Laws of Motion – IIT‑JEE/Competitive Physics Notes
(Prepared by an expert teacher for AIIMS Admission)
Goal – Master the conceptual and mathematical essence of Newton’s laws, momentum, impulse, and work–energy.
Exam focus – Precise definitions, derivations from first principles, and subtle points that frequently appear in JEE‑Mains, JEE‑Advanced, and AIIMS physics problems.
1. Core Definitions
| Symbol | Meaning | Units |
|---|---|---|
| (m) | Mass of a particle | kg |
| (\mathbf{v}) | Velocity vector | m s⁻¹ |
| (\mathbf{a}) | Acceleration vector | m s⁻² |
| (\mathbf{F}) | Net external force on a body | N |
| (\mathbf{p}) | Linear momentum | kg m s⁻¹ |
| (\mathbf{I}) | Impulse | N s |
| (W) | Work done | J |
| (K) | Kinetic energy | J |
| (\mu_k, \mu_s) | Coefficients of kinetic & static friction | – |
Notation – Vectors are bold. All derivations assume an inertial frame unless specified.
2. Newton’s Laws – Statement & Consequences
2.1 First Law (Inertia)
In an inertial frame, a particle continues in uniform motion unless acted upon by a net external force.
- Consequence: If (\mathbf{F}_{\text{net}} = \mathbf{0}) → (\mathbf{a} = \mathbf{0}).
- Application: Straight‑line motion, satellite orbits, free‑fall in vacuum.
2.2 Second Law (Fundamental Relation)
The rate of change of linear momentum equals the net external force.
[ \boxed{\mathbf{F}_{\text{net}} = \frac{d\mathbf{p}}{dt}} ]
- Special case (constant mass): (\mathbf{p} = m\mathbf{v}) → (\mathbf{F}_{\text{net}} = m\mathbf{a}).
- Derivation:
[ m\mathbf{a} = \frac{d}{dt}(m\mathbf{v}) = \frac{dm}{dt}\mathbf{v} + m\frac{d\mathbf{v}}{dt} ] For constant (m), first term vanishes.
2.3 Third Law (Action–Reaction)
For every action there is an equal and opposite reaction.
[ \mathbf{F}{12} = -\mathbf{F}{21} ]
- Implication: Forces always occur in pairs; no “self‑action”.
- Tricky point: In a single-body analysis, only external forces appear in Newton’s 2nd law.
3. Momentum & Impulse
3.1 Momentum Conservation
- Closed system (no external forces) → (\displaystyle \frac{d\mathbf{p}{\text{tot}}}{dt}=0 \Rightarrow \mathbf{p}{\text{tot}}= \text{constant}).
- Collision problems: Use conservation of momentum + energy (elastic) or just momentum (inelastic).
3.2 Impulse–Momentum Theorem
[ \boxed{\mathbf{I}= \int \mathbf{F},dt = \Delta \mathbf{p}} ]
- Interpretation: The impulse delivered by a force equals the change in momentum.
- Typical exam trick: Compute the impulse from a simple force–time graph (area under curve).
3.3 Work–Energy Theorem (derived from 2nd law)
[ \boxed{W_{\text{net}} = \Delta K} ]
- Derivation:
[ W_{\text{net}} = \int \mathbf{F}{\text{net}}\cdot d\mathbf{s} = \int m\mathbf{a}\cdot d\mathbf{s} = m\int \frac{d\mathbf{v}}{dt}\cdot d\mathbf{s} = m\int \mathbf{a}\cdot \mathbf{v},dt = \frac{1}{2}m v^2\Big|{i}^{f} ] - Caveat: Only conservative forces contribute to potential energy considerations; non‑conservative (friction) appear directly in work.
4. Forces in Common Problems
| Force | Symbol | Direction | Typical Magnitude |
|---|---|---|---|
| Weight | (\mathbf{W}=m\mathbf{g}) | Downward | (mg) |
| Normal | (\mathbf{N}) | Perpendicular to surface | Variable |
| Friction | (\mathbf{f}) | Opposes motion | (\mu N) (kinetic), (\le \mu_s N) (static) |
| Tension | (\mathbf{T}) | Tension in a string | Variable |
| Applied | (\ |