Chapter Introduction
How can the invisible motion of trillions of molecules explain the pressure of a gas, its temperature, and the laws it obeys? Kinetic theory answers this by building a microscopic model of an ideal gas. Chapter 13 of NCERT Physics for Class 11 derives Boyle's law, Charles's law, and the ideal gas equation from the molecular picture, introduces the equipartition theorem to explain why different gases have different specific heats, and connects the microscopic (molecular speeds, collisions) to the macroscopic (pressure, temperature, heat capacity). This chapter is the bridge between thermodynamics (Ch 12) and statistical mechanics.
Key Definitions
| Term | Definition | SI Unit |
|---|---|---|
| Ideal gas | A gas whose molecules are point particles with no intermolecular forces and perfectly elastic collisions | — |
| RMS speed (v_rms) | Square root of the mean of the squares of molecular speeds | m/s |
| Most probable speed (v_mp) | The speed at which the maximum number of molecules are moving (peak of Maxwell distribution) | m/s |
| Mean speed (v_avg) | Arithmetic mean of the speeds of all molecules | m/s |
| Degree of freedom | The number of independent ways a molecule can possess energy | — |
| Equipartition of energy | Each degree of freedom contributes ½kT of energy per molecule | — |
| Mean free path | Average distance a molecule travels between two successive collisions | m |
| Avogadro's number (N_A) | Number of molecules in one mole of any substance = 6.022 × 10²³ | mol⁻¹ |
| Boltzmann constant (k) | k = R/N_A = 1.38 × 10⁻²³ J/K | J/K |
Detailed Concepts
Molecular Nature of Matter and Behaviour of Gases
The kinetic theory makes the following assumptions for an ideal gas: 1. Gas consists of a large number of identical point molecules (negligible volume) 2. Molecules are in constant random motion 3. All collisions (molecule-molecule and molecule-wall) are perfectly elastic 4. No intermolecular forces except during collisions 5. The effect of gravity on molecular motion is negligible
Gas Laws from Kinetic Theory
Boyle's law: At constant temperature, the pressure of a given mass of gas is inversely proportional to its volume.
P ∝ 1/V (at constant T) → PV = constant
From kinetic theory: P = (1/3)nmv²_rms, and at constant T, v_rms is constant. If N is fixed, P ∝ 1/V.
Charles's law: At constant pressure, the volume of a given mass of gas is directly proportional to its absolute temperature.
V ∝ T (at constant P) → V/T = constant
From kinetic theory: P = (1/3)(N/V)mv²_rms and v_rms ∝ √T. At constant P, V must increase proportionally with T.
Ideal gas equation: Combining Boyle's and Charles's laws:
PV = nRT
where n = number of moles, R = 8.314 J mol⁻¹ K⁻¹ (universal gas constant)
Kinetic Theory of an Ideal Gas — Pressure and RMS Speed
Consider N molecules of mass m in a cubical container of side L. The pressure on a wall is derived from the momentum transfer of molecules colliding with it:
P = (1/3) (N/V) m v²_rms
where v²_rms = mean of the squares of molecular speeds = (v₁² + v₂² + ... + v_N²)/N
Using the ideal gas equation PV = NkT (where N = number of molecules, k = Boltzmann constant):
PV = NkT = (1/3) Nmv²_rms
Therefore:
- v_rms = √(3kT/m) = √(3RT/M) where M = molar mass
- v_avg = √(8kT/πm) = √(8RT/πM)
- v_mp = √(2kT/m) = √(2RT/M)
Ratio: v_mp : v_avg : v_rms = √2 : √(8/π) : √3 ≈ 1 : 1.128 : 1.224
Kinetic interpretation of temperature:
From (1/2)mv²_rms = (3/2)kT, the average translational kinetic energy per molecule is:
E = (3/2)kT
Temperature is a measure of the average kinetic energy of molecules. At T = 0 K, all molecular motion ceases (classical picture).
Law of Equipartition of Energy
The law states: Each degree of freedom contributes ½kT of energy per molecule (or ½RT per mole).
| Molecule Type | Translational DOF | Rotational DOF | Total DOF | C_v (per mole) | γ = C_p/C_v |
|---|---|---|---|---|---|
| Monoatomic (He, Ne, Ar) | 3 | 0 | 3 | (3/2)R = 12.5 | 5/3 ≈ 1.67 |
| Diatomic (N₂, O₂, H₂) | 3 | 2 | 5 | (5/2)R = 20.8 | 7/5 = 1.40 |
| Polyatomic (CO₂, CH₄) | 3 | 3 | 6 | 3R = 24.9 | 4/3 ≈ 1.33 |
Why diatomic has 2 rotational DOF: A diatomic molecule can rotate about two axes perpendicular to its bond axis. Rotation about the bond axis has negligible moment of inertia (point masses), so it is not counted.
