Physic Labs

Theory of relativity

Time dilation and length contraction

Compare moving clocks and rods with the laboratory frame as β=v/c\beta = v/c varies; verify Δt=γ Δτ\Delta t = \gamma\,\Delta\tau and L=L01−β2L = L_0\sqrt{1-\beta^2} against the quantitative panel.

Undergraduate

Equipment

  • “Speed β = v/c” slider driving the clock-and-rod figure
  • “Model parameter” and second “Speed β” sliders for the relation plot
  • “Pause” animation and “Reset view” buttons
  • β and γ readout plus the 1/γ label on the figures

Procedure

  1. Watch the moving clock run slow

    Sweep “Speed β = v/c” from 0 to 0.95: the moving clock's ticks stretch out compared with the lab clock. Read γ on the readout and check Δt=γ Δτ\Delta t = \gamma\,\Delta\tau; drag the canvas to rotate the scene if needed.

  2. Measure the rod's contraction along the motion

    At the same β, look at the rod: its projected length along the motion shrinks while the transverse size stays fixed. Compare with L=L0/γL = L_0/\gamma and stress that this is a measurement effect between frames, not a mechanical deformation.

  3. Read the γ(β) plot and the non-relativistic limit

    In the “Quantitative relation” panel, sweep the second β slider: γ departs from 1 by only parts per thousand at small β but blows up as β → 1. Use γ=1/1−β2\gamma = 1/\sqrt{1-\beta^2} to estimate which β gives a 1% correction and explain why the effect is invisible at everyday speeds.

Simulation

Experiment history

In 1905 Albert Einstein built special relativity on two postulates, and time dilation with length contraction emerged as consequences of the Lorentz transformations — transformations Hendrik Lorentz had written in 1904 within ether theory, while George FitzGerald had suggested a physical contraction in 1889 to explain the Michelson–Morley result (1887). The difference is that Einstein derived the effects from principles rather than ad-hoc ether assumptions. Direct confirmations include the Ives–Stilwell experiment (1938) measuring the Doppler shift of fast ions, the extended lifetime of cosmic-ray muons, and the Hafele–Keating experiment (1971) flying atomic clocks around the Earth — all matching γ to high precision.

Related physicists

Related library topics