method

quantum spectroscopy

Spectroscopy techniques exploiting quantum effects to study atomic and material properties.
4 formulas

Description

Quantum spectroscopy refers to techniques that exploit quantum mechanical properties of light or matter—such as entanglement, squeezing, or discrete energy levels—to probe the structure and dynamics of atoms, molecules, and materials with sensitivities or resolutions beyond classical limits. It encompasses methods like entangled-photon spectroscopy, where correlated photon pairs reveal information about a sample that would be obscured by classical noise, and quantum-enhanced Raman or absorption spectroscopy, which use non-classical light to beat the shot-noise limit.

How it works

In classical spectroscopy, light interacts with a sample, and the transmitted or scattered light reveals absorption or emission features. Quantum spectroscopy often uses non-classical light states: for example, entangled photon pairs can be used in 'induced coherence' setups where one photon probes the sample and the other carries the information, suppressing background noise. Alternatively, squeezed light reduces intensity fluctuations below the quantum limit, improving signal-to-noise in absorption measurements. The technique relies on precise control of quantum states and detection, often involving single-photon detectors and coincidence counting.

In practice

Quantum spectroscopy is being developed for ultra-sensitive trace-gas detection, biological imaging with low light levels to avoid photodamage, and characterizing quantum materials and devices.

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Formulas

$$\frac{dN}{dE} \propto E^{-\alpha} \exp(-E/E_{\mathrm{cut}})$$
Particle energy spectrum with power law and exponential cutoff.
What is in the formula
dN/dEvariableDifferential number of particles per energy interval — particle spectrum joule per joule
EvariableParticle energy — energy joule
alphavariableSpectral index of the power law
E_cutvariableCutoff energy — energy joule
\frac{dn}{de}\proptoe^{-α}\exp(-e/e_{{cut}}) · 2606.06974v1
$$P \propto N^2$$
Power scales with the square of number of atoms.
What is in the formula
PvariablePower — power watt
NvariableNumber of atoms — particle number
p\propton^2 · 2510.12017
$$\text{Var}(X_n) \sim f(d_s)$$
Variance scaling with spectral dimension.
What is in the formula
X_nvariablerandom variable indexed by n — random variable
d_svariablespectral dimension — spectral dimension
Varoperatorstatistical variance of a random variable — variance
~operatorasymptotically proportional to (up to a constant factor) — asymptotic equivalence
foperatorsome function of the spectral dimension — function
{var}(x_n)\sim\begin{cases}{var}(x_\infty)>0,&d_s<2\(\logn)^{-2},&d_s=2\n^{-(d_s-2)},&2<d_s<3\(\logn)/n,&d_s=3\1/n,&d_s>3\end{cases} · 2607.04252
$$n_s - 1 = -2\epsilon - \eta, \quad r = 16\epsilon$$
Relate slow-roll parameters to observable CMB power spectra.
What is in the formula
n_svariableScalar spectral index — scalar spectral index
\epsilonvariableFirst slow-roll parameter — slow roll parameter
\etavariableSecond slow-roll parameter — slow roll parameter second
rvariableTensor-to-scalar ratio — tensor to scalar ratio
n_s-1=-2ε-\eta,\quadr=12ε · 2607.06582

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