Doc QP / QO-LECTURES Page Reading Section Level first principles → project Contents 6 primers · 13 lectures Issued Oct 2026

Quantum optics, from the photon to stored light

Six primers and thirteen lectures that build the ideas behind the Zeeman EIT guide, one step at a time: history and motivation, the maths and quantum mechanics you need, the physics of EIT and stored light, and the bench itself. Each has learning goals, a worked example with real ⁸⁷Rb/795 nm numbers, an analogy beside every equation (including where it breaks down), questions with hidden answers, extra “Go deeper” material, interactive 3D illustrations, hover help on every symbol, and a bibliography whose entries were checked against their publisher records.

Prerequisites
first-year physics; the maths and quantum mechanics are rebuilt in P3–P5
Path
P0–P5 start here · L1–L4 foundations · L5–L9 atoms & light · L10–L12 memories & beyond · L13 the bench
Interactive
11 three.js illustrations · symbol hover help · photon counter (L1) · Rabi/Bloch (L3) · EIT window (L7)
Conventions
Rabi-frequency factors of 2 vary between books; we say which we use
Tags
paper Steck estimate
P0

Start here: how to use these notes

Learning goals
  • Choose a route through the notes that fits your background.
  • Use the 3D illustrations and the hover-help on symbols.
  • Check that the prerequisites are in place before L1.

These notes exist for one reason: so that anyone in the group can read the Zeeman EIT guide and understand why every part of the bench is there and what the numbers in it mean. They start from first-year physics and climb, step by step, to the collective light–matter physics behind the project. They do not replace a textbook. Every section ends with real sources (all references in the bibliography were checked against their publisher records, and where a statement comes from a particular paper or data sheet it says so).

The notes have three layers. Primers P1–P5 give the history, the motivation, and the mathematics, quantum mechanics and quantum optics you need. Lectures L1–L12 build the physics of the experiment, from the photon to stored light and strong coupling. Lecture L13 turns to the bench itself: polarization, Gaussian beams, acousto-optic modulators, laser locking, cells and shielding, detectors and laser safety.

Pick a route

If you…Read in this order
know first-year physics onlyP1 → P2 → P3 → P4 → P5 → L1 → L2 → … → L13, working the questions as you go
know basic quantum mechanics (Griffiths level)skim P3 and P4, read P5, then L1 → L12 and L13
know quantum optics alreadyP2 (motivation), L5, L7–L10 (the project physics), L13 (the bench)
are building the bench nowL13 first, then L1, L3, L5–L9; keep the 3D bench simulator open beside it

Tools in the page

3D illustrations

Eleven interactive three.js scenes sit next to the equations they illustrate. Drag to rotate, scroll to zoom, and use the sliders: the physics in the scene is the same equation as in the text.

Hover help for symbols

Hover, focus (Tab) or tap any underlined symbol in the text, any symbol inside an equation, or any chip under an equation, to see its name, meaning and units. The full list is in Appendix A.

Analogies, with limits

Each key equation has an analogy box that says in words what it means and where the analogy breaks down. The limit is as important as the picture.

Worked examples and questions

Worked examples use real ⁸⁷Rb numbers. Questions have hidden answers: try before you open them. “Go deeper” boxes carry extra derivations, pitfalls and further reading.

Conventions used throughout

TopicConvention here
UnitsSI, with practical units (nm, MHz, mW/cm², G, mG) where the lab uses them. Magnetic fields in gauss: 1 G = 10⁻⁴ T.
Frequency vs angular frequencyν in Hz; ω = 2πν in rad/s. A linewidth “in MHz” is almost always Γ/2π, so the rate in s⁻¹ is 2π times larger.
Rabi frequencyΩ is defined so the coupling term in the Hamiltonian is ħΩ/2 (so Ω is the on-resonance oscillation rate). The EIT tutorial of Finkelstein et al. defines its Ω with coupling ħΩ, which differs by a factor 2: compare formulas only after checking the convention. For example, their Autler–Townes doublet is E± = ±ħΩc where ours is ±ħΩc/2.
DetuningΔ = ωlaser − ωatom. The two-photon (Raman) detuning is δ.
Circular polarizationσ⁺ carries +ħ of angular momentum along the quantization axis (the magnetic field direction in the experiment). Handedness depends on the direction of travel relative to that axis, so it flips when a beam is reflected.
Optical depthOD is natural-log based: transmission = e−OD. A neutral-density filter “OD 2” is base 10 (transmission 10⁻²). The conversion is OD(e) = 2.303 × OD(10), and one natural OD is 4.34 dB.
Data tagspaper from the EIT tutorial; Steck from D. A. Steck’s ⁸⁷Rb data sheet (revision 2.3.4, August 2025); estimate a rough number for orientation only.

