Einstein's Theory of Relativity
When space and time become relative — a revolution that transformed our understanding of the Universe
Albert Einstein revolutionized physics in the early 20th century with two theories that changed our view of the universe. Special relativity (1905) unifies space and time into a space-time continuum, while general relativity (1915) reveals that gravity is not a force, but a curvature of this space-time caused by mass.
Special Relativity
Space and time are no longer absolute
The most famous equation in physics: energy equals mass multiplied by the speed of light squared.
Central idea: Time and space are not absolute, but depend on the speed at which one travels. The only absolute is the speed of light: 299,792,458 m/s.
Principle of Relativity
The laws of physics are identical for all observers in uniform linear motion (no acceleration). No experiment can detect absolute motion.
Constance de c
Light in a vacuum always travels at 299,792,458 m/s, regardless of the speed of the object emitting or receiving it. This is an insurmountable limit.
Strange consequences
Concrete examples
Cosmic muons: These particles created in the upper atmosphere should decay before reaching the ground, but thanks to time dilation (they travel at ~0.99c), they survive until they reach the ground.
GPS: Satellites move quickly and are subject to less gravity → their clocks run differently. Without relativistic corrections, GPS would drift by 10 km per day!
Einstein's postulates
1. Principle of relativity (Galilean extension): The laws of mechanics AND electromagnetism are identical in all inertial reference frames.
2. Invariance of c: The speed of light in a vacuum, c = 299,792,458 m/s, is independent of the motion of the source and the observer.
Lorentz transformation
Replaces Galilean transformations to connect two reference frames moving relative to each other at velocity v:
Mathematical Consequences
- Time dilation: Δt' = γ × Δt — If v → c, then γ → ∞: time slows down dramatically
- Length contraction: L' = L / γ — If v → c, then L' → 0
- Addition of velocities: u' = (u + v) / (1 + uv/c²) — Ensures that no velocity exceeds c
- Total energy: E² = (mc²)² + (pc)² — If p = 0: E = mc²
Minkowski space-time
The three spatial dimensions plus one temporal dimension form a four-dimensional continuum. The space-time interval is invariant:
Quantitative Applications
- GPS: Satellites at v ≈ 3.9 km/s → time dilation of -7 μs/day (special relativity) + 45 μs/day (general relativity) = +38 μs/day net
- Cosmic muons: Rest lifetime τ₀ = 2.2 μs, but observed on the ground thanks to γ ≈ 10-100
- LHC: Protons at 0.999999991c → γ ≈ 7500, effective mass 7500× greater
General Relativity
Gravity as a curvature of space-time
Revolutionary idea: Gravity is not a force, but a distortion of space-time caused by the presence of mass and energy.
Mass distorts space-time like a ball on a stretched sheet.
Principle of Equivalence
Being in a gravitational field is equivalent to being in an accelerated reference frame. In a rocket accelerating at 9.8 m/s², you feel exactly the same as you do on Earth.
General Covariance
The laws of physics have the same form in all reference frames (accelerated or not). Physics does not depend on the chosen coordinate system.
Simple analogy
Imagine a sheet stretched out representing space-time. Place a bowling ball (a star) on it: it distorts the sheet. A marble (planet) rolling nearby will follow the curve created → this is the orbit! Planets do not "fall" toward the Sun because of a force; they simply follow the most natural path in curved space-time.
Einstein's Equation
Meaning: "The geometry of space-time (left side) is determined by the distribution of matter and energy (right side)."
Founding Principles
- Principle of equivalence (weak): Inertial mass = gravitational mass. m_inertia (F=ma) ≡ m_gravity (F=GMm/r²)
- Equivalence principle (strong): Locally (small region), it is impossible to distinguish between acceleration and gravity through any physical experiment.
- General covariance principle: Physical laws are expressed by tensor equations that are valid in any reference frame.
Schwarzschild metric (static black hole)
Experimental Tests
- Mercury's perihelion precession: +43 arc seconds per century (unexplained by Newton)
- Light deflection by the Sun: 1.75 arc seconds (measured during the 1919 eclipse by Eddington)
- Gravitational redshift: Δν/ν = -GM/(rc²), verified with atomic clocks (Pound-Rebka, 1959)
- Gravitational waves: Direct detection 2015 (GW150914, merger of black holes 36+29 M☉)
- Image of black hole M87*: Event Horizon Telescope (2019)
Friedmann equations (Cosmology)
The Equation That Describes the Universe
This tensor equation relates the curvature of space-time (left side) to the distribution of matter and energy (right side). It predicts black holes, gravitational waves, the expansion of the Universe, and the Big Bang. It is one of the most beautiful and powerful equations in all of physics.
Verified Predictions
A century of spectacular experimental confirmations
Modern Applications
Relativity is not just an abstract theory—it is essential to the functioning of everyday technologies.
GPS
Without relativistic corrections (restricted + general), GPS would drift by 10 km per day. Every smartphone uses relativity!
Particle Accelerators
At the LHC, protons reach γ ≈ 7500. Their effective mass is 7500 times greater than at rest.
Nuclear Energy
E = mc² explains the energy released by nuclear fission and fusion. 1 kg of matter = 90 petajoules.
Cosmology
Big Bang, age of the Universe (13.8 billion years), dark energy, dark matter—everything is based on general relativity.
Detection of Exoplanets
Gravitational microlensing allows planets to be detected by observing the bending of light.
LIGO/Virgo
Gravitational wave detectors capable of measuring deformations of 10⁻²¹ meters.