Einstein Equivalence Principle
Also known as: Equivalence principle · EEP · Weak/strong equivalence
Inside a sealed elevator you cannot tell gravity from acceleration: a falling lab and a coasting rocket give identical physics. Because gravitational and inertial mass are the same number, everything falls at the same rate — so 'gravity' is locally just the geometry of an accelerating frame.
Side-by-side: a box accelerating in empty space vs a box at rest on a planet. A released ball traces the identical parabola in both, showing the two scenes are physically indistinguishable.
Equivalent forms
The deepest free lunch in physics: equating two a-priori unrelated masses turns gravity from a force into the curvature of spacetime.
Einstein called it 'the happiest thought of my life' (1907): a person in free fall feels no weight. Galileo had already argued all bodies fall alike; Eotvos torsion-balance experiments (1885-1909) verified m_i = m_g to 1 part in 10^9. Einstein elevated this coincidence to a principle, the seed of general relativity.
- Free-fall 'zero-g' aircraft and drop towers reproduce weightlessness by removing the floor's normal force, not gravity.
- Gravitational redshift of clocks follows directly and underlies GPS timing.
- Inertial navigation accelerometers cannot separate gravity from acceleration — the principle in engineering form.
- MICROSCOPE satellite (2017/2022) tested EEP to 1 part in 10^15.
- 'Astronauts float because there's no gravity.' — Gravity at the % of surface value; they float because they are in free fall.
- 'Equivalence is exact everywhere.' — Only locally: tidal forces (curvature) reveal a real gravitational field over extended regions.
- 'It just means heavy things fall fast.' — It means they fall at the SAME rate regardless of mass.
- Newton's law in a gravitational field: .
- Observation (Galileo, Eotvos): to extreme precision for every material.
- Therefore independent of mass or composition — all bodies share one trajectory.
- A uniformly accelerating frame (rocket, a) is then locally indistinguishable from rest in a gravitational field -a).
- Promoting this to all (non-gravitational) physics gives the Einstein Equivalence Principle, and demanding it hold over extended regions forces spacetime to be curved.
Limiting cases
What if…
Different materials would fall at different rates; a torsion balance would twist, and general relativity's geometric picture would collapse.
Tidal effects appear — two coins released apart drift together (curvature). Equivalence is only local.
The dropped-coin elevator
- In the inertial frame the coin coasts at constant velocity once released.
- The floor accelerates up at 9.8 m/s^2 toward the coin.
- Relative to the elevator the coin 'falls' at 9.8 m/s^2.