Self-check before you start

Q1. What is eiπ + 1?
Zero. By Euler’s formula eiπ = cos π + i sin π = −1. Complex exponentials are the language of phases (P3).
Q2. What is the frequency of 795 nm light?
ν = c/λ = (2.998 × 10⁸ m/s)/(795 × 10⁻⁹ m) ≈ 3.77 × 10¹⁴ Hz = 377 THz.
Q3. What are the eigenvalues of the matrix [[0, 1], [1, 0]]?
+1 and −1, with eigenvectors (1, 1)/√2 and (1, −1)/√2. This matrix is the Pauli matrix σx (P4); its eigenvectors are the equal superpositions of two states.
Q4. For the state (|g⟩ + i|e⟩)/√2, what is the probability of finding |g⟩?
½: the probability is the squared magnitude of the amplitude, |1/√2|² = ½. The factor i changes only the relative phase.
Q5. What are 1 mW and 1 µW in dBm?
dBm = 10 log₁₀(P/1 mW). So 1 mW = 0 dBm and 1 µW = −30 dBm.

If any of these felt unfamiliar, start with P3 and P4. If all were easy, skim P3–P4 and begin at P5 or L1.

P1

A short history: from light quanta to stored light

Learning goals
  • Place the main ideas (quantum, photon, coherence, laser, EIT, memory) in order.
  • See that EIT and light storage are built from much older tools (magnetic resonance, optical pumping, the laser).
  • Know which papers are the original sources.

The physics in this project did not arrive in one step. It is the meeting of three older lines: quantization of light and matter (1900–1930), coherent control of two-level systems by oscillating fields (1937 onward, first with spins, then with lasers), and the laser itself (1960). Electromagnetically induced transparency was observed in 1991, and the step to slow, stopped and stored light followed within a decade. The timeline lists the landmark papers; every entry links to its source in the bibliography.

