Modern PhysicsSpecial Relativity

The Postulates of Relativity

The laws of physics and the speed of light are the same in every inertial frame.

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In Galilean relativity, velocities simply add: a ball thrown forward at 20 m/s from a train moving at 30 m/s goes 50 m/s relative to the ground. And no experiment with balls and springs inside a smoothly moving train can tell you how fast the train is going. Then Maxwell's equations predicted that light moves at one definite speed, $c = 1/\sqrt{\mu_0\varepsilon_0}$. Relative to what? Physicists assumed an invisible medium, the “ether”. In 1887 Michelson and Morley's interferometer looked for Earth's motion through it and found none.

Key idea

Einstein's two postulates (1905):
  1. The laws of physics are the same in every inertial (non-accelerating) frame.
  2. The speed of light in a vacuum is $c = 3.00 \times 10^8$ m/s in every inertial frame, whatever the motion of the source or the observer.
Since $c$ must come out the same for everyone, our everyday rules for adding velocities, and for time and distance themselves, have to give way at high speeds.

Why it works

The second postulate follows from the first once you trust Maxwell's equations. They are laws of physics, so by postulate 1 they hold in every inertial frame. And they give the speed of light as $1/\sqrt{\mu_0\varepsilon_0}$, built from two constants with no mention of anyone's velocity. So every inertial observer must measure the same $c$. The price is high: if two observers moving relative to each other time the same flash and both get $c$, they cannot also agree about distances and times in the everyday way. The rest of this unit works out what they do agree on.
A light clock bounces a pulse between two mirrors. Seen from the ground, the moving clock's light must travel a longer, slanted path at the same speed $c$, so each tick takes longer. Constant $c$ already forces time to stretch.

Worked examples

Worked example: A headlight on a fast ship

A spaceship moving at $0.50c$ toward Earth turns on a forward headlight. How fast does the light move according to the crew, and according to observers on Earth?
  1. By postulate 2, the crew measures $c$, since the light moves through vacuum.
  2. By postulate 2 again, Earth observers also measure $c$, not $1.5c$. The source's motion does not add to light's speed.

Answer: $3.00 \times 10^8$ m/s for both

Worked example: Timing light in a moving cabin

A ship moves past Earth at $0.80c$. A light pulse crosses its 30 m cabin, front to back. How long does the crossing take, as measured by the crew?
  1. In the crew's own frame the cabin is at rest, and by postulate 1 their physics is ordinary.
  2. By postulate 2 the pulse moves at $c$: $t = \frac{30\ \text{m}}{3.00 \times 10^8\ \text{m/s}} = 1.0 \times 10^{-7}$ s.

Answer: $100$ ns, exactly as if the ship were parked

The evidence is strong. In 1964 an experiment at CERN timed gamma rays given off by neutral pions moving at $0.99975c$. Galilean addition would predict nearly $2c$ for photons sent forward; the measured speed was $c$, to within about one part in ten thousand.

Common mistake

Thinking light from a moving source travels faster than $c$, the way a ball thrown from a train goes faster than the throw. That rule works for balls at everyday speeds, but light's speed is the same for every inertial observer whatever the source does. A check: binary stars orbit fast toward and away from us, yet their light arrives at the same speed; if it did not, their images would scramble in ways never seen.

Common mistake

Reading postulate 1 as “everything is relative”. It says the laws are the same in every inertial frame. Some quantities, like $c$ and (as you will see) the spacetime interval, are the same for everyone.

Practice

Pass with 3 right answers, the last 2 in a row. Each right answer earns 1 XP.

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Sources and further reading

  • OpenStax University Physics Volume 3, 5.1 Invariance of Physical Laws
  • MIT OpenCourseWare 8.20 Introduction to Special Relativity (January IAP 2005)
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