The study of gases and kinetic theory is an important part of the JEE Physics syllabus. Understanding gas laws, molecular theory, and the statistical behavior of gas molecules forms the basis of many JEE problems. This detailed guide covers all the essentials of gas laws, kinetic theory, Maxwell-Boltzmann distribution, specific heat capacities, and related formulas and concepts to help you prepare effectively.
Gases are fluids that expand to fill their containers. The behavior of gases is described by empirical gas laws which relate pressure, volume, temperature, and amount of gas.
At constant temperature, the volume of a given mass of gas is inversely proportional to pressure:
At constant pressure, the volume of a given mass of gas is directly proportional to its absolute temperature:
At constant volume, the pressure of a given mass of gas is directly proportional to its absolute temperature:
Equal volumes of gases at the same temperature and pressure contain equal number of molecules.
Combining the above gas laws leads to the ideal gas equation:
Where \( P \) = pressure, \( V \) = volume, \( n \) = number of moles, \( R = 8.314 \, \text{J/mol K} \), \( T \) = absolute temperature.
Kinetic theory explains macroscopic properties of gases in terms of molecular motion and collisions.
Pressure arises from molecules colliding elastically with container walls. For \( N \) molecules of mass \( m \) in volume \( V \), average molecular speed squared is \( \overline{v^2} \). The pressure is:
The average kinetic energy per molecule is:
where \( k_B = 1.38 \times 10^{-23} \, \text{J/K} \) is Boltzmann constant.
The root mean square speed \( v_{\text{rms}} \) is:
Where \( M \) is molar mass in kg/mol.
This distribution describes the fraction of molecules having speed between \( v \) and \( v + dv \).
The distribution curve shifts to higher speeds with increasing temperature.
Specific heat is the heat capacity per unit mass or mole. For gases:
Typical values: \( \gamma = \frac{5}{3} \) for monoatomic gases, \( \frac{7}{5} \) for diatomic gases.
Each molecule has degrees of freedom representing independent ways it can store energy: translation, rotation, and vibration.
Each degree of freedom contributes \( \frac{1}{2} k_B T \) energy per molecule.
For \( f \) degrees of freedom,
Real gases deviate from ideal gas behavior due to molecular size and intermolecular forces.
where \( a \) accounts for attractive forces, and \( b \) for finite molecular volume.
Critical temperature \( T_c \), pressure \( P_c \), and volume \( V_c \) characterize gas-liquid transition.
The mean free path \( \lambda \) is average distance traveled between collisions:
where \( d \) is molecular diameter and \( \frac{N}{V} \) number density.
Diffusion: Movement of gas molecules from high to low concentration.
Effusion: Escape of gas molecules through a tiny hole without collisions.
Rate of effusion \( r \) is inversely proportional to square root of molar mass:
Concept | Formula | Remarks |
---|---|---|
Ideal Gas Equation | \( PV = nRT \) | Relates pressure, volume, temperature |
Pressure from Kinetic Theory | \( P = \frac{1}{3} \frac{N}{V} m \overline{v^2} \) | Pressure due to molecular collisions |
Average Kinetic Energy | \( E_{\text{avg}} = \frac{3}{2} k_B T \) | Energy per molecule proportional to temperature |
Root Mean Square Speed | \( v_{\text{rms}} = \sqrt{\frac{3RT}{M}} \) | Speed measure in kinetic theory |
Van der Waals Equation | \( \left(P + \frac{a}{V_m^2}\right)(V_m - b) = RT \) | Real gas behavior |
Mean Free Path | \( \lambda = \frac{1}{\sqrt{2} \pi d^2 \frac{N}{V}} \) | Average distance between collisions |
Given molar mass of oxygen \( M = 32 \times 10^{-3} \, \text{kg/mol} \), find \( v_{\text{rms}} \).
Solution:
Calculating,
\( v_{\text{rms}} = \sqrt{233606.25} = 483.3 \, \text{m/s} \)
One mole of an ideal gas expands isothermally at 300 K from volume 10 L to 20 L. Calculate work done.
Solution:
\( W = 2494.2 \times 0.693 = 1728.5 \, \text{J} \)
Mastering gases and kinetic theory requires understanding core concepts, practicing formulas, and solving a variety of problems. This guide compiles everything you need to confidently handle this important JEE physics chapter. Regular revision and problem solving will enhance your command over the topic and boost your JEE score.
Keep practicing, stay curious, and success will follow. Good luck!