  1. 1900Planck proposes that energy is exchanged in discrete amounts to explain the spectrum of thermal radiation (Planck 1901).
  2. 1905Einstein proposes that light itself comes in quanta, using the photoelectric effect as the test (Einstein 1905).
  3. 1913Bohr’s atom: discrete energy levels, spectral lines from jumps between them (Bohr 1913).
  4. 1917Einstein introduces the coefficients A and B for spontaneous emission, absorption and stimulated emission (Einstein 1917). Stimulated emission is the process behind the laser, and the same coefficients set the natural linewidth.
  5. 1922Stern and Gerlach show that the direction of an atom’s magnetic moment is quantized (Gerlach & Stern 1922): the origin of the mF sublevels of L5.
  6. 1923Compton scattering of X-rays supports the idea that a light quantum carries momentum (Compton 1923).
  7. 1925–26Matrix mechanics (Heisenberg 1925), wave mechanics (Schrödinger 1926) and the probability interpretation of the wavefunction (Born 1926) give quantum mechanics its modern form (P4).
  8. 1927Dirac quantizes the electromagnetic field and derives spontaneous emission from first principles (Dirac 1927); this is the root of P5.
  9. 1937Rabi analyses a spin in a gyrating (rotating) magnetic field (Rabi 1937): the Rabi oscillation of L3. The matching equations for nuclear magnetic resonance follow in 1946 (Bloch 1946).
  10. 1954–60The maser (Gordon et al. 1954), the proposal to extend it to light (Schawlow & Townes 1958), and the first laser (MAIMAN 1960). Narrow, intense, tunable light opens atomic coherence to experiments.
  11. 1956Hanbury Brown and Twiss measure correlations between photons in two beams (BROWN & TWISS 1956): the technique behind g(2)(0) of L11.
  12. 1957Feynman, Vernon and Hellwarth show that any two-level problem can be pictured as a vector precessing on a sphere (Feynman et al. 1957): the Bloch-sphere picture of L2–L4.
  13. 1963Glauber’s quantum theory of optical coherence (Glauber 1963; Glauber 1963) defines coherent states and photon correlations (Nobel Prize 2005, Nobel 2005). Jaynes and Cummings compare quantum and semiclassical descriptions of an atom in a field (Jaynes & Cummings 1963).
  14. 1972Happer’s review of optical pumping (HAPPER 1972) collects the methods for preparing atoms in chosen sublevels.
  15. 1976Alzetta and colleagues observe coherent population trapping, a dark resonance in sodium vapour driven by two laser frequencies (Alzetta et al. 1976). It is the same dark state as in L7.
  16. 1977Kimble, Dagenais and Mandel observe photon antibunching in resonance fluorescence (Kimble et al. 1977): the first observation of this signature of non-classical light.
  17. 1991Boller, Imamoğlu and Harris report the observation of electromagnetically induced transparency (Boller et al. 1991); Harris’s article in Physics Today (Harris 1997) is a short, readable overview.
  18. 1995Bose–Einstein condensation of dilute atomic gases (Anderson et al. 1995; Davis et al. 1995) gives the ultracold, long-lived samples used in the first slow-light experiments.
  19. 1999Light speed reduced to 17 metres per second in an ultracold atomic gas (Hau et al. 1999). In the same year slow light was reported in hot or warm atomic vapours (Kash et al. 1999; Budker et al. 1999), the regime of this project.
  20. 2000–01The dark-state polariton picture (Fleischhauer & Lukin 2000; the quantum-memory version in Fleischhauer & Lukin 2002); halted light pulses and coherent storage of optical information (Liu et al. 2001); storage of light in atomic vapour (Phillips et al. 2001); and the proposal to use atomic ensembles for long-distance quantum communication (Duan et al. 2001).
  21. 2001–10EIT carries over to other systems: ultraslow and stored light in a solid (Turukhin et al. 2001); stopped light with storage times of over a second in a solid (Longdell et al. 2005); EIT on a single artificial atom (Abdumalikov et al. 2010); optomechanical analogues (Weis et al. 2010; Safavi-Naeini et al. 2011).
  22. 2005The standard review of EIT (Fleischhauer et al. 2005), and storage and retrieval of single-photon pulses in atomic ensembles (Chanelière et al. 2005; Eisaman et al. 2005).
  23. 2008–09The vision of a quantum internet (Kimble 2008) and the review of optical quantum memory (Lvovsky et al. 2009).
  24. 2012Nobel Prize in Physics to Haroche and Wineland for methods of measuring and manipulating individual quantum systems (Nobel 2012; Nobel lectures Haroche 2013, Wineland 2013).
  25. 2018–23A highly efficient EIT-based optical memory (Hsiao et al. 2018) and the practical guide to EIT in atomic vapour (Finkelstein et al. 2023) that Zeeman EIT follows.
  26. 2022Nobel Prize in Physics to Aspect, Clauser and Zeilinger for experiments with entangled photons and the pioneering of quantum information science (Nobel 2022).
What the history teaches
  • The equations are old; the experiments are new. The Bloch and Rabi equations come from magnetic resonance in the 1930s–40s. The laser let them be applied to optical transitions, where EIT appears.
  • EIT is the optical cousin of a dark resonance seen in 1976. What changed in 1991 and after is the viewpoint: use the dark resonance to control light (slow it, store it) rather than to study the atom.
  • Memory is the application that kept the field alive. From 2000, “store a quantum state of light” (dark-state polaritons, DLCZ) turned an optical curiosity into a building block for quantum networks (P2).
  • Many platforms, one idea. The same transparency window appears in vapours, crystals, superconducting circuits and mechanical resonators; the project’s later stage asks whether it can be made to work in a solid-state material (L12).

Further reading: the history is told with technical detail in Scully & Zubairy 1997 and Loudon; Harris’s overview Harris 1997 and the review Fleischhauer et al. 2005 cover the EIT part.

P2

Why this project: quantum memories and quantum networks

Learning goals
  • Explain why quantum information needs both light and matter.
  • Explain why long-distance links need quantum memories.
  • State what Objectives 1, 2 and 3 of the project are, and why the order matters.

Light is the natural carrier of quantum information: photons travel fast, interact weakly with their surroundings and can be sent through fibre or free space. Quantum key distribution (the 1984 proposal of Bennett and Brassard, reprinted in Bennett & Brassard 2014), quantum communication in general (Gisin & Thew 2007) and the proposals for a quantum internet (Kimble 2008) all rely on photons as “flying qubits”. But weak interaction is also the problem: photons are hard to hold, to delay or to make interact. Matter is the natural place to store and process information. Atoms, ions, spins in crystals and superconducting circuits keep a state for a useful time and can be controlled precisely, but are poor at travelling. A quantum memory is the interface: it takes in a photon’s quantum state, holds it, and gives it back on demand (Lvovsky et al. 2009; Hammerer et al. 2010).

