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Complete Theory of General Relativity in Everyday Language
Rating: 3.6 out of 5(2 ratings)
242 students

Complete Theory of General Relativity in Everyday Language

Einstein's General Relativity, Explained Simply I Riemannian Geometry I Einstein Field Equations
Created byVaibhav Singh
Last updated 1/2026
English

What you'll learn

  • Gain knowledge of the underlying concepts that make up General Relativity
  • The History of General Relativity
  • Learn about the man behind the theory: Albert Einstein
  • Understand concepts like Time Dilation and Curved Geometry
  • Riemannian Geometry
  • Einstein Field Equations
  • Special Relativity

Course content

6 sections28 lectures1h 13m total length
  • Introduction0:28
  • Setting the Historical Context- Newton vs Einstein2:50
  • Crash Course in Special Relativity7:48
  • Gravity as Geometry—A Radical Reimagining2:44
  • Introduction to Gravitational Time Dilation0:46

    Explore how gravity slows time, making clocks tick slower deeper in a gravitational well. See GPS evidence and experiments that compare sea level and mountain elevations.

  • Test your knowledge!

Requirements

  • Science background is not required, this course is in everyday language, going from introduction to relativity to advanced concepts

Description

This course contains the use of artificial intelligence

This course is a comprehensive exploration of Albert Einstein’s most profound legacy: the reimagining of the universe as a geometric masterpiece. We begin by tracing the historic shift from Isaac Newton’s "invisible force" of gravity to Einstein’s radical realization that space and time are not separate entities, but are woven together into a single, four-dimensional fabric called spacetime. You will discover how mass and energy actually warp this fabric, turning gravity from a mysterious pull into a physical property of the world around us.

The curriculum then dives into the mind-bending reality of Gravitational Time Dilation, proving that your sense of time is dictated by your location in a gravitational well. You will explore the "living mathematics" of Riemannian geometry, where we define geodesics—the straightest possible paths in a curved world—to understand why planets orbit and apples fall. We simplify the intimidating Einstein Field Equations, breaking down the symbols that serve as the universal rulebook: telling mass-energy how to curve spacetime, and curved spacetime how to move mass-energy.

Finally, we venture into the most extreme corners of the cosmos, from the "blunder" of the Cosmological Constant that now explains the accelerating expansion of our universe to the terrifying reality of Black Holes. You will stand at the edge of the Event Horizon and Peer into the Singularity, where our current equations fail and the search for a "Theory of Everything" begins.

Who this course is for:

  • College Students
  • High School Students
  • Science Enthusiasts
  • Reserchers