The standard quantum limit is the fundamental lower bound on measurement precision imposed by quantum noise in sensors and detectors.In the 1970s, Vladimir Braginsky, analyzing the limits of measurement precision in macroscopic quantum systems, introduced the concept of the standard quantum limit. It stems from the Heisenberg uncertainty principle, but applies to continuous measurements. If you illuminate a mirror with a laser to track its position, quantum fluctuations in the photon number create radiation pressure that randomly displaces the mirror. The total coordinate error has a minimum, known as the SQL. Interestingly, this limit can be circumvented using quantum non-demolition measurements and squeezed states of light.
Vladimir Braginsky in 1967 first pointed out the quantum sensitivity limit in gravitational wave antennas. Further development of the SQL theory is associated with the work of Carlton Caves, who formalized the concept of the standard quantum limit in the 1980s. Experimental surpassing of the SQL was achieved at LIGO in collaboration with Caroline McKenzie and others, where using squeezed states of light improved sensitivity by 3 dB. Key contributions to understanding and overcoming the SQL were also made by Yu. I. Vorontsov and Kip Thorne.
SQL limits the precision of interferometric measurements, such as gravitational wave detectors, atomic force microscopes, and optical traps. For free masses, the limit depends on the measurement time: Δx SQL ~ √(ħτ/m). For a harmonic oscillator, there is a resonant regime where the SQL is reached when measuring amplitude. Overcoming the SQL is possible using quantum non-demolition measurements (measuring only one quadrature without disturbing the other) or squeezed states. Modern LIGO interferometers already operate below the SQL for certain frequency bands.
LIGO and Virgo gravitational wave detectors constantly hit this limit, requiring sophisticated quantum tricks to overcome it and detect tiny fluctuations of space-time.
LIGO gravitational wave observatories already operate in a regime where sensitivity is limited by quantum effects rather than classical noise.
| \Delta \theta | variable | Uncertainty in the estimated parameter — parameter uncertainty |
| N | variable | Number of independent probes or particles — particle number |
| \ge | operator | Indicates a lower bound — greater than or equal |
| LOD | variable | limit of detection — limit of detection mole per cubic metre |
| k | variable | confidence factor (typically 3) — confidence factor |
| σ_noise | variable | standard deviation of the blank signal — noise standard deviation |
| sensitivity | variable | slope of calibration curve (signal per concentration) — sensitivity cubic metre per mole |