Why can the photon not simply be amplified and sent on? Because an unknown quantum state cannot be copied (the no-cloning theorem). The only way to cover a long distance is to split it into segments, create entanglement across each segment, and join the segments. The segments succeed at random times, so each must be held until its neighbours also succeed. That holding device is a quantum memory, and the scheme is the quantum repeater (Briegel et al. 1998; Sangouard et al. 2011). The DLCZ proposal showed how atomic ensembles and linear optics could do this (Duan et al. 2001).

P2.1\[ T_{\rm fibre}=10^{-\alpha_{\rm dB}L/10},\qquad \alpha_{\rm dB}\sim0.2\ \mathrm{dB/km}\ \ (\text{typical telecom fibre near 1550 nm})\ \Rightarrow\ T(1000\ \mathrm{km})\sim10^{-20}. \]

What a good memory needs

Figure of meritMeaningWhy it matters for a repeater
Efficiency ηprobability that a stored photon comes backloss in each memory multiplies along the chain
Fidelity ℱhow closely the returned state matches the inputerrors accumulate with every step
Storage timehow long the state survives before η fallsmust exceed the time to learn that the neighbour succeeded (light travel time plus processing)
Bandwidththe spectral width of pulses it can storemust match the photon source and the repetition rate
Multimode capacitynumber of distinguishable pulses held at onceraises the rate of the whole link

These are defined carefully in Heshami et al. 2016 and Bussières et al. 2013; L10 returns to them with numbers.

Why atoms in a warm vapour

EIT-based memories store light as a collective ground-state coherence of many atoms (Fleischhauer & Lukin 2000; Phillips et al. 2001). A warm vapour needs no laser cooling or vacuum chamber, only a cell, a heater and magnetic shielding, which makes it the simplest platform on which to learn the physics (Novikova et al. 2011; Finkelstein et al. 2023). Its price is motion: atoms fly through the beam at hundreds of metres per second, which L9 deals with. The same idea has been demonstrated in cold atoms, in rare-earth-doped crystals and in other media; L10 gives a short survey with sources. EIT-type effects are also used outside memories, for example in coherent-population-trapping clocks (Vanier 2005) and in optical magnetometry (Budker & Romalis 2007).

The project in three objectives

Objective 1: a locked laser and an operating cell

Build a calibrated optical platform: a 795 nm laser locked to a rubidium reference and a heated, magnetically shielded ⁸⁷Rb cell. This is the foundation for everything else.

Objective 2: EIT and light storage

Observe the transparency window (Zeeman EIT with two acousto-optic modulators) and then store and retrieve light pulses, measuring efficiency, delay, bandwidth and storage time with classical (attenuated) light.

Objective 3: a solid-state test (next stage)

The wider programme aims to test room-temperature solid-state materials (P3HT microcavities, α-MoO₃ single-photon emitters) as quantum-memory candidates. This is outside the present guide; L12 explains the physics context without claiming results.

Why calibrate firstAn unproven material cannot be tested on an uncalibrated bench. If storage failed, you would not know whether the material or the optics was at fault. Rubidium vapour is a well-understood reference: its linewidths, optical depths and storage curves are documented (Finkelstein et al. 2023), so every habit learned here (alignment, polarization purity, field control, measuring OD and linewidth) carries over to the next stage.
Q1. A fibre link is 200 km long with 0.2 dB/km loss. What fraction of photons arrives?
Loss = 0.2 × 200 = 40 dB, so T = 10−4 = 0.01 %. Only one photon in ten thousand survives, which is why a repeater chain is attractive.
Q2. Why can an amplifier not rescue a quantum signal?
A noiseless copy of an unknown quantum state is forbidden (no-cloning), and any ordinary amplifier adds noise. A memory-based repeater avoids amplification: it re-creates entanglement over short segments instead.
Q3. Why does a memory with high efficiency but a short storage time not help a long link?
The memory must hold the state until the neighbouring segment also succeeds. If storage time is shorter than that waiting time, the state is lost before it is used.

Where it shows up: project framingquantum memory metrics (L10)Objective 3 context (L12)

P3

Maths toolkit: complex numbers, matrices, Dirac notation, Fourier

Learning goals
  • Handle complex amplitudes and phases with Euler’s formula.
  • Read and write states and operators in Dirac notation.
  • Use eigenvalues, the matrix exponential and the Fourier relation between time and frequency.
  • Convert comfortably between eV, Hz, nm, dBm and OD.

Quantum optics uses a small set of mathematical ideas over and over. This primer collects them, with the lab numbers they will be applied to. If you studied linear algebra and complex numbers recently, skim; otherwise work the exercises at the end of each part.

