \overline{E_k} = \frac{3}{2} k T \). Average kinetic energy is directly proportional to absolute temperature.
Since \( \overline{E_k} \propto T \), doubling \(T\) doubles the average kinetic energy.
Remember, average kinetic energy varies linearly with absolute temperature.
Rapid, random molecular collisions with walls create pressure—foundation of microscopic gas view.
Gas temperature directly reflects average translational kinetic energy per molecule.
\(P = \frac{1}{3} n m v^{2}\) mathematically links particle motion to measurable pressure.
Point particles with no forces obey \(PV = nRT\), unifying motion and macroscopic law.
Departures highlight intermolecular attractions and sizes, sharpening our microscopic understanding.