Summary

General Principles

Principle of Relativity

The laws of physics are the same in all inertial reference frames.

  • The speed of light c is the same in all inertial reference frames.

  • No particle or causal influence can travel at a speed greater than c.

Solving Relativity Problems

  • Base the analysis on events.

  • Time intervals can often be found using time dilation.

  • Distances can often be found using length contraction.

  • Use the Lorentz transformations for general problems.

Important Concepts

Space

Spatial measurements depend on the motion of the experimenter relative to the events. An object’s length is the difference between simultaneous measurements of the positions of both ends.

Proper length ℓ is the length of an object measured in a reference frame in which the object is at rest. The object’s length in a frame in which the object moves with velocity v is

L=1−β2ℓ≤ℓ

This is called length contraction.

Momentum

The law of conservation of momentum is valid in all inertial reference frames if the momentum of a particle with velocity u is p=γpmu, where

γp=1/1−u2/c2

The momentum approaches ∞ as u→c.

The figure illustrates relativistic momentum graphically.

Invariants are quantities that have the same value in all inertial reference frames.

Spacetime interval: s2=(c Δt)2−(Δx)2

Particle rest energy: E0 2=(mc2)2=E2−(pc)2

Time

Time measurements depend on the motion of the experimenter relative to the events. Events that are simultaneous in reference frame S are not simultaneous in frame S′ moving relative to S.

Proper time Δτ is the time interval between two events measured in a reference frame in which the events occur at the same position. The time interval between the events in a frame moving with relative velocity v is

Δt=Δτ/1−β2≥Δτ

This is called time dilation.

Energy

The law of conservation of energy is valid in all inertial reference frames if the energy of a particle with velocity u is E=γpmc2=E0+K.

Rest energy E0=mc2

Kinetic energy K=(γp−1)mc2

The figure illustrates relativistic kinetic energies graphically.

Mass-energy equivalence

Mass m can be transformed into energy ΔE=mc2.

Two arrows are kept side by side. The arrow on the left points upward, while the arrow on the right points downward.

Energy can be transformed into mass m=ΔE/c2.

Applications

An event happens at a specific place in space and time. Spacetime coordinates are (x, t) in frame S and (x′, t′) in frame S′.

A reference frame is a coordinate system with meter sticks and clocks for measuring events.

The Lorentz transformations transform spacetime coordinates and velocities between reference frames S and S′.

x′=γ(x−vt)x=γ(x′+vt′)y′=yy=y′z′=zz=z′t′=γ(t−vx/c2)t=γ(t′+vx′/c2)u′=u−v1−uv/c2u=u′+v1+u′v/c2

where u and u′ are the x- and x′-components of an object’s velocity.

β=v/c and γ=1/1−v2/c2=1/1−β2
The figure illustrates the velocity of a moving object with respect to two reference frames.

Terms and Notation