P3.1 Complex numbers and phases

Every oscillation in the notes is written with a complex exponential. A complex number z = a + ib has a magnitude |z| and a phase φ, and Euler’s formula links the two descriptions. Multiplying by eiφ rotates z by φ in the complex plane without changing its length: this is what a phase shift is. Quantum amplitudes are complex numbers; probabilities are their squared magnitudes, so a common phase never matters but a relative phase does (L2).

P3.1\[ z=a+ib=|z|\,e^{i\varphi},\qquad e^{i\varphi}=\cos\varphi+i\sin\varphi,\qquad |z|^2=zz^*=a^2+b^2,\qquad \cos\varphi=\tfrac12\big(e^{i\varphi}+e^{-i\varphi}\big). \]

P3.2 Vectors, inner products and basis states

A quantum state of an n-level system is a vector with n complex components. The inner product of two vectors measures their overlap; two states with zero overlap are orthogonal (perfectly distinguishable). A set of mutually orthogonal, normalised vectors is a basis; any state can be written as a weighted sum of basis vectors, and the weights are the amplitudes. For the two ground states |1⟩ and |2⟩ of the Λ system, or the lower and upper states |g⟩ and |e⟩, the basis is just “which level”.

P3.2\[ \langle u|v\rangle=\sum_j u_j^*v_j,\qquad \langle\psi|\psi\rangle=1,\qquad |\psi\rangle=\sum_j c_j|j\rangle,\qquad c_j=\langle j|\psi\rangle,\qquad \sum_j|c_j|^2=1. \]

P3.3 Matrices, eigenvalues and the matrix exponential

Physical quantities (energy, spin, polarization) are represented by matrices. The special vectors that a matrix only stretches, never rotates, are its eigenvectors, and the stretch factors are the eigenvalues. For the Hermitian matrices of quantum mechanics the eigenvalues are real (they are the possible measurement results) and the eigenvectors are orthogonal. Time evolution under a constant Hamiltonian is a matrix exponential: each energy eigenstate simply acquires a phase.

P3.3\[ \hat H|n\rangle=E_n|n\rangle,\qquad \hat U(t)=e^{-i\hat Ht/\hbar},\qquad \hat U(t)|n\rangle=e^{-iE_nt/\hbar}|n\rangle,\qquad \hat H^\dagger=\hat H\ \Rightarrow\ E_n\ \text{real}. \]
Worked example · the simplest two-level problem

Take two states coupled with strength ħΩ/2 and no detuning, Ĥ = (ħΩ/2)[[0, 1], [1, 0]]. The eigenvalues of [[0, 1], [1, 0]] are ±1 with eigenvectors (|g⟩ ± |e⟩)/√2, so the energies are ±ħΩ/2 and the two states are split by ħΩ. Starting in |g⟩ = (|+⟩ + |−⟩)/√2, the two components acquire phases e∓iΩt/2, and the amplitude to be in |e⟩ is −i sin(Ωt/2). That is a Rabi oscillation: P(e) = sin²(Ωt/2), reaching 1 at t = π/Ω. L3 derives it properly.

P3.4 Dirac notation

Dirac’s bra–ket notation is shorthand for vectors and their conjugate transposes: |ψ⟩ is a column vector (a “ket”), ⟨ψ| the corresponding conjugate row (a “bra”), ⟨φ|ψ⟩ an inner product (a number), and |ψ⟩⟨φ| an outer product (a matrix). The projector |e⟩⟨e| picks out the excited-state part of a state; the sum of projectors over a full basis is the identity (completeness). Operators like the lowering operator σ̂ = |g⟩⟨e| are written as outer products, which makes their action obvious: take the part in |e⟩ and put it in |g⟩.

P3.4\[ \hat P_e=|e\rangle\langle e|,\qquad \hat\sigma=|g\rangle\langle e|,\qquad \sum_j|j\rangle\langle j|=\hat 1,\qquad \hat\rho=|\psi\rangle\langle\psi|\ \ (\text{pure state}). \]

P3.5 Fourier transform, pulses and line shapes

A signal in time and its spectrum in frequency are two views of the same thing, related by the Fourier transform. A short pulse has a broad spectrum; a long, steady wave has a narrow one. Two results are used constantly: a Gaussian pulse of FWHM duration Δt has FWHM bandwidth Δν = 0.441/Δt, and a field whose amplitude decays as e−Γt/2 has a Lorentzian power spectrum of FWHM Γ (in rad/s), that is Γ/2π in Hz. The second is the natural line shape of an atom (L4); the first limits how fast a pulse can be before it no longer fits inside the EIT window (L8).

