Acceleration
Acceleration changes the phase accumulated between atomic paths. This is why atom interferometers are studied as quantum accelerometers.
Metrology 101 explains optical interferometry. Metrology 201 steps into atomic interferometry: matter waves, laser-pulse beam splitters, cold atoms, inertial phase, and the hard control problem hiding under the miracle. It also introduces Information-Stationary Locking (ISL) — the generalization of PQS's noise-stationary control from optical systems to the entire quantum-sensor landscape.
In optical interferometry, the “wave” is light. In atomic interferometry, the “wave” is the quantum wavefunction of an atom. Laser pulses play the role of beam splitters and mirrors, separating and redirecting matter-wave paths before recombination. The measured output is often a population or fringe signal rather than a simple optical intensity fringe.
Acceleration changes the phase accumulated between atomic paths. This is why atom interferometers are studied as quantum accelerometers.
Rotation changes the relative phase geometry, making atom interferometers relevant to gyroscopes and inertial navigation.
Gravity acts like acceleration. Falling atoms can therefore serve as exquisitely sensitive test masses for gravimetry and geodesy.
The exact architecture varies, but the bones are usually recognizable. A practical atom-interferometric sensor must prepare atoms, interrogate them with phase-coherent laser pulses, detect the final state, and keep the machine disciplined enough that the measured phase is not swallowed by technical noise.
PQS is not trying to turn atom interferometry into a slogan. The serious connection is control. Atomic interferometers depend on coherent phase relationships, fringe contrast, stable readout, and rejection of platform disturbance. That is the same kind of “keep the measurement useful under non-ideal conditions” problem that motivates Noise-Stationary Locking — and that motivation led to Information-Stationary Locking (ISL).
In optical NSL, the objective function normalizes band-limited noise against detected optical power:
ISL replaces optical power with a measurement-information functional — any physically appropriate proxy for how much useful information the sensor is actually extracting. The universal ISL objective becomes:
The lock condition is the same: drive the derivative to zero. But the denominator I(θ) can now be fringe contrast, atom number times contrast squared, classical Fisher information, quantum Fisher information, or signal-response gain — whatever is physically appropriate for the sensor at hand.
This is provably not equivalent to contrast maximization. When technical noise has an asymmetric component, the ISL stationary point diverges from the contrast peak — ISL selects the point of minimal first-order noise leverage, not the visually “prettiest” fringe.
ISL is designed as a layered control system. It does not replace the fast loop that every atom interferometer already runs — it sits on top of it and slowly adjusts the operating conditions.
The fast, conventional atom-interferometer control loop. It holds the phase near the target operating point (typically mid-fringe). ISL does not replace this loop.
The novel contribution. It estimates band-limited noise, computes the measurement-strength denominator, forms the ISL objective, applies a small dither, extracts the gradient, and slowly trims the control parameter to stationarize the normalized noise.
Prevents the optimizer from driving into a low-noise but low-accuracy or invalid state. Enforces minimum contrast, minimum atom number, and maximum parameter deviation. Confidence-weighted updates ensure ISL freezes gracefully when measurement quality degrades.
ISL does not grab the steering wheel. It adjusts the alignment of the steering column. The fast loop keeps the interferometer running; ISL slowly tunes the conditions under which it runs, finding the operating point where the sensor is most robust to whatever the environment is throwing at it.
ISL is not just an algorithm extension — it is a directional expansion for PQS. By generalizing from optical power to measurement-information functionals, ISL opens a path to the entire quantum-sensor landscape.
The three-loop ISL architecture can be implemented as firmware or DSP changes on existing atom-interferometer hardware — no new optics, no new vacuum system, no new laser. This lowers the barrier to adoption dramatically compared to optical bench builds.
Beyond optical interferometers, ISL now addresses fieldable gravimeters, inertial navigation sensors (ship, aircraft, drone), long-baseline gravitational-wave detectors, atomic clocks, and quantum-enhanced sensors using squeezed or entangled ensembles.
| Topic | Laser optical interferometer | Atomic interferometer |
|---|---|---|
| Wave | Electromagnetic field. | Matter-wave phase of atoms. |
| Beam splitter | Glass/fiber/integrated optical beamsplitter. | Laser pulse sequence, often Raman or Bragg based. |
| Readout | Photodiode, balanced detector, homodyne, heterodyne. | Population or state readout, often via fluorescence/absorption. |
| Main control burden | Phase, path length, optical power, vibration, coupling, detector noise. | Laser phase/timing, vibration, wavefronts, atom number, contrast, magnetic/environmental drift. |
| PQS relevance | Direct NSL and dark-mode injection embodiments. | ISL: measurement-information-normalized noise objective, three-loop architecture, software-only deployment on existing hardware. |
Each row represents a sensor type where ISL's measurement-information-normalized noise objective has a natural embodiment.
| Application | Description | ISL control variable |
|---|---|---|
| Atom gravimeters | Chirp rate or phase servo to stationarize normalized noise against atom-number-weighted contrast. | Chirp rate, Raman phase |
| Ship / aircraft / drone INS | Same metric under dynamic vibration spectra — the environment ISL was designed for. | Chirp rate, Raman phase |
| Long-baseline GW detectors | Stationarity of differential phase noise normalized by differential Fisher information. | Multiple (per link) |
| Atomic clocks (Ramsey) | Servo on stability metric normalized by quality factor, contrast, and atom number. | Raman detuning, pulse timing |
| Quantum-enhanced sensors | Denominator becomes quantum Fisher information for spin-squeezed or entangled ensembles. | Ensemble preparation parameters |
This page shows that PQS understands the deeper sensing landscape: optical interferometry is the entry point, but atomic interferometry and ISL are the long game — a hardware-agnostic control architecture that travels with the physics.
ISL positions PQS as a control-architecture company, not a single-bench-build company. The claims are sober, the validation path is clear, and the software-only deployment model lowers the barrier to partnership.
Start with Metrology 101 for the optical interferometry foundation. Return to the home page for the technology overview, IP status, and applications. Or contact Peterson Quantum Sensing for a non-confidential technical discussion about ISL, atom interferometry, or partnership opportunities.
This page describes Information-Stationary Locking as a control architecture concept with natural applicability to atom interferometry. It is not a claim that ISL has already been validated in cold-atom hardware. The signal is phase, the useful information is statistical, and environmental disturbance can dominate real instruments. Validation for atom-interferometric embodiments still has to come from a lab — ideally in partnership with a group that operates the relevant hardware.