General Relativity
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General Relativity

Spacetime, geometry, and gravity explained step by step

General Relativity

Spacetime, explained step by step

Build the geometry first, then use it to understand gravity, black holes, gravitational waves, and the expanding universe.

Coming soon5 stages
gspacetime
ds² = gμν dxμ dxν
Gμν = 8πTμν
space
time

Contents

The route through GR

Chapters will be added in this order.

01

3 chapters

Foundations

Build the mathematical and physical language needed for curved spacetime.

Chapter 01x^μ

Spacetime

Describe events, intervals, light cones, and causality.

Coming soon
Chapter 02T^μν

Vectors and tensors

Learn the objects that make physical laws coordinate-independent.

Coming soon
Chapter 03γ(λ)

Curves and motion

Move from ordinary trajectories to geometric paths through spacetime.

Coming soon
02

3 chapters

Differential geometry

Turn curved spaces into a precise language for physics.

Chapter 04M

Manifolds

Describe spaces locally with coordinates and globally with charts.

Coming soon
Chapter 05gμν

Metrics

Measure distances, times, angles, and causal structure geometrically.

Coming soon
Chapter 06∇, R

Connections and curvature

Compare vectors at different points and measure geometric bending.

Coming soon
03

3 chapters

General relativity

Build Einstein’s theory from the equivalence principle and an action.

Chapter 07g

The equivalence principle

Understand why gravity can be described as spacetime geometry.

Coming soon
Chapter 08Gμν

Einstein equations

Relate spacetime curvature to matter and energy.

Coming soon
Chapter 09δS = 0

Geodesics

Derive free fall as extremal motion in curved spacetime.

Coming soon
04

3 chapters

Spacetime solutions

Explore the geometries that describe stars, black holes, and the universe.

Chapter 10rₛ

Schwarzschild spacetime

Study the geometry outside a spherical, non-rotating body.

Coming soon
Chapter 11Δt

Black holes

Understand horizons, singularities, and causal structure.

Coming soon
Chapter 12a(t)

Cosmology

Apply Einstein’s equations to an expanding homogeneous universe.

Coming soon
05

3 chapters

Gravitational phenomena

Connect the geometry to observable effects and experiments.

Chapter 13hμν

Gravitational waves

Describe propagating distortions of spacetime and their detection.

Coming soon
Chapter 14z

Lensing and redshift

Calculate how gravity bends light and changes observed frequencies.

Coming soon
Chapter 15Δτ

Tests of relativity

Compare geometric predictions with measurements in the solar system.

Coming soon
General Relativity — a route from spacetime geometry to Einstein’s universe.