REL-22

Length contraction

Proper length seen in motion.

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GoverningLength contraction

Governing equation

L=L_0/\gamma

where

L0: L0 (m)
beta: beta (—)
L: Length contraction (m)

Lecture brief

Historical brief

Einstein’s 1905 Lorentz kinematics and 1915 field equation, then Schwarzschild (1916) and Hawking temperature, recast time, mass and gravity. The lab computes dilation, E=mc² and horizon scales. This sheet (REL-22 — Length contraction) is the form associated with Length contraction. Working symbols: $L0$ , $beta$ $\rightarrow$ $L$ . Proper length seen in motion. Pedagogical SI sheet with a live model and a swept parameter.

Purpose

Purpose: compute

L

from

L0

beta

in Relativity via

L=L_0/\gamma

Proper length seen in motion. Use it when a real relativity question must be answered in SI before a code check.

Live realistic example

In symbols

Live case. Given

L0 = 1.000\,\mathrm{m}

beta = 0.600\,\mathrm{—}

, the governing relation

L=L_0/\gamma

yields

L = 0.800\,\mathrm{m}

. One governing identity, SI units, a single sweep on the sheet. Move a slider: the numbers are this situation, not a canned story.

Calculator

Inputs

L0 L01 mbeta beta0.6 —

Outputs

Length contraction L0.800 m

Reading speed

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Narration of this film

One governing identity, SI units, a single sweep on the sheet.

Proper length seen in motion. Pedagogical SI sheet with a live model and a swept parameter.

Reading speed

Watch on YouTube