P3.5\[ \tilde E(\omega)=\int E(t)\,e^{i\omega t}\,dt,\qquad \Delta\nu\,\Delta t=\frac{2\ln2}{\pi}\approx0.441\ \ (\text{Gaussian}),\qquad \mathcal L(\Delta)=\frac{(\Gamma/2)^2}{\Delta^2+(\Gamma/2)^2}\ \ (\text{FWHM}=\Gamma). \]

P3.6 Differential equations you will meet

Two equations cover most of what follows. Exponential decay, dx/dt = −γx, gives x = x₀e−γt: populations and coherences decay this way. Harmonic oscillation, d²x/dt² = −ω²x, gives cos(ωt) and sin(ωt): a driven two-level atom oscillates between its states in just this way, as do the electromagnetic field and the polariton. A rotating frame is a change of variables that removes a fast oscillation (such as the 377 THz optical carrier) so that only slow changes remain: this is the idea behind the rotating-wave approximation (L3).

P3.7 Units and orders of magnitude

QuantityValue or conversionUse
Photon energy vs wavelengthE[eV] = 1239.84 / λ[nm]; at 794.979 nm, E = 1.5596 eVphoton counting (L1)
Energy vs frequency1 eV ↔ 241.80 THz; 1 THz ↔ 4.1357 meV; 1 GHz ↔ 4.1357 µeVcomparing optical and hyperfine scales
Thermal energykBT at 333 K (60 °C) = 28.7 meV = 6.9 THz × hwhy a hot vapour is thermal but still far below the optical photon energy
Rb D1 lineλ = 794.979 nm; ν = 377.107 THz; Γ/2π = 5.750 MHz (Steck)everything
⁸⁷Rb ground hyperfine splitting6.834 683 GHz (Steck)Λ-system energy scale (L5)
Zeeman scaleµB/h = 1.3996 MHz/G, so gF = ½ gives 0.70 MHz/G per mFshielding requirement (L5, L13)
Power in dBmdBm = 10 log₁₀(P / 1 mW): 1 mW = 0 dBm, 1 µW = −30 dBm, +3 dB = ×2RF chain, photodiode signals (L13)
Optical depthOD(e) = 2.303 × OD(10); 1 OD(e) = 4.34 dB; transmission = e−ODcell, filters (L6, L13)
Intensity1 mW/cm² = 10 W/m²control and probe intensities (L1, L3)
Q1. Show that multiplying z = 1 by eiπ/2 gives i. What does that do to the arrow?
eiπ/2 = cos 90° + i sin 90° = i, so 1 × i = i: the arrow of length 1 along the real axis is turned by 90° to point along the imaginary axis. Phases add when amplitudes multiply.
Q2. A two-level state has amplitudes (cos θ, sin θ). Are the two basis states’ amplitudes properly normalised?
Yes: cos²θ + sin²θ = 1. This is why a two-level state can be written with a single angle (the Bloch sphere of L2).
Q3. A pulse has a Gaussian envelope of FWHM 5 µs. What is its minimum FWHM bandwidth?
Δν = 0.441/Δt = 0.441/(5 × 10⁻⁶ s) ≈ 88 kHz.
Q4. Convert 3.77 × 10¹⁴ Hz to an energy in eV.
E = hν = 4.1357 × 10⁻¹⁵ eV·s × 3.77 × 10¹⁴ Hz ≈ 1.56 eV.

Further reading: Griffiths & Schroeter (chapters on linear algebra and Dirac notation) and Feynman et al. for the first principles; Sakurai & Napolitano for a more advanced treatment.

P4

Basic quantum mechanics for atoms and photons

Learning goals
  • State the postulates of quantum mechanics in plain words.
  • Use the Schrödinger equation, operators, commutators and the uncertainty relation.
  • Describe spin-½, angular momentum and the quantum numbers of an atom.
  • Understand the harmonic oscillator, which is the basis of light quantization.

Quantum mechanics rests on a few rules (Griffiths & Schroeter; Sakurai & Napolitano; Feynman et al.). State: a system is described by a normalised vector |ψ⟩ in a complex vector space. Observables: each measurable quantity (energy, position, spin component) is a Hermitian operator; its eigenvalues are the possible results. Measurement: the probability of result a is |⟨a|ψ⟩|² (the Born rule, Born 1926), and afterwards the system is in the state |a⟩. Evolution: between measurements the state evolves smoothly under the Schrödinger equation (Schrödinger 1926). Combining systems: the state space of two systems is the tensor product of their spaces, which allows entanglement.

