AP® Physics 2: Algebra-Based · Unit 9 · Topic 9.2
The Ideal Gas Law
The ideal gas law, PV = nRT, says pressure times volume equals the amount of gas times a constant times absolute temperature. Change any one quantity and the others must shift together to keep the equation balanced.
Picture a gas as a swarm of tiny particles slamming into the walls of their container. Pressure is just the force of all those collisions spread over the wall's area. Volume is how much room the particles have to roam. Temperature measures how fast they are moving on average, and n (or N) counts how many particles are doing the moving. PV = nRT ties all four together through one constant, R = 8.314 J/(mol K), that makes the units work out. Raise the temperature and the particles hit the walls harder and more often, so pressure or volume must rise to compensate. Squeeze the volume down and the same number of particles crowd into less space, so pressure climbs. Nothing about the gas itself changes in these swaps, only how its energy gets distributed among P, V, and T.
Working the equation is mostly solving for whichever letter is missing, but the trap is temperature. R was built assuming T is measured in kelvin, where zero actually means zero particle motion. Plug in Celsius and you can get negative or nonsense pressures, because 0 C is not zero energy, it is 273.15 K of very real molecular jostling. Always convert with T(K) = T(C) + 273.15 before touching the formula.
The two versions of the law, PV = nRT and PV = NkT, describe the same physics at two different scales. One counts gas in moles using R, the other counts individual particles using the Boltzmann constant k = 1.38 x 10−23 J/K. Since a mole is just 6.022 x 1023 particles, nR and Nk are the same number written two ways. This sets up the next idea in the unit, kinetic theory, where temperature gets connected directly to the average kinetic energy of each particle.
Key terms
- Ideal gas
- A simplified gas model where particles have no volume and no attraction to each other, only collisions.
- R (gas constant)
- The proportionality constant 8.314 J/(mol K) that makes PV = nRT dimensionally consistent when using moles.
- Boltzmann constant (k)
- The particle-counting version of R, equal to 1.38 x 10−23 J/K, used in PV = NkT.
- Absolute temperature
- Temperature measured in kelvin, where 0 K corresponds to zero average particle kinetic energy.
- Moles (n)
- A count of particles in units of 6.022 x 1023, used to measure the amount of gas present.
Watch it explained
- How it worksWalk me through how P, V, n, and T trade off against each other in PV = nRT.
- Worked exampleFind the new pressure when 2.0 mol of gas in a 0.050 m3 tank goes from 300 K to 450 K.
- Worked exampleFind the volume one mole of ideal gas occupies at 273 K and 1.0 x 105 Pa.
- How it worksHow is PV = NkT the very same law as PV = nRT, only counted particle by particle?
- Common mistakeWhy doesn't the ideal gas law work when you plug the temperature in as degrees Celsius?
Check yourself
End of topic.