In short
- Three quantum properties do the work: superposition, entanglement and coherence let quantum sensors respond to tiny fields and keep their phase long enough to measure them precisely.
- They beat classical noise limits. Entangled particles push precision from the standard quantum limit (1/√N) towards the Heisenberg limit (1/N), and squeezed light or atoms cut quantum noise below the classical floor.
- The applications are already real: NV-diamond magnetometry, atomic clocks for navigation and timing, atom-interferometer gravimeters, defence sensing, and quantum imaging and lidar.
- Try the numbers. The calculator below shows how atom number, interrogation time and squeezing set the sensitivity of a quantum gravimeter.

Introduction
This article is part of our series on the First and Second Quantum Revolutions and how they shape modern technology. Quantum technologies have moved from theory into real applications, and quantum sensing stands out as one of the most transformative of them.
The advantage of quantum sensing comes from three quantum-mechanical properties: superposition, entanglement and quantum coherence. Together they enable a precision and sensitivity that classical sensors cannot reach. Below we explain the principles that give quantum sensors their edge over classical ones, and then walk through the applications where that edge already matters.
The science behind quantum sensing
Superposition and quantum coherence: the path to precision
Superposition lets a quantum system exist in several states at once. Because of it, a quantum sensor can interact with an external field, such as a magnetic or gravitational field, in ways a classical system cannot: the field shifts the relative phase between the superposed states, and that phase can be read out with great precision.
Quantum coherence is the system’s ability to keep this phase relationship over time. It is the basis of stable, precise measurement and matters most in atomic clocks. The coherence time T₂ tells how long the quantum state stays undisturbed, and it largely sets a sensor’s stability: the longer the phase can accumulate, the smaller the change that can be detected.
An atomic clock locks to the frequency of the transition between two energy levels of an atom:
ν = (E₂ − E₁) / h
where E₂ and E₁ are the energy levels and h is Planck’s constant. Because the transition frequency is fixed by nature, every atom of the same species ticks at the same rate; the SI second itself is defined by the caesium-133 hyperfine transition at 9,192,631,770 Hz. This level of precision underpins GPS and high-resolution spectroscopy.
Entanglement: the quantum advantage
Entangled particles share correlated quantum states: the result of a measurement on one is correlated with the result on the other, regardless of the distance between them. Sensors can use this correlation to go beyond the classical limits on measurement resolution.
With N independent (unentangled) atoms, the phase uncertainty of an atomic interferometer falls only as 1/√N, the standard quantum limit. Entangling the atoms allows the measurement to beat this limit and approach Heisenberg-limited precision:
Δθ = 1 / N
where Δθ is the measurement uncertainty and N is the number of entangled particles. For a million atoms, that is a thousand-fold improvement over the standard quantum limit. Classical techniques cannot reach this level, because noise and environmental interference limit them. In practice, entangled states are fragile, so real sensors operate between the two limits.
Quantum noise reduction: beating classical limits
Classical sensors are limited by thermal noise and shot noise. Quantum sensors can use squeezed states of light or atoms, which reduce the uncertainty in the measured quantity below the classical limit (at the cost of more uncertainty in a quantity that is not measured). Squeezed-light interferometry is already used in the LIGO gravitational-wave detectors to improve their sensitivity.
The noise reduction follows the squeezing relation:
ΔX = e−r ΔX₀
where ΔX is the reduced quantum noise, r is the squeezing parameter and ΔX₀ is the original (vacuum or shot-noise) uncertainty. Squeezing is usually quoted in decibels: 20·log₁₀(er) ≈ 8.69·r dB, so 10 dB of squeezing (r ≈ 1.15) reduces the noise amplitude by a factor of about 3.2. This is what makes it possible to detect extremely small ripples in spacetime. Squeezed light is generated in nonlinear crystals, the same physics described in our article on nonlinear optics and its quantum impact.
Key advantages of quantum sensing
Detects extremely weak signals: tiny magnetic fields, small gravitational changes and even single-photon interactions.
Quantum-enhanced interferometry reaches a precision that classical methods cannot.
Less affected by thermal fluctuations and environmental disturbance, so measurements stay stable.
Extracts information without disturbing the system, which matters for biomedical imaging and remote sensing.
Real-world applications of quantum sensing
Magnetometry and biomedical imaging
Quantum magnetometers based on nitrogen-vacancy (NV) centres in diamond detect extremely weak magnetic fields at the nanoscale. Applications include non-invasive mapping of brain activity (quantum-enabled magnetoencephalography, MEG) and early disease detection. Our article on NV centers and Zeeman splitting explains how these sensors work.
