Kinetic Theory

ЁЯПл NCERTClass 11Physics

ЁЯУР Formula & Cheat Sheet (English)

Class 11 Physics | Chapter: Kinetic Theory (рдЕрдгреБрдЧрддрд┐ рд╕рд┐рджреНрдзрд╛рдВрдд)

Quick Revision Notes & Formula Sheet (MP Board)


1. Fundamental Ideal Gas Laws (рдЧреИрд╕ рдХреЗ рдирд┐рдпрдо)

  • BoyleтАЩs Law (рдмреЙрдпрд▓ рдХрд╛ рдирд┐рдпрдо): At constant temperature ($T$), $P \propto \frac{1}{V} \implies P_1 V_1 = P_2 V_2$
  • CharlesтАЩs Law (рдЪрд╛рд░реНрд▓реНрд╕ рдХрд╛ рдирд┐рдпрдо): At constant pressure ($P$), $V \propto T \implies \frac{V_1}{T_1} = \frac{V_2}{T_2}$
  • Gay-LussacтАЩs Law (рдЧреЗ-рд▓реБрд╕рд╛рдХ рдХрд╛ рдирд┐рдпрдо): At constant volume ($V$), $P \propto T \implies \frac{P_1}{T_1} = \frac{P_2}{T_2}$
  • AvogadroтАЩs Law (рдЖрд╡реЛрдЧрд╛рджреНрд░реЛ рдХрд╛ рдирд┐рдпрдо): Equal volumes of all gases under the same temperature and pressure contain an equal number of molecules ($N_1 = N_2$).

2. Ideal Gas Equation (рдЖрджрд░реНрд╢ рдЧреИрд╕ рд╕рдореАрдХрд░рдг)

An ideal gas strictly obeys all gas laws at all pressures and temperatures.

$$\mathbf{P V = n R T = N k_B T}$$

Where:

  • $P$ = Pressure (рджрд╛рдм)
  • $V$ = Volume (рдЖрдпрддрди)
  • $n$ = Number of moles (рдореЙрд▓ рдХреА рд╕рдВрдЦреНрдпрд╛) $= \frac{m}{M} = \frac{N}{N_A}$
  • $R$ = Universal Gas Constant $= 8.314 \text{ J/(mol}\cdot\text{K)}$
  • $N$ = Total number of molecules
  • $N_A$ = Avogadro's Number $= 6.022 \times 10^{23} \text{ molecules/mol}$
  • $k_B$ = Boltzmann Constant $= \frac{R}{N_A} = 1.38 \times 10^{-23} \text{ J/K}$

3. Assumptions of Kinetic Theory of Gases (рдЕрдгреБрдЧрддрд┐ рд╕рд┐рджреНрдзрд╛рдВрдд рдХреА рдкрд░рд┐рдХрд▓реНрдкрдирд╛рдПрдВ)

  1. A gas consists of extremely small particles called molecules.
  2. Molecules are in a state of continuous, random motion in all directions.
  3. The actual volume of molecules is negligible compared to the total volume of the gas.
  4. There are no intermolecular attractive or repulsive forces between molecules.
  5. Collisions between molecules and with the container walls are perfectly elastic (Kinetic Energy and Momentum are conserved).
  6. The time spent during a collision is negligible compared to the time between two consecutive collisions.

4. Pressure Exerted by an Ideal Gas (рдЖрджрд░реНрд╢ рдЧреИрд╕ рдХрд╛ рджрд╛рдм)

$$\mathbf{P = \frac{1}{3} \rho v_{rms}^2 = \frac{1}{3} \frac{N m}{V} v_{rms}^2}$$

Where:

  • $\rho$ = Density of the gas $= \frac{m N}{V}$
  • $m$ = Mass of a single molecule
  • $v_{rms}$ = Root Mean Square speed of gas molecules

5. Kinetic Interpretation of Temperature (рддрд╛рдк рдХреА рдЧрддрд┐рдЬ рд╡реНрдпрд╛рдЦреНрдпрд╛)

  • Average Kinetic Energy per Molecule: $$E_k = \frac{3}{2} k_B T$$

  • Total Kinetic Energy of 1 Mole of Gas: $$E_{mole} = \frac{3}{2} R T$$

Key Takeaway: Temperature is a direct measure of the average translational kinetic energy of gas molecules. At $T = 0 \text{ K}$ (Absolute Zero), molecular motion completely stops ($v_{rms} = 0$).


