Puducherry TET (Teacher Eligibility) /General Awareness & Current Affairs

Physics basics

General Science · free study notes

Physics Basics – MIT‑Level Study Notes

(Prepared for the Puducherry TET – General Awareness & Current Affairs)

These notes start from first principles and progressively build a rigorous mathematical framework, suitable for a university‑level understanding while remaining focused on concepts that appear in the TET syllabus.
Where appropriate, we point out subtle edge cases and give a challenging problem at the end.


1. Introduction

Topic Why It Matters for TET Typical Question Types
Classical mechanics Foundations of motion, kinematics, dynamics Multiple‑choice, short‑answer, derivation
Thermodynamics Heat, temperature, energy transfer Conceptual, calculation
Electromagnetism Electricity & magnetism, Maxwell’s equations Vector calculus, circuit analysis
Waves & optics Light, sound, interference Wave equations, resonance
Relativity & Quantum Modern physics, current research Conceptual explanations, derivations

2. Classical Mechanics (First Principles)

2.1 Newton’s Laws

  1. Inertia – An object remains at rest or in uniform motion unless acted upon by a net external force.
  2. Dynamics –
    [ \mathbf{F}=m,\mathbf{a} ]
  3. Action‑Reaction –
    [ \mathbf{F}{12}=-\mathbf{F}{21} ]

Edge case – Zero mass: (m=0) gives (\mathbf{F}=0) regardless of acceleration; physically impossible for a massive particle.

2.2 Lagrangian & Hamiltonian Formulations

  • Lagrangian (L=T-U)
    Euler–Lagrange equation:

    [ \frac{d}{dt}\frac{\partial L}{\partial \dot{q}_i} -\frac{\partial L}{\partial q_i}=0 ]

  • Hamiltonian (H=\sum_i p_i\dot{q}_i - L)
    Generates equations of motion via Poisson brackets.

Edge case – Constrained systems: For a bead on a wire, coordinates reduce; Lagrange multipliers enforce constraints.

2.3 Conservation Laws

  • Linear momentum (\mathbf{p}=m\mathbf{v}) conserved in isolated systems.
  • Angular momentum (\mathbf{L}=\mathbf{r}\times\mathbf{p}); torque (\boldsymbol{\tau}=\frac{d\mathbf{L}}{dt}).
  • Energy (E=T+U) conserved if potential is time‑independent.

3. Work, Energy, and Power

Concept Formula Physical Insight
Work (W=\int \mathbf{F}\cdot d\mathbf{r}) Path independence for conservative forces
Kinetic Energy (T=\tfrac12 m v^2) Scalar invariant of motion
Potential Energy (U=-\int \mathbf{F}\cdot d\mathbf{r}) Defined up to a constant
Power (P=\frac{dW}{dt}=\mathbf{F}\cdot\mathbf{v}) Energy transfer rate

Edge case – Impulse–momentum theorem: For impulsive forces (F(t)), ( \Delta \mathbf{p} = \int F(t),dt ).


4. Thermodynamics

4.1 Laws

Law Statement Mathematical Form
0 Temperature equalizes (T_1=T_2) at equilibrium
1 Energy conservation ( \Delta U = Q - W )
2 Entropy never decreases ( \Delta S \ge 0)
3 Absolute zero unattainable (T\rightarrow 0) impossible

4.2 Entropy & Statistical Mechanics

  • Boltzmann's formula
    [ S = k_B \ln \Omega ] where (\Omega) is the number of microstates.
  • Canonical distribution
    [ P_i = \frac{e^{-\beta E_i}}{Z},\quad Z=\sum_i e^{-\beta E_i} ]

Edge case – Negative temperatures: In systems with bounded spectra, population inversion leads to (\beta<0), implying higher energy states are more populated.


5. Electromagnetism

5.1 Coulomb’s Law

[ \mathbf{F} = k_e \frac{

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