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Modern Physics Course
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Modern Physics Course

Master the theoretical framework that defines modern physics, from quantum mechanics and special relativity to nuclear structure and quantum field theory. This course takes you from the failures of classical physics all the way to the Standard Model and beyond. Whether you are advancing your academic career or deepening your scientific foundation, this is the most comprehensive modern physics programme available.

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What you will learn:

You will build a rigorous understanding of quantum mechanics, starting with wave functions and the Schrödinger equation and extending to three-dimensional systems, atomic structure, and molecular bonding. You will study special relativity, statistical mechanics, and solid-state physics, connecting microscopic quantum behaviour to macroscopic physical properties. The course also covers nuclear and particle physics, quantum field theory, and applications in quantum computing, astrophysics, and laser optics. Numerical methods and experimental techniques are included to give you practical problem-solving tools. By the end, you will have the theoretical depth and analytical skills expected at the graduate level.

How you study in practice Modern Physics Course

How you practise Modern Physics Course

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Course content

8 Chapters • 38 LessonsDuration between 4 and 360 hours (you decide)

Chapter 1See details

Foundations of Modern Physics

  • Lesson 1 • Quantization of Energy

    Presents Planck's quantum hypothesis and Einstein's photon model. Bridges the gap between classical wave theory and discrete energy packets.

  • Lesson 2 • Special Relativity Fundamentals

    Introduces Einstein's two postulates and their logical consequences. Connects to classical mechanics by showing where it remains valid at low speeds.

  • Lesson 3 • Limits of Classical Mechanics

    Identifies where Newtonian mechanics and Maxwell's electromagnetism fail. Sets the stage for understanding why new physics was necessary.

  • Lesson 4 • Relativistic Energy and Momentum

    Derives relativistic expressions for momentum and energy. Demonstrates mass-energy equivalence as a direct consequence of special relativity.

Chapter 2See details

Quantum Mechanics Principles

  • Lesson 1 • Wave Functions and Probability

    Defines the wave function as the fundamental quantum descriptor. Establishes Born's probabilistic interpretation and normalization requirements.

  • Lesson 2 • The Schrodinger Equation

    Derives the time-dependent and time-independent Schrodinger equations. Connects energy quantization to boundary conditions on wave functions.

  • Lesson 3 • Simple Quantum Systems

    Solves exactly solvable models to build physical intuition. Results from these models underpin more complex atomic and molecular systems.

  • Lesson 4 • Dirac Notation and Formalism

    Introduces bra-ket notation as a compact and general quantum language. Prepares students for advanced treatments of spin and multi-particle systems.

  • Lesson 5 • Operators and Observables

    Introduces Hermitian operators as representations of physical quantities. Links eigenvalue equations to measurable outcomes in experiments.

Chapter 3See details

Quantum Mechanics in Three Dimensions

  • Lesson 1 • Angular Momentum in Quantum Mechanics

    Derives quantization of orbital angular momentum from commutation relations. Establishes quantum numbers l and m as labels for angular momentum states.

  • Lesson 2 • Electron Spin

    Introduces intrinsic spin as a purely quantum mechanical property. Extends the quantum number set to include spin and explains the Stern-Gerlach experiment.

  • Lesson 3 • The Hydrogen Atom

    Solves the Coulomb potential problem exactly using spherical coordinates. Produces the full set of hydrogen wave functions and energy levels.

  • Lesson 4 • 3D Schrodinger Equation

    Generalizes the Schrodinger equation to three spatial dimensions. Introduces separation of variables as the primary solution strategy.

  • Lesson 5 • Multi-Electron Atoms

    Applies the Pauli exclusion principle to build up atomic structure. Explains periodic table trends through electron configuration and shell filling.

Chapter 4See details

Atomic and Molecular Structure

  • Lesson 1 • Molecular Bonding Basics

    Describes covalent bonding through quantum mechanical overlap of atomic orbitals. Introduces the Born-Oppenheimer approximation for separating nuclear and electronic motion.

  • Lesson 2 • Perturbation Theory

    Introduces time-independent perturbation theory as a tool for real systems. Applies corrections to hydrogen energy levels from small additional interactions.

  • Lesson 3 • Molecular Spectra

    Analyzes rotational and vibrational energy levels of diatomic molecules. Connects molecular quantum numbers to infrared and microwave spectroscopy.

  • Lesson 4 • Atomic Spectra and Selection Rules

    Explains observed spectral lines using quantum transitions and selection rules. Links photon emission and absorption to changes in quantum numbers.