P4.1\[ i\hbar\frac{d}{dt}|\psi\rangle=\hat H|\psi\rangle,\qquad \hat H|n\rangle=E_n|n\rangle\ \Rightarrow\ |\psi(t)\rangle=\sum_nc_n\,e^{-iE_nt/\hbar}|n\rangle,\qquad P(a)=|\langle a|\psi\rangle|^2. \]

P4.1 Operators, commutators and uncertainty

Operators do not always commute: the order in which you apply them matters. The commutator [Â, B̂] = ÂB̂ − B̂Â measures how much. Position and momentum have the fundamental commutator [x̂, p̂] = iħ, which leads to the uncertainty relation: no state has both a sharply defined position and a sharply defined momentum (Griffiths & Schroeter). For atoms the more useful consequence is a Fourier relation between lifetime and linewidth: a level that lives for a time τ has a spectral width of order 1/(2πτ) (L4).

P4.2\[ [\hat x,\hat p]=i\hbar,\qquad \Delta x\,\Delta p\ge\frac{\hbar}{2},\qquad [\hat J_x,\hat J_y]=i\hbar\hat J_z\ \text{(and cyclic)},\qquad \Delta\nu=\frac{1}{2\pi\tau}\ \ (\text{natural linewidth}). \]

P4.2 Spin-½, angular momentum and the Bloch sphere

Angular momentum is quantized: the length of an angular momentum J has the value √(J(J+1))ħ and its projection on any axis takes only the 2J+1 values mħ, with m from −J to +J (Gerlach & Stern 1922). A spin-½ (an electron, a proton, or an effective two-level system) has just two projections, ±ħ/2, and is described by the Pauli matrices. Every pure state of a two-level system is a point on a sphere, the Bloch sphere (L2; Feynman et al. 1957). Rubidium’s valence electron has spin ½ and its nucleus has spin 3/2, and the sublevels of the experiment are the projections of the total angular momentum F (L5).

P4.3\[ \hat\sigma_x=\begin{pmatrix}0&1\\1&0\end{pmatrix},\quad \hat\sigma_y=\begin{pmatrix}0&-i\\i&0\end{pmatrix},\quad \hat\sigma_z=\begin{pmatrix}1&0\\0&-1\end{pmatrix},\qquad \hat S_k=\frac{\hbar}{2}\hat\sigma_k,\qquad |\vec J|=\hbar\sqrt{J(J+1)},\ \ J_z=m\hbar. \]

P4.3 The harmonic oscillator

The quantum harmonic oscillator is the most important model system in quantum optics because each mode of the electromagnetic field is one (Dirac 1927). Its energies are equally spaced, En = ħω(n + ½), with a zero-point energy ħω/2. Two operators, the lowering and raising (annihilation and creation) operators â and â†, move between levels. In the field picture they remove and add a photon of energy ħω, which is why the next primer can quantize light with the same algebra.

P4.4\[ \hat H=\hbar\omega\Big(\hat a^\dagger\hat a+\tfrac12\Big),\qquad [\hat a,\hat a^\dagger]=1,\qquad \hat a|n\rangle=\sqrt n\,|n-1\rangle,\qquad \hat a^\dagger|n\rangle=\sqrt{n+1}\,|n+1\rangle,\qquad E_n=\hbar\omega\big(n+\tfrac12\big). \]

P4.4 Atoms: quantum numbers, energy levels and selection rules

In a hydrogen-like atom the energy depends mainly on the principal quantum number n (En ≈ −13.6 eV/n²). The electron’s orbital angular momentum l and spin ½ combine to J (fine structure), and J combines with the nuclear spin I to F (hyperfine structure). Alkali atoms such as rubidium have one valence electron outside closed shells, so they behave much like hydrogen with adjusted energies (Foot 2005). Light couples states through the electric-dipole interaction, which obeys selection rules: the orbital quantum number changes by one (Δl = ±1), and the magnetic quantum number changes by 0 or ±1 depending on the light’s polarization (L5). That is why the D lines of rubidium (5S → 5P) are strong and why σ⁺ and σ⁻ light connect different sublevels.

P4.5\[ E_n\simeq-\frac{13.6\ \mathrm{eV}}{n^2},\qquad \Delta l=\pm1,\qquad \Delta m=0,\pm1,\qquad \Gamma_{i\to f}=\frac{2\pi}{\hbar}\,|\langle f|\hat V|i\rangle|^2\,\rho(E_f)\ \ (\text{Fermi's golden rule}). \]
Worked example · scales in ⁸⁷Rb

The 5S₁/₂ → 5P₁/₂ gap is 1.5596 eV (Steck). The hyperfine splitting of the ground state, 6.8347 GHz, is only 28 µeV: about 55 000 times smaller. The Zeeman splitting per gauss, 1.4 MHz × 0.5 for F = 2, is smaller again by ~10⁴. These three widely separated energy scales (optical, hyperfine, Zeeman) are why each part of the experiment can be treated separately: the laser addresses the first, the Λ system lives in the second and third, and the shield protects the third.