Why polyatomic has 3 rotational DOF: A polyatomic molecule (non-linear) can rotate about all three mutually perpendicular axes.
Specific Heat Capacity of Gases
For an ideal gas, the specific heats are determined entirely by the degrees of freedom:
C_v = (f/2)R (per mole), where f = total DOF
C_p = C_v + R (Mayer's relation)
γ = C_p/C_v = (f + 2)/f
| Gas | f | C_v | C_p | γ |
|---|---|---|---|---|
| Monoatomic | 3 | 3R/2 | 5R/2 | 5/3 |
| Diatomic | 5 | 5R/2 | 7R/2 | 7/5 |
| Polyatomic | 6 | 3R | 4R | 4/3 |
Note: At moderate temperatures, vibrational DOF are "frozen" (not excited). At very high temperatures, they contribute. This explains why measured γ values deviate from the simple model at extreme temperatures.
Mean Free Path
The mean free path (λ) is the average distance a molecule travels between successive collisions:
λ = 1 / (√2 π n d²)
where n = number density of molecules (N/V), d = molecular diameter.
- λ increases when pressure decreases (n decreases) — fewer molecules per unit volume means fewer collisions.
- λ increases when temperature increases at constant pressure (n decreases as V increases).
- At STP, λ for air ≈ 68 nm.
Important Derivations
1. Pressure of an Ideal Gas
Consider a molecule of mass m and velocity v hitting a wall of the container (area A = L²) at the x-face.
Change in momentum per collision: Δp = 2mv_x
Time between collisions with the same wall: Δt = 2L/v_x
Force by one molecule: F₁ = 2mv_x / (2L/v_x) = mv_x²/L
Total force from N molecules: F = Σ(mv_x²/L) = (Nm/L) × v²_x_mean = (N/V) × m × v²_x_rms
Since v²_rms = v²_x + v²_y + v²_z and by symmetry v²_x = v²_y = v²_z = v²_rms/3:
P = F/A = (1/3)(N/V)mv²_rms
2. Mayer's Relation (C_p – C_v = R)
For 1 mole of ideal gas at constant volume: Q_v = C_v ΔT = ΔU (since W = 0)
For 1 mole of ideal gas at constant pressure: Q_p = C_p ΔT = ΔU + W = C_v ΔT + PΔV = C_v ΔT + RΔT
3. Degrees of Freedom and γ
For f degrees of freedom: C_v = fR/2, C_p = C_v + R = (f + 2)R/2
γ = C_p/C_v = (f + 2)/f
- Monoatomic (f = 3): γ = 5/3
- Diatomic (f = 5): γ = 7/5
- Polyatomic (f = 6): γ = 8/6 = 4/3
Common Mistakes
1. Using R in molecular formula instead of k: PV = NkT uses k (Boltzmann constant) for N molecules; PV = nRT uses R (gas constant) for n moles. Nk = nR. Do not substitute R where k belongs. 2. Confusing m (molecular mass) with M (molar mass): v_rms = √(3kT/m) = √(3RT/M). Using molar mass M in the k formula (without dividing by N_A) gives wrong results. 3. Forgetting that equipartition gives energy per molecule, not per mole: Each DOF contributes ½kT per molecule (= ½RT per mole). When calculating total energy, decide whether you need per-molecule or per-mole quantities. 4. Assuming all molecules have the same speed: The Maxwell-Boltzmann distribution shows a spread. v_rms, v_avg, and v_mp are different statistical measures of this distribution. 5. Counting vibrational DOF at room temperature: At room temperature, vibrational modes of diatomic molecules are "frozen" (energy gap too large for kT to excite). Only translational (3) and rotational (2) DOF are active, giving f = 5, not 7. 6. Mixing up C_p and C_v: C_p is always greater than C_v by R. C_p is the heat at constant pressure (gas expands and does work); C_v is at constant volume (no work done).
Numerical Practice
Example 1: RMS Speed
Calculate the RMS speed of nitrogen molecules (M = 28 g/mol) at 300 K.
v_rms = √(3RT/M) = √(3 × 8.314 × 300 / 0.028) = √(7482.6 / 0.028) = √(267235) ≈ 517 m/s
Example 2: Degrees of Freedom and Specific Heats
Find C_v, C_p, and γ for oxygen (O₂, diatomic).
f = 5 (3 translational + 2 rotational)
C_v = (5/2)R = 2.5 × 8.314 = 20.8 J mol⁻¹ K⁻¹
C_p = C_v + R = 20.8 + 8.314 = 29.1 J mol⁻¹ K⁻¹
γ = C_p/C_v = 29.1/20.8 = 1.40
Example 3: Mean Free Path
If the molecular diameter of nitrogen is 0.3 nm and the number density at STP is 2.7 × 10²⁵ m⁻³, find the mean free path.
