Physic Labs

Theory of relativity

The equivalence principle

Compare the motion of a free body inside an accelerating frame with motion in a uniform gravitational field, and verify that locally the two descriptions are indistinguishable — the equivalence principle at the heart of general relativity.

Advanced

Equipment

  • 3D canvas: accelerating elevator plus curved-grid view near a mass
  • Slider “accelerating frame” (frame acceleration)
  • Slider “Tốc độ thời gian” (animation speed) and “Tạm dừng” button

Procedure

  1. Release a body in the accelerating frame

    Set a moderate acceleration on the “accelerating frame” slider and watch the free body's path in the elevator. In the accelerated frame it appears to fall with acceleration aa, exactly as if a uniform gravitational field g=ag=a pulled it — no local experiment distinguishes the two.

  2. Match acceleration to gravity

    Raise and lower the acceleration and compare with the warped-grid view near the mass. Find the slider setting where the apparent fall in the elevator reproduces free fall in the gravitational field, confirming aframe↔agrava_{\mathrm{frame}}\leftrightarrow a_{\mathrm{grav}}.

  3. Probe the local limit

    Ask what would spoil the equivalence: over a large region, tidal effects — the variation of g from place to place — betray real gravity. Pause the model and explain why the equivalence principle holds only in a sufficiently small neighborhood and is the seed of curved-spacetime gravity.

Simulation

Experiment history

Einstein called the idea “the happiest thought of my life”: in 1907 he realized that a person falling freely feels no gravity, so a uniform gravitational field can be cancelled — or mimicked — by a change of reference frame. Elevator and rocket thought experiments built on this led him through eight years of work to the field equations of general relativity, published in November 1915. The principle has a precise experimental ancestry: Galileo's legendary comparisons of falling bodies and Newton's pendulum tests already showed inertial and gravitational mass coincide; Loránd Eötvös's torsion-balance measurements from the 1880s pushed the equivalence to one part in 10910^9, and modern missions like MICROSCOPE (2016) reached 10−1510^{-15}.

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