Chapter 5See details

Statistical Mechanics and Quantum Statistics

  • Lesson 1 • Bose-Einstein Condensation

    Describes the macroscopic occupation of the ground state in bosonic systems. Connects theoretical predictions to experimental observations in ultracold gases.

  • Lesson 2 • Free Electron Model of Metals

    Applies Fermi-Dirac statistics to conduction electrons in metals. Explains heat capacity, electrical conductivity, and the Fermi energy concept.

  • Lesson 3 • Classical Statistical Mechanics Review

    Revisits Maxwell-Boltzmann statistics as the classical limit. Establishes partition functions and free energy as bridges between micro and macro descriptions.

  • Lesson 4 • Blackbody Radiation Revisited

    Derives the Planck distribution using photon statistics as massless bosons. Recovers Wien's law and Stefan-Boltzmann law from the full quantum treatment.

  • Lesson 5 • Quantum Distribution Functions

    Derives Fermi-Dirac and Bose-Einstein distributions from indistinguishability. Contrasts quantum statistics with classical Maxwell-Boltzmann behaviour.

Chapter 6See details

Solid State and Condensed Matter Physics

  • Lesson 1 • Semiconductor Physics

    Analyses intrinsic and extrinsic semiconductors using band theory. Explains carrier concentration, doping, and the p-n junction at the quantum level.

  • Lesson 2 • Electrons in Periodic Potentials

    Applies Bloch's theorem to electrons in a crystal lattice. Derives energy bands and band gaps from the periodic potential.

  • Lesson 3 • Crystal Structure and Lattices

    Introduces Bravais lattices, unit cells, and reciprocal space. Provides the geometric foundation for all subsequent band structure calculations.

  • Lesson 4 • Superconductivity Fundamentals

    Introduces the phenomenology of superconductivity and Cooper pair formation. Covers the Meissner effect and the BCS theory at a conceptual level.

  • Lesson 5 • Phonons and Lattice Vibrations

    Quantises lattice vibrations as phonons using the harmonic approximation. Connects phonon dispersion to thermal and acoustic properties of solids.

Chapter 7See details

Nuclear and Particle Physics

  • Lesson 1 • Radioactive Decay

    Analyses alpha, beta, and gamma decay using quantum tunnelling and selection rules. Derives decay laws and applies them to half-life calculations.

  • Lesson 2 • Nuclear Reactions and Fission

    Covers Q-value calculations and cross sections for nuclear reactions. Explains fission chain reactions and the physics of nuclear energy release.

  • Lesson 3 • Elementary Particles and Forces

    Classifies quarks, leptons, and gauge bosons within the Standard Model. Describes the four fundamental forces and their mediating particles.

  • Lesson 4 • Nuclear Structure

    Describes the nucleus in terms of protons, neutrons, and binding energy. Introduces the liquid drop and shell models as complementary descriptions.

  • Lesson 5 • Particle Accelerators and Detectors

    Explains how accelerators produce high-energy collisions for particle discovery. Describes detector technologies used to identify and measure particle properties.

Chapter 8See details

Quantum Field Theory Introduction

  • Lesson 1 • Renormalisation Concepts

    Explains ultraviolet divergences and the renormalisation procedure at a conceptual level. Introduces running coupling constants and the renormalisation group idea.

  • Lesson 2 • Quantum Electrodynamics Overview

    Introduces QED as the quantum field theory of electrons and photons. Explains gauge invariance and the minimal coupling of matter to the electromagnetic field.

  • Lesson 3 • Classical Field Theory Review

    Recasts classical mechanics in terms of fields using the Lagrangian formalism. Establishes Noether's theorem as the link between symmetries and conservation laws.

  • Lesson 4 • Quantisation of the Scalar Field

    Promotes the classical scalar field to a quantum operator using canonical quantisation. Introduces creation and annihilation operators and the Fock space of particle states.

  • Lesson 5 • Path Integral Formulation

    Presents Feynman's path integral as an alternative to operator quantisation. Connects the classical action to quantum amplitudes through sum over histories.

Certification

Your valid completion certificate

This course is for you:

  • Undergraduate physics students: ready to go deeper than their coursework allows.

  • Aspiring graduate students: building the theoretical foundation for competitive PhD applications.

  • Electrical engineers: seeking the quantum mechanics behind semiconductor and device physics.

  • Career changers: moving from classical engineering into quantum technology or research roles.

  • Science enthusiasts: committed to understanding modern physics with full mathematical rigor.

  • Working physicists: refreshing and formalizing knowledge across areas outside their specialty.

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