6. Speeds of Gas Molecules (рдЧреИрд╕ рдЕрдгреБрдУрдВ рдХреА рдЪрд╛рд▓)

  1. Root Mean Square Speed ($v_{rms}$): $$v_{rms} = \sqrt{\frac{3 R T}{M}} = \sqrt{\frac{3 k_B T}{m}} = \sqrt{\frac{3 P}{\rho}}$$

  2. Average Speed ($v_{avg}$): $$v_{avg} = \sqrt{\frac{8 R T}{\pi M}} = \sqrt{\frac{8 k_B T}{\pi m}}$$

  3. Most Probable Speed ($v_{mp}$): $$v_{mp} = \sqrt{\frac{2 R T}{M}} = \sqrt{\frac{2 k_B T}{m}}$$

  • Comparison / Ratio: $$v_{mp} : v_{avg} : v_{rms} = \sqrt{2} : \sqrt{\frac{8}{\pi}} : \sqrt{3} \approx 1 : 1.128 : 1.225$$ $$\mathbf{v_{rms} > v_{avg} > v_{mp}}$$

7. Degrees of Freedom ($f$) (рд╕реНрд╡рд╛рддрдВрддреНрд░реНрдп рдХреЛрдЯрд┐)

The total number of independent coordinates or ways in which a system can possess energy.

Gas AtomicityDegrees of Freedom ($f$)BreakdownExamples
Monoatomic (рдПрдХрдкрд░рдорд╛рдгреБрдХ)33 Translational$\text{He, Ne, Ar}$
Diatomic (Rigid) (рджреНрд╡рд┐рдкрд░рдорд╛рдгреБрдХ)53 Trans + 2 Rotational$\text{O}_2, \text{N}_2, \text{H}_2$
Diatomic (Non-rigid/High T)73 Trans + 2 Rot + 2 Vibrational$\text{O}_2 \text{ at high temp}$
Polyatomic / Non-linear63 Trans + 3 Rotational$\text{H}_2\text{O}, \text{NH}_3, \text{CH}_4$

8. Law of Equipartition of Energy (рдКрд░реНрдЬрд╛ рдХреЗ рд╕рдорд╡рд┐рднрд╛рдЬрди рдХрд╛ рдирд┐рдпрдо)

For any dynamical system in thermal equilibrium, the total energy is equally distributed among all its degrees of freedom.

  • Energy associated with each degree of freedom per molecule $= \frac{1}{2} k_B T$
  • Total Internal Energy of 1 mole of gas with '$f$' degrees of freedom: $$U = \frac{f}{2} R T$$

9. Specific Heat Capacities of Gases (рдЧреИрд╕реЛрдВ рдХреА рд╡рд┐рд╢рд┐рд╖реНрдЯ рдКрд╖реНрдорд╛)

  • Molar Heat Capacity at Constant Volume ($C_v$): $$C_v = \frac{dU}{dT} = \frac{f}{2} R$$

  • Molar Heat Capacity at Constant Pressure ($C_p$): $$C_p = C_v + R = \left(\frac{f}{2} + 1\right) R$$

  • MayerтАЩs Relation (рдореЗрдпрд░ рдХрд╛ рд╕рдВрдмрдВрдз): $$C_p - C_v = R$$

  • Adiabatic Index / Ratio of Specific Heats ($\gamma$): $$\gamma = \frac{C_p}{C_v} = 1 + \frac{2}{f}$$

Summary Table for Specific Heats:

Type of Gas$f$$C_v$$C_p$$\gamma = C_p / C_v$
Monoatomic3$\frac{3}{2} R$$\frac{5}{2} R$$\frac{5}{3} \approx 1.67$
Diatomic (Rigid)5$\frac{5}{2} R$$\frac{7}{2} R$$\frac{7}{5} = 1.40$
Polyatomic (Non-linear)6$3 R$$4 R$$\frac{4}{3} \approx 1.33$

10. Mean Free Path ($\lambda$) (рдорд╛рдзреНрдп рдореБрдХреНрдд рдкрде)

The average distance traveled by a gas molecule between two successive collisions.

$$\mathbf{\lambda = \frac{1}{\sqrt{2} n \pi d^2}}$$

In terms of Pressure and Temperature: $$\mathbf{\lambda = \frac{k_B T}{\sqrt{2} \pi d^2 P}}$$

Where:

  • $n$ = Number density (number of molecules per unit volume $= N/V$)
  • $d$ = Diameter of the gas molecule
  • $P$ = Pressure of the gas
  • $T$ = Absolute temperature

Factors affecting Mean Free Path:

  1. $\lambda \propto \frac{1}{n}$ (Inversely proportional to molecular density)
  2. $\lambda \propto \frac{1}{d^2}$ (Inversely proportional to square of molecular diameter)
  3. $\lambda \propto T$ (Directly proportional to temperature at constant pressure)
  4. $\lambda \propto \frac{1}{P}$ (Inversely proportional to pressure at constant temperature)

Quick Revision Tips for Board Exams

  • Derivation Alert: Practice the derivation of Pressure exerted by an ideal gas ($P = \frac{1}{3}\rho v_{rms}^2$) тАФ extremely popular in MP Board long-answer questions.
  • Definitions: Memorize definitions of Degrees of Freedom, Law of Equipartition of Energy, and Mean Free Path.
  • Numerical Focus: Practice finding $v_{rms}$ at different temperatures and calculating ratios of $C_p/C_v$ for gas mixtures.