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Theoretical Physicist Course
More than 20 lakh learners worldwide

Theoretical Physicist Course

Master the full mathematical and conceptual framework of theoretical physics, from classical mechanics and electrodynamics to quantum field theory and general relativity. This course delivers graduate-level rigour across every foundational domain, equipping you with the tools to tackle research-grade problems. If you are serious about theoretical physics, this is where that journey is built.

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What you will learn:

You will develop a rigorous command of the mathematical methods underpinning modern theoretical physics, including PDEs, tensor calculus, and complex analysis. You will study classical mechanics in Lagrangian and Hamiltonian forms, then progress through Maxwell's electrodynamics, special and general relativity, and non‑relativistic quantum mechanics. Statistical mechanics and thermodynamics are presented with full ensemble formalism, linking microscopic quantum states to macroscopic observables. The course culminates in quantum field theory, covering canonical quantisation, path integrals, renormalisation, and the Standard Model. Supplementary material includes group theory, computational methods, scientific writing, and career development for theoretical physicists.

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Course content

8 Chapters • 40 LessonsDuration between 4 and 360 hours (you decide)

Chapter 1See details

Mathematical Foundations for Physics

  • Lesson 1 • Ordinary Differential Equations

    Develops solution techniques for ODEs governing physical motion and fields. Connects directly to Newton's laws and oscillatory systems.

  • Lesson 2 • Partial Differential Equations

    Covers wave, heat, and Laplace equations central to classical and quantum physics. Separation of variables and Green's functions are emphasized.

  • Lesson 3 • Complex Analysis and Special Functions

    Introduces complex variables, contour integration, and special functions used throughout physics. Residue theorem enables evaluation of physical integrals.

  • Lesson 4 • Linear Algebra and Tensor Calculus

    Introduces vector spaces, matrices, eigenvalue problems, and tensors. Tensors are essential for relativity and continuum mechanics.

  • Lesson 5 • Calculus and Vector Analysis

    Covers multivariable calculus, gradient, divergence, and curl operators. These tools underpin field theories and classical mechanics formulations.

Chapter 2See details

Classical Mechanics

  • Lesson 1 • Hamiltonian Mechanics

    Reformulates mechanics using phase space and Hamilton's equations. Canonical transformations and Poisson brackets prepare students for quantum mechanics.

  • Lesson 2 • Small Oscillations and Normal Modes

    Treats coupled oscillators and normal mode decomposition using matrix methods. Lays groundwork for field quantisation and phonon physics.

  • Lesson 3 • Lagrangian Mechanics

    Introduces generalised coordinates and the principle of least action. Euler-Lagrange equations replace Newton's laws in complex systems.

  • Lesson 4 • Newtonian Mechanics and Conservation Laws

    Reviews Newton's laws and derives conservation of energy, momentum, and angular momentum. Provides the physical intuition underlying formal mechanics.

  • Lesson 5 • Rigid Body Dynamics

    Analyses rotation of rigid bodies using inertia tensors and Euler angles. Connects tensor algebra from Chapter 1 to physical rotational motion.

Chapter 3See details

Electrodynamics

  • Lesson 1 • Electrostatics and Magnetostatics

    Derives Coulomb's law, Gauss's law, and Biot-Savart law from Maxwell's equations. Establishes field concepts and potential theory for static configurations.

  • Lesson 2 • Electromagnetic Potentials and Gauge Theory

    Introduces scalar and vector potentials and gauge freedom. Lorentz and Coulomb gauges are applied to simplify field equations.

  • Lesson 3 • Maxwell's Equations and Electromagnetic Waves

    Presents the full set of Maxwell's equations and derives the wave equation. Plane wave solutions and polarisation states are analysed in detail.

  • Lesson 4 • Radiation from Accelerating Charges

    Derives Lienard-Wiechert potentials and radiation fields from moving charges. Larmor formula and synchrotron radiation are key outcomes.

  • Lesson 5 • Electrodynamics in Media

    Extends Maxwell's equations to dielectric and magnetic materials. Dispersion, absorption, and wave propagation in media are treated systematically.

Chapter 4See details

Special and General Relativity

  • Lesson 1 • Special Relativity and Spacetime

    Introduces Lorentz transformations, four-vectors, and spacetime intervals. Resolves apparent paradoxes and establishes covariant notation.

  • Lesson 2 • Differential Geometry for Gravity

    Introduces manifolds, metric tensors, Christoffel symbols, and curvature tensors. These geometric tools are prerequisites for general relativity.

  • Lesson 3 • Covariant Electrodynamics

    Reformulates Maxwell's equations using four-tensors and the electromagnetic field tensor. Demonstrates manifest Lorentz covariance of electrodynamics.

  • Lesson 4 • Solutions and Physical Applications

    Analyses Schwarzschild and Friedmann-Robertson-Walker solutions. Covers black holes, gravitational waves, and standard cosmological models.

