Physics · Glossary

What is Events and simultaneity?

Definition 4.3 University Physics — Year 3 · Chapter 4 — Relativistic Kinematics

An event is a point occurrence: a definite place and a definite instant — a spark, a detector click, a decay. Each inertial frame assigns an event its coordinates (t,x,y,z)(t, x, y, z), using rulers at rest in the frame and synchronised clocks distributed through it. Two events are simultaneous in a frame when that frame’s clocks assign them the same tt — and the first casualty of the postulates is that this notion depends on the frame.

Two strikes marking both the train and the track. The ground observer, midway between the marks, receives the flashes together: simultaneous for her. The passenger runs toward flash B; it reaches him first, and — equidistant from the marks in his own frame — he concludes B struck first. Simultaneity is relative.
Two strikes marking both the train and the track. The ground observer, midway between the marks, receives the flashes together: simultaneous for her. The passenger runs toward flash B; it reaches him first, and — equidistant from the marks in his own frame — he concludes B struck first. Simultaneity is relative.

Examples

Example 4.4 (The train and the two lightning bolts)

Lightning strikes both ends of a fast train, leaving marks on train and track. For the observer on the ground, midway between the marks, the two flashes arrive together: the strikes were simultaneous for her. The passenger seated at the train’s midpoint, however, is moving toward one flash and away from the other; travelling at cc in his frame too, the forward flash reaches him first — and since he sits equidistant from the two marks on the train, he must conclude the forward strike happened earlier. Neither is wrong: simultaneity of separated events is not a fact about the world but about the frame. Every relativistic “paradox” dissolves here.

Example 4.16 (The travelling twin)

One twin flies to a star 88 light-years away at 0.8c0.8c (γ=5/3\gamma = 5/3) and returns. Earth time: 2×8/0.8=20yr2 \times 8/0.8 = 20\,\mathrm{yr}. The traveller’s proper time: 20/γ=12yr20/\gamma = 12\,\mathrm{yr} — eight years younger, and no paradox: the twins’ situations are not symmetric, since one worldline is straight (inertial throughout) and the other has a kink at turnaround. Between two fixed events, the straight worldline is the one of longest proper time — in spacetime’s geometry, the detour is shorter-lived. The effect is measured routinely: atomic clocks flown around the world disagree with their stay-at-home siblings by exactly the predicted nanoseconds (Problem 4.1).

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