Spacetime and the cosmos

1905

Special relativity

Albert Einstein

What would you see if you could ride alongside a beam of light?

Einstein took two rules seriously: physics is the same for everyone moving steadily, and everyone measures the same speed of light. The price is that moving clocks run slow and moving rulers shrink. Time and space depend on who is measuring.

First, make a guess

At 87% of light speed, the moving clock ticks…

How they figured it out

At sixteen, Einstein imagined chasing a light beam. If he caught up, he would see a frozen wave, and Maxwell’s equations do not allow such a thing. The puzzle stayed with him for ten years.

In May 1905, working as a “technical expert, third class” at the patent office in Bern, he talked the problem through with his friend Michele Besso and suddenly saw it: two events that are simultaneous for one person need not be for another. Time itself depends on how you move. He wrote the paper in about five weeks. It has no references at all.

The equation

Δt′=Δt1−v2/c2\Delta t' = \frac{\Delta t}{\sqrt{1 - v^2/c^2}}

The faster a clock moves past you, the slower you see it tick.

Everyday echoParticles from space reach the ground only because their clocks run slow.

See it in real life

Particles that should not reach the ground

Cosmic rays make muons about 15 km up. A muon lives about 2.2 microseconds: at nearly light speed that is only about 660 m of travel. Yet detectors at sea level catch them all the time. Moving that fast, their clocks run slow.

Where engineers use it

  • Particle accelerators

    Designs at CERN account for particles living longer and getting heavier as they near light speed.

  • GPS

    Satellite clocks run slow by about 7 microseconds a day from their speed alone.

Worked example: A fast muon

  1. At v=0.995cv = 0.995c: γ=1/1−0.9952≈10\gamma = 1/\sqrt{1 - 0.995^2} \approx 10
  2. Its 2.2 µs lifetime becomes about 22 µs, enough to reach the ground.