Free Course Image General Relativity of Einstein

Free online courseGeneral Relativity of Einstein

Duration of the online course: 30 hours and 22 minutes

New

Understand spacetime, gravity and black holes with a free online course in General Relativity, with exercises and optional certificate to boost your skills.

In this free course, learn about

  • Geometric view of physics: spacetime as the arena for relativistic dynamics
  • Tensor basics: indices, transformations, contractions, and physical meaning
  • Special relativity tools: 4-velocity invariant norm and the metric tensor
  • Volume elements, tensor densities, and conservation laws in curved spacetime
  • Stress-energy tensor (e.g., T00 as energy density) and its role as gravity source
  • Christoffel symbols, covariant derivatives, and parallel transport
  • Equivalence principle as the core physical motivation for general relativity
  • Lie transport, symmetries, and Killing vectors; conserved quantities from symmetries
  • Geodesics as free-fall trajectories; connection to gravity as geometry
  • Spacetime curvature: Riemann curvature and its physical effects (tidal forces)
  • Einstein field equation and key derivation ideas connecting curvature to stress-energy
  • Linearized gravity: weak-field limit, static approximation, and dynamic sources
  • Gravitational radiation: waves, generation, and basic properties
  • Cosmology, compact spherical sources, and black holes (Schwarzschild and beyond)

Course Description

General Relativity can feel like a wall of equations until you see the simple idea behind it: gravity is not a mysterious force acting at a distance, but the geometry of spacetime itself. In this free online course, you build that geometric intuition step by step and learn how to translate it into the mathematical language physicists use to make real predictions.

The course begins by reframing physics through symmetry, invariants and spacetime viewpoints that unify motion and gravity. From there, you develop comfort with tensors, the natural tools for expressing physical laws in any coordinate system. Rather than treating tensors as abstract symbols, you learn why they matter: they keep your equations meaningful when you change perspective, and they reveal what is truly physical versus what is just a coordinate choice.

As the ideas deepen, you connect conservation laws to volume elements and curved geometry, then move into the objects that carry physical content in relativity, such as the stress-energy tensor, and the geometric quantities that encode how coordinates and vectors vary in curved spacetime. With the equivalence principle as a guiding theme, the course shows how free fall, inertial motion and gravitational effects become the same story told in the right language, leading naturally to concepts like parallel transport, symmetries in spacetime and geodesics.

You then reach the heart of the subject: curvature and the Einstein field equation, including insight into why the equation has the form it does and how matter tells spacetime how to curve. With that foundation, you explore approximations that make the theory usable in practical settings, including linearized gravity and the transition from static limits to dynamical sources. From there, the course opens the door to gravitational radiation, cosmology, compact spherical sources and the physics of black holes, tying mathematical structure to phenomena that shape modern astronomy and cosmology.

Exercises throughout help you check understanding and gain fluency, whether you are strengthening school physics knowledge, preparing for university-level studies, or revisiting relativity with clearer intuition. By the end, you will be able to read core formulas of General Relativity with confidence and understand what they say about the universe.

Course content

  • Video class: 1. Introduction and the geometric viewpoint on physics. 1h08m
  • Exercise: What is the recommended textbook for the course?
  • Video class: 2. Introduction to tensors. 1h19m
  • Exercise: What is an invariant feature of the 4-velocity in special relativity?
  • Video class: 3. Tensors continued. 1h11m
  • Exercise: What is the Metric Tensor in Special Relativity?
  • Video class: 4. Volumes and volume elements; conservation laws. 1h19m
  • Exercise: What is a key concept of tensors according to the lecture on working with them?
  • Video class: 5. The stress energy tensor and the Christoffel symbol. 1h20m
  • Exercise: What is the component T00 of the stress-energy tensor in the stress-energy tensor for dust, according to the lecture?
  • Video class: 6. The principle of equivalence. 1h20m
  • Exercise: What is a Christoffel symbol and its role in tensors?
  • Video class: 7. Principle of equivalence continued; parallel transport. 1h21m
  • Exercise: What is the main physical principle underlying general relativity that was introduced in the lecture?
  • Video class: 8. Lie transport, Killing vectors, tensor densities. 1h16m
  • Exercise: What principle did the Apollo program test by dropping a hammer and a feather on the moon?
  • Video class: 9. Geodesics. 1h20m
  • Video class: 10. Spacetime curvature. 1h20m
  • Video class: 11. More on spacetime curvature. 1h19m
  • Video class: 12. The Einstein field equation. 1h17m
  • Video class: 13. The Einstein field equation (variant derivation). 1h18m
  • Video class: 14. Linearized gravity I: Principles and static limit. 1h14m
  • Video class: 15. Linearized gravity II: Dynamic sources 1h15m
  • Video class: 16. Gravitational radiation I 1h25m
  • Video class: 17. Gravitational radiation II 1h30m
  • Video class: 18. Cosmology I 1h28m
  • Video class: 19. Cosmology II 1h36m
  • Video class: 20. Spherical compact sources I 1h03m
  • Video class: 21. Spherical compact sources II 1h13m
  • Video class: 22. Black holes I 1h26m
  • Video class: 23. Black holes II 1h11m

This free course includes:

30 hours and 22 minutes of online video course

Digital certificate of course completion (Free)

Exercises to train your knowledge

100% free, from content to certificate

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