
A setup of mirrors that traps light, allowing it to bounce and amplify signals.An optical cavity is an arrangement of mirrors that traps light, making it bounce back and forth between reflective surfaces. This confinement dramatically increases the interaction time between light and matter, which is crucial for building lasers, enhancing weak signals, and studying quantum effects. In a cavity, light can build up to high intensities even with modest input power, and the resonant frequencies of the cavity act like a filter, selecting specific wavelengths while suppressing others.
The concept of an optical cavity dates back to the early 20th century with the Fabry–Pérot interferometer, invented in 1897 by Charles Fabry and Alfred Pérot. The idea became central to laser physics after the first working laser was demonstrated in 1960 by Theodore Maiman, who used a simple two-mirror cavity.
Light enters the cavity through a partially reflective mirror and then reflects between two or more mirrors, creating standing waves at certain resonant frequencies. The cavity's geometry—mirror spacing and curvature—determines which modes of light are stable and can persist. When atoms or other quantum systems are placed inside the cavity, their interaction with the trapped light is greatly enhanced because each photon passes through the medium many times. This principle underlies cavity quantum electrodynamics, where single atoms can strongly couple to single photons.
Optical cavities are the heart of every laser, from laser pointers to industrial cutting tools, and are also used in gravitational wave detectors like LIGO, where they amplify the tiny displacement caused by passing gravitational waves.
In the LIGO gravitational wave detector, the optical cavities are about 4 kilometers long, and the mirrors are so sensitive that they can detect a change in length smaller than one-thousandth the diameter of a proton.



















