
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.
What your team will master:
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.
How your team learns in practice Theoretical Physicist Course
How your team practises Theoretical Physicist Course
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Course content
8 Chapters • 40 LessonsDuration between 4 and 360 hours (you decide)
Chapter 1HideHide detailsSee detailsMathematical Foundations for Physics
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 emphasised.
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 2HideHide detailsSee detailsClassical Mechanics
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 3HideHide detailsSee detailsElectrodynamics
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 4HideHide detailsSee detailsSpecial and General Relativity
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 5HideHide detailsSee detailsQuantum Mechanics
Quantum Mechanics
Lesson 1 • Schrodinger 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 6HideHide detailsSee detailsStatistical Mechanics and Thermodynamics
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 7HideHide detailsSee detailsQuantum Field Theory
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 8HideHide detailsSee detailsAdvanced Topics in Theoretical Physics
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.
Your valid completion certificate
This course is for you:
Physics undergraduates: ready to push beyond introductory coursework into theory.
Graduate school applicants: building the depth needed to succeed in PhD programmes.
Self-taught science enthusiasts: committed to mastering physics at a serious level.
Engineers pivoting to research: seeking the theoretical grounding academia demands.
Working scientists: filling gaps left by narrowly focused graduate training.
Maths-strong career changers: drawn to fundamental questions about how nature works.
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