Ideal Gas Equation and Gas Constant

Understand the equation PV = nRT and the meaning of the universal gas constant R.

1. What the Ideal Gas Equation Represents

The ideal gas equation combines all individual gas laws (Boyle’s, Charles’, and Gay-Lussac’s laws) into one simple relation:

PV = nRT

This equation connects pressure, volume, temperature, and amount of gas in a single formula.

2. Variables in the Ideal Gas Equation

Each symbol in the equation has a clear physical meaning:

  • P → pressure of the gas
  • V → volume of the gas
  • n → number of moles
  • R → universal gas constant
  • T → absolute temperature (in Kelvin)

2.1. Requirement

Temperature must be in Kelvin for the equation to work correctly.

3. Meaning of the Universal Gas Constant (R)

The gas constant R is a fixed value that relates energy scale to temperature and moles. Its value is:

R = 8.314\ \text{J mol}^{-1} \text{K}^{-1}

This constant appears in many areas of physics and chemistry because it links macroscopic gas properties to molecular motion.

3.1. Other Common Units of R

  • 0.0821 L·atm mol⁻¹ K⁻¹
  • 8.314 J mol⁻¹ K⁻¹
  • 62.36 L·torr mol⁻¹ K⁻¹

4. How the Ideal Gas Equation Is Derived

The ideal gas equation is obtained by combining basic gas laws:

PV = nRT

comes from:

  • Boyle’s law: \( P \propto 1/V \)
  • Charles’ law: \( V \propto T \)
  • Avogadro’s law: \( V \propto n \)

Combining these proportionalities gives the full equation.

4.1. Microscopic View

Kinetic theory also gives the same relation:

P = \dfrac{1}{3} \rho \bar{c^2}

This links molecular motion directly to pressure.

5. Using the Ideal Gas Equation

The equation is often used to calculate unknown values when others are known. Common uses:

5.1. 1. Finding Pressure

P = \dfrac{nRT}{V}

5.2. 2. Finding Volume

V = \dfrac{nRT}{P}

5.3. 3. Finding Number of Moles

n = \dfrac{PV}{RT}

6. When the Ideal Gas Equation Works Well

Most gases follow the ideal gas equation closely when:

  • pressure is low
  • temperature is high

Under these conditions, the molecules are far apart and intermolecular forces become negligible.

6.1. Examples

Air, helium, nitrogen, and oxygen behave nearly ideally at room temperature and atmospheric pressure.

7. When the Ideal Gas Equation Fails

Deviation happens when conditions make molecules come close together:

  • high pressure
  • low temperature

Here, intermolecular forces become important and real gases no longer perfectly satisfy PV = nRT.

7.1. Real Gas Correction

To fix deviations, modified equations like the Van der Waals equation are used.