
Light exhibiting non-classical statistical properties, such as photon bunching.Quantum light refers to light whose statistical properties cannot be described by classical electromagnetic theory. In classical physics, light is a wave whose intensity can vary continuously, and its photon statistics follow a Poisson distribution for coherent sources like lasers. Quantum light, however, exhibits non-classical features such as photon bunching (where photons arrive in clusters more often than random) or anti-bunching (where photons arrive more evenly spaced). These behaviors arise from the quantum nature of the electromagnetic field, where photons are discrete particles that can be correlated or entangled.
The concept of photon bunching was first predicted by Roy Glauber in 1963, who developed the quantum theory of optical coherence. Hanbury Brown and Twiss had earlier observed intensity correlations in 1956, which were later understood as a classical effect, but Glauber's formalism distinguished classical from quantum light.
The quantum state of light is described by a density matrix or a wavefunction in Fock space, where each mode has a definite photon number. Photon bunching occurs in thermal light, where photons tend to arrive together due to Bose-Einstein statistics. Anti-bunching, seen in single-photon sources, results from the fact that a two-level atom can emit only one photon at a time. These statistics are measured via second-order correlation functions, which compare the probability of detecting two photons simultaneously versus at different times.
Quantum light is essential for quantum cryptography, quantum computing, and quantum metrology, where non-classical correlations enable secure communication and precision measurements beyond classical limits.
A single-photon source emits light that exhibits anti-bunching, meaning the probability of detecting two photons at exactly the same time is zero, a behavior impossible for any classical light source.