  • Lesson 5 • Einstein's Field Equations

    Derives Einstein's field equations from the Einstein-Hilbert action. Physical interpretation of the stress-energy tensor and cosmological constant is given.

Chapter 5See details

Quantum Mechanics

  • Lesson 1 • Schrödinger Equation and Canonical Problems

    Derives the time-dependent and time-independent Schrödinger equations. Solves the infinite well, harmonic oscillator, and hydrogen atom exactly.

  • Lesson 2 • Angular Momentum and Spin

    Develops angular momentum algebra using ladder operators and Clebsch-Gordan coefficients. Introduces intrinsic spin and its physical consequences.

  • Lesson 3 • Hilbert Space and Dirac Formalism

    Introduces state vectors, operators, and the Dirac bra-ket notation. Establishes the mathematical framework for all subsequent quantum theory.

  • Lesson 4 • Approximation Methods

    Covers time-independent and time-dependent perturbation theory, variational method, and WKB approximation. Applies these to atomic and molecular systems.

  • Lesson 5 • Identical Particles and Entanglement

    Treats symmetrisation postulate, Fermi-Dirac and Bose-Einstein statistics, and quantum entanglement. Connects to many-body physics and quantum information.

Chapter 6See details

Statistical Mechanics and Thermodynamics

  • Lesson 1 • Thermodynamic Foundations

    Reviews laws of thermodynamics, thermodynamic potentials, and Maxwell relations. Establishes the macroscopic framework that statistical mechanics must reproduce.

  • Lesson 2 • Statistical Ensembles

    Introduces microcanonical, canonical, and grand canonical ensembles. Derives partition functions and connects them to free energies.

  • Lesson 3 • Quantum Statistical Mechanics

    Applies statistical mechanics to quantum systems obeying Fermi-Dirac and Bose-Einstein distributions. Treats ideal quantum gases and their physical realisations.

  • Lesson 4 • Non-Equilibrium Statistical Mechanics

    Introduces Boltzmann transport equation, linear response theory, and fluctuation-dissipation theorem. Connects microscopic dynamics to transport coefficients.

  • Lesson 5 • Phase Transitions and Critical Phenomena

    Analyses first- and second-order phase transitions using mean-field theory and the Ising model. Introduces critical exponents and universality classes.

Chapter 7See details

Quantum Field Theory

  • Lesson 1 • Canonical Quantisation of Fields

    Quantises scalar, spinor, and vector fields using commutation and anti-commutation relations. Fock space and creation/annihilation operators are central tools.

  • Lesson 2 • Path Integral Formulation

    Derives the path integral from the canonical formalism and applies it to scalar and gauge fields. Functional methods and generating functionals are introduced.

  • Lesson 3 • Renormalisation and Loop Corrections

    Treats ultraviolet divergences, dimensional regularisation, and renormalisation schemes. Running coupling constants and the renormalisation group equation are derived.

  • Lesson 4 • Classical Field Theory

    Extends Lagrangian mechanics to fields using the Euler-Lagrange field equations. Noether's theorem connects symmetries to conserved currents.

  • Lesson 5 • Interacting Fields and Feynman Diagrams

    Introduces interaction picture, Dyson series, and Wick's theorem. Feynman rules are derived and applied to tree-level scattering amplitudes.

Chapter 8See details

Advanced Topics in Theoretical Physics

  • Lesson 1 • Condensed Matter Field Theory

    Applies QFT methods to many-body systems, superconductivity, and the quantum Hall effect. Effective field theories and emergent phenomena are emphasised.

  • Lesson 2 • Introduction to String Theory

    Introduces bosonic and superstring actions, worldsheet quantisation, and the string spectrum. Provides conceptual entry into beyond-Standard-Model physics.

  • Lesson 3 • Spontaneous Symmetry Breaking and Topology

    Analyses Goldstone's theorem, topological defects, and instantons. Connects symmetry breaking to phase transitions and non-perturbative phenomena.

  • Lesson 4 • Renormalisation Group Methods

    Develops Wilsonian renormalisation group, fixed points, and scaling near criticality. Bridges QFT renormalisation and statistical mechanics universality.

  • Lesson 5 • Gauge Theories and the Standard Model

    Constructs non-Abelian gauge theories and the electroweak and strong interactions. Higgs mechanism and spontaneous symmetry breaking are treated in detail.

Certification

Your valid completion certificate

This course is for you:

  • Physics undergraduates: ready to move beyond introductory coursework into theory.

  • Graduate school applicants: building the depth required to succeed in PhD programmes.

  • Self-taught science enthusiasts: committed to mastering physics at a serious level.

  • Engineers shifting to research: seeking the theoretical grounding that academia demands.

  • Working scientists: filling gaps left by narrowly focused graduate training.

  • Career changers with strong mathematics background: drawn to fundamental questions about how nature works.

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