Physics · Ch 3 — Kinetic Theory of Gases and Radiation
Introduction
Introduction
The state of a fixed mass of gas is completely specified by a small set of macroscopic quantities -- its pressure , volume , temperature , and internal energy -- and any equation relating these quantities for a given gas is called its equation of state.
Three separate experimental gas laws, each holding one variable fixed, describe how these quantities are linked for a fixed mass of gas:
- Boyle's law: at constant
- Charles' law: at constant
- Gay-Lussac's law: at constant
Combining all three into a single relation for a fixed mass of gas gives , so that for the same gas in two different states, .
Expressing the fixed mass in terms of the number of moles , this generalises to the ideal gas equation
where is the universal gas constant, , the same for every gas. Writing the mass in terms of the actual number of molecules instead of moles gives the equivalent microscopic form
where is the Boltzmann constant, related to by ( being Avogadro's number, the number of molecules in one mole).
The gas laws of Boyle, Charles and Gay-Lussac are strictly valid only when the pressure is not too high and the temperature is not close to the gas's liquefaction temperature. A gas that obeys at all pressures and temperatures, with no exception, is called an ideal gas -- a theoretical idealisation that real gases only approach under suitable conditions, explored further in the next section.
Equation of State. The state of a gas is specified by physical quantities such as its pressure P, temperature T, volume V and internal energy E. The equation relating these quantities — PV = nRT for an ideal gas — is called the equation of state; a gas obeying it at all pressures and temperatures is an ideal gas.