Quantum clocks for navigation and timing
Atomic clocks based on quantum transitions are essential for GPS, secure communications and the synchronisation of financial transactions. Their accuracy also makes precise positioning possible in GPS-denied environments, where a vehicle must navigate on its own clock and inertial sensors.
Gravitational and geophysical sensing
Quantum gravimeters use atom interferometry to measure small variations in Earth’s gravitational field. A cloud of cold atoms is split, reflected and recombined by laser pulses, and the gravitational acceleration appears as a phase shift:
Δφ = keff g T²
where keff is the effective wavevector of the laser pulses (about 4π/λ for counter-propagating two-photon transitions), g is the gravitational acceleration and T is the interrogation time between pulses. Because the phase grows with T², a longer free fall gives a much larger signal. Uses include underground exploration, earthquake prediction and planetary science.
Defense and security
Quantum sensors can detect submarines, underground bunkers and stealth aircraft by sensing tiny gravitational and magnetic anomalies. Because this kind of sensing is passive, the sensor emits no signal that could reveal its own position, unlike active radar or sonar.
Quantum imaging and spectroscopy
Quantum-enhanced imaging enables ultra-sensitive spectroscopy for environmental monitoring and materials science. Quantum-enhanced lidar improves imaging in low-light or obscured conditions, where correlated photon pairs help separate the true return signal from background light. See understanding photon entanglement for how such correlations are measured.
Quantum gravimeter sensitivity calculator
See the three precision limits of this article at work in an atom-interferometer gravimeter. Enter the laser wavelength, the interrogation time T, the number of atoms per shot, the fringe contrast, the squeezing and the cycle time. The tool returns the gravity phase and the smallest change in g you can resolve at the standard quantum limit, with squeezing and at the Heisenberg limit.
keff = 4π/λ; phase noise per shot δφ = 1/(C√N) at the standard quantum limit, e−r/(C√N) with squeezing (r = SdB·ln10/20) and 1/(C·N) at the Heisenberg limit; δg = δφ/(keffT²); sensitivity = δg·√(cycle time). 1 µGal = 10−8 m/s². These are ideal atom-noise limits: real instruments are usually limited by vibration, laser phase noise and systematic effects.
Conclusion
Quantum sensing is a fundamental advance in measurement science. By using superposition, entanglement and quantum noise reduction, quantum sensors reach a precision and sensitivity once considered impossible, with applications across healthcare, defence, navigation, space exploration and more.
The author leads the Advanced Quantum Lab course at the Technion, and at IZAK Scientific we are working to bring these advances into real-world systems: stable optics and nonlinear-crystal alignment, deterministic timing electronics and complete electro-optical set-ups. Future articles in this series go deeper into specific quantum sensors, starting with NV centers and Zeeman splitting.
When this article was first published, IZAK Scientific was preparing to exhibit at OASIS 2025. The invitation still stands: if you work on quantum sensing or related technologies, we would be glad to talk.
IZAK products for this application
Instruments from our catalog that match the measurements and set-ups in this article.
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References
- Taylor, M. A., & Bowen, W. P. (2016). Quantum metrology and its application in biology. Physics Reports, 615, 1–59.
- Pezzè, L., Smerzi, A., Oberthaler, M. K., Schmied, R., & Treutlein, P. (2018). Quantum metrology with nonclassical states of atomic ensembles. Reviews of Modern Physics, 90(3), 035005.
- Giovannetti, V., Lloyd, S., & Maccone, L. (2011). Advances in quantum metrology. Nature Photonics, 5(4), 222–229.
- Kitching, J., Knappe, S., & Donley, E. A. (2011). Atomic sensors – a review. IEEE Sensors Journal, 11(9), 1749–1758.
Frequently asked questions
QWhat makes quantum sensors better than classical sensors?
QWhat is the difference between the standard quantum limit and the Heisenberg limit?
QWhere is quantum sensing used today?
Tzachi Sabati
CEO, IZAK Scientific
Physicist specializing in photonics and quantum technologies, with deep expertise in quantum sensors and advanced optical systems. Leads the Advanced Quantum Lab course at the Technion, bridging academic excellence with industry innovation. At IZAK Scientific, provides cutting-edge photonics-based solutions, developing customized inspection and sensing systems for R&D and production. Passionate about advancing quantum sensing applications and integrating novel technologies to meet industry needs.
Tzachi Sabati