
Measurement noise is unwanted random fluctuations that obscure the signal in an experiment.Measurement noise is the unwanted random fluctuation that obscures the true signal in any experimental measurement. In physics, every measurement is subject to noise, whether from thermal jitter, quantum fluctuations, or imperfections in the measuring apparatus. The titles in the corpus—'Гигантский шум в сэндвиче из сверхпроводника и магнита' (Giant noise in a sandwich of superconductor and magnet), 'Почему лазерный сенсор дрожит даже в идеале' (Why a laser sensor trembles even in the ideal case)—illustrate how noise appears in diverse systems, from solid-state devices to optical sensors. Understanding and mitigating noise is central to experimental physics, as it sets the limit on how precisely we can measure anything.
The systematic study of noise began in the early 20th century. Johnson and Nyquist characterized thermal noise in 1928, and Schottky described shot noise in 1918. The concept of quantum noise was formalized in the 1960s with the development of quantum optics.
Noise arises from multiple sources. Thermal noise (Johnson-Nyquist) is due to the random motion of charge carriers in a conductor, and its power is proportional to temperature. Shot noise comes from the discrete nature of charge carriers or photons arriving at a detector. Quantum noise, such as vacuum fluctuations, is intrinsic to the electromagnetic field. In a measurement, these fluctuations add to the signal, and the signal-to-noise ratio (SNR) determines how well the true value can be extracted. Techniques like lock-in amplification, averaging, and cryogenic cooling are used to reduce noise, but some noise, like quantum noise, is irreducible.
Noise analysis is used in materials science to detect defects, in gravitational wave detectors (like LIGO) to separate signals from seismic and thermal noise, and in all precision measurements to quantify uncertainty.
In gravitational wave detectors, the noise floor is so low that the mirrors are affected by the quantum vacuum fluctuations of light—a phenomenon called quantum radiation pressure noise, which sets a fundamental limit on their sensitivity.