λ = 1/(√2 π n d²) = 1/(√2 × π × 2.7 × 10²⁵ × (0.3 × 10⁻⁹)²)
= 1/(1.414 × 3.14 × 2.7 × 10²⁵ × 9 × 10⁻²⁰)
= 1/(1.414 × 3.14 × 2.43 × 10⁶)
= 1/(1.08 × 10⁷) ≈ 9.3 × 10⁻⁸ m = 93 nm
Exam Tips
1. Pressure derivation: The derivation of P = (1/3)(N/V)mv²_rms from molecular collisions is a 5-mark question favourite. Practise it step by step with a diagram of the cubical container. 2. Gas laws from kinetic theory: Be ready to show how Boyle's and Charles's laws follow from P = (1/3)(N/V)mv²_rms and v_rms ∝ √T. 3. Equipartition theorem: Know the DOF table for monoatomic, diatomic, and polyatomic gases. This is the most commonly tested concept. 4. γ values: Memorise γ = 5/3 (monoatomic), 7/5 (diatomic), 4/3 (polyatomic). Quick recall saves time in MCQs. 5. Mayer's relation derivation: A 2–3 mark standard derivation using the first law of thermodynamics. 6. RMS speed numericals: Always convert molar mass to kg/mol before using v_rms = √(3RT/M). 7. Mean free path: Usually a 1-mark formula recall or a short numerical.
NCERT Exercise Focus Areas
The table below highlights the most frequently tested NCERT exercise question types for this chapter, along with typical mark allocation and difficulty level as observed in CBSE board exams.
| NCERT Exercise Focus Area | Typical Marks | Difficulty Level |
|---|---|---|
| Pressure derivation from kinetic theory (P = 1/3 ρv²_rms) | 3–5 | Moderate |
| RMS speed, most probable speed, and mean speed calculations | 2–3 | Easy to Moderate |
| Equipartition theorem — energy per degree of freedom | 2–3 | Moderate |
| Specific heats of gases (C_v, C_p, γ) and Mayer's relation | 3–5 | Moderate |
| Degrees of freedom for monoatomic, diatomic, and polyatomic gases | 1–2 | Easy |
| Mean free path derivation and numerical problems | 2–3 | Moderate to Hard |
Board exam pattern: This chapter typically carries 3–5 marks in the theory paper. Derivations (pressure, Mayer's relation) are the high-value questions. Numerical problems on RMS speed and mean free path appear regularly in the 2-mark segment. MCQs frequently test γ values and DOF counts for quick recall.
Conceptual Questions for Practice
Test your understanding of kinetic theory with these conceptual questions. Try answering them before checking your notes.
1. Gases have two principal specific heats (C_p and C_v), but solids generally have only one. Why?
2. On a humid day, sound travels faster than on a dry day. How does kinetic theory explain this?
3. The RMS speed of hydrogen molecules at room temperature is very high (nearly 2000 m/s), yet hydrogen does not escape from an open bottle instantly. Why?
4. Two gases — helium and carbon dioxide — are at the same temperature. Which has the higher RMS speed, and why?
5. According to the equipartition theorem, each degree of freedom contributes ½kT of energy. Why then do vibrational degrees of freedom of diatomic molecules not contribute at room temperature?
Quick Revision Notes
| Formula | Meaning |
|---|---|
| PV = nRT | Ideal gas equation |
| P = (1/3)(N/V)mv²_rms | Pressure from kinetic theory |
| v_rms = √(3RT/M) | RMS speed |
| v_avg = √(8RT/πM) | Mean speed |
| v_mp = √(2RT/M) | Most probable speed |
| E = (3/2)kT | Average KE per molecule |
| C_v = (f/2)R | Molar specific heat at const V |
| C_p = C_v + R | Mayer's relation |
| γ = (f + 2)/f | Adiabatic exponent |
| λ = 1/(√2 π n d²) | Mean free path |
DOF summary: Monoatomic = 3, Diatomic = 5, Polyatomic = 6
γ values: 5/3 (mono), 7/5 (di), 4/3 (poly)
Speed ratio: v_mp : v_avg : v_rms = 1 : 1.128 : 1.224
