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γ(v)

Special Relativity

What stays true for every observer, once nothing outruns light.

Lorentz TransformationsTranslating position and time between observers moving relative to each other.Coming soonTime Dilation & Length ContractionWhy moving clocks run slow and moving rulers run short.Coming soonRelativistic Energy & MomentumRedefining momentum and energy so conservation still holds near light speed.Coming soonSpacetime DiagramsReading simultaneity, causality, and worldlines off a Minkowski diagram.Coming soon