Overview

In physics, coherence refers to the degree to which oscillating quantities—most often electromagnetic waves—maintain a predictable phase relationship and correlation in time and space. When two wave sources share a constant phase difference, identical frequency and the same waveform, they are said to be perfectly coherent; this ideal situation produces stationary interference patterns. Practical sources are usually only partially coherent, but the concept of coherence remains central to understanding interference, diffraction and many measurement techniques. For more advanced treatments see advanced coherence theory.

Key characteristics

Several distinct but related aspects of coherence are commonly considered:

  • Temporal coherence — how well a wave maintains a fixed phase relationship over time. It is related to the source bandwidth and determines the length of path difference over which stable interference occurs.
  • Spatial coherence — how uniform the phase is across different points of a wavefront; it controls visibility of interference across separated apertures.
  • Degree of coherence — a normalized measure of correlation between fields at two points; mathematically expressed by correlation functions and spectra.
  • Perfect vs partial coherence — perfect coherence is an idealization rarely reached in practice; most physical light lies between perfect coherence and complete incoherence.

Physical description and measures

Coherence can be characterized by correlation functions such as the mutual coherence function and the complex degree of coherence. These quantify how closely related two samples of a field are in phase and amplitude. The idea depends on phase stability (phase difference), frequency content (frequency) and waveform shape (waveform). Idealized descriptions treat coherence as stationary in time and space, an assumption that simplifies the analysis but does not hold for every real source. Coherence is a property of waves in general, whether classical waves or quantum probability amplitudes.

History and theoretical development

Interference experiments such as Young’s double-slit and Michelson interferometer exposed the practical importance of phase relations long before a formal theory was developed. In the 20th century, optical coherence theory matured to link statistical descriptions of light with observable interference. The concept was later generalized in quantum optics and quantum mechanics, where coherence describes superposition between states and is quantified by off-diagonal elements of a density matrix. For historical and mathematical context see foundational discussions.

Applications and examples

Coherence underlies many technologies and measurements. Examples include:

  • Interferometry for precision distance and surface measurements, including astronomy and metrology.
  • Lasers, which are highly temporally and spatially coherent compared with thermal sources, enabling tight focusing and long-range interference.
  • Holography and coherent imaging methods that rely on stable phase relationships to reconstruct wavefronts.
  • Spectroscopy and telecommunications, where coherence bandwidth and coherence time limit resolution and data-carrying capacity.

Distinctions and notable facts

Coherence is not the same as monochromaticity, polarization, or intensity. A source can be monochromatic but spatially incoherent, or polarized but temporally incoherent. In quantum contexts, loss of coherence—decoherence—explains how quantum superpositions become classical mixtures through interactions with environments; this is central to quantum computing and foundational studies. Practical analysis often treats coherence statistically via correlation functions that quantify how predictable a field is across space and time (correlation measures).