Q1. A spin-1 object has how many projections, and which?
2J + 1 = 3, namely m = −1, 0, +1 (in units of ħ).
Q2. Why can a photon not take an atom from S to D in a single electric-dipole step?
The dipole selection rule requires Δl = ±1, but S to D is Δl = 2. Such transitions are only possible through weaker (quadrupole) processes.
Q3. What is the zero-point energy of a mode of frequency 377 THz, and why can it not be removed?
ħω/2 = ½ × 1.5596 eV ≈ 0.78 eV (here ħω is the photon energy). It is a consequence of [â, â†] = 1: the lowest state still has non-zero energy, because position and momentum cannot both be zero. It sets the vacuum fluctuations that cause spontaneous emission (P5).

Where it shows up: L2 states and measurementL5 atomic structureP5 quantized light

P5

Basic quantum optics: photons, coherent states and emission

Learning goals
  • Describe a mode of light as a quantum harmonic oscillator and define number and coherent states.
  • Explain absorption, stimulated emission and spontaneous emission with Einstein’s coefficients.
  • Compute a decay rate from a dipole matrix element.
  • Compare natural, Doppler and pressure line widths.

The semiclassical picture, in which atoms are quantum but light is a classical wave, explains most of what follows (Rabi flopping, EIT, slow light). But three effects need the quantum light field: spontaneous emission, photon counting statistics, and the quantum state of a stored pulse (L8, L10, L11). The route is short: treat each mode of the electromagnetic field as a harmonic oscillator (P4.3) whose quanta are photons (Dirac 1927; Loudon; Gerry & Knight; Fox 2006).

P5.1\[ \hat H_{\rm field}=\hbar\omega\Big(\hat a^\dagger\hat a+\tfrac12\Big),\qquad \hat E(t)=\mathcal E_0\big(\hat a\,e^{-i\omega t}+\hat a^\dagger e^{i\omega t}\big),\qquad \mathcal E_0=\sqrt{\frac{\hbar\omega}{2\epsilon_0V}},\qquad \hat n=\hat a^\dagger\hat a. \]

P5.1 Number states and coherent states

A number (Fock) state |n⟩ has exactly n photons and a completely undefined phase. A coherent state |α⟩ is the quantum version of an ideal classical wave: it is the eigenstate of the lowering operator, â|α⟩ = α|α⟩, with a mean photon number |α|² and a Poisson photon-number distribution (Glauber 1963). A well-stabilised laser emits light very close to a coherent state, which is why attenuating it never produces a single-photon source (L11). The price of a well-defined phase is an uncertain photon number: for a coherent state ΔN = √N̄ and the phase uncertainty is about 1/(2√N̄).

P5.2\[ \hat a|\alpha\rangle=\alpha|\alpha\rangle,\qquad \bar n=|\alpha|^2,\qquad P(n)=e^{-|\alpha|^2}\frac{|\alpha|^{2n}}{n!},\qquad \Delta N=\sqrt{\bar n},\qquad \Delta\varphi\approx\frac{1}{2\sqrt{\bar n}}. \]
Worked example · a µW beam is nowhere near a single photon

1 µW at 795 nm is 4.0 × 10¹² photons/s (L1). In a 10 µs pulse the mean number is n̄ = 4.0 × 10⁷, so the shot-noise uncertainty is √n̄ ≈ 6 300 photons (0.016 %). The phase uncertainty 1/(2√n̄) ≈ 8 × 10⁻⁵ rad. Such a pulse is classical for every practical purpose. To make it quantum, attenuate until n̄ ≈ 1; at that point the Poisson spread is as large as the mean (L11).

P5.2 Absorption, stimulated and spontaneous emission

Einstein (Einstein 1917) described the exchange of energy between atoms and radiation with three processes. An atom in the lower level can absorb a photon (rate ∝ B₁₂ times the radiation density). An atom in the upper level can be stimulated to emit a photon identical to the incoming one (rate ∝ B₂₁ times the same density), and can also decay on its own by spontaneous emission at rate A₂₁. Consistency with thermal radiation fixes the ratios between the coefficients. Spontaneous emission is not an extra assumption in quantum optics: it can be understood as emission stimulated by the vacuum fluctuations of P5.1.

P5.3\[ \frac{dN_2}{dt}=-A_{21}N_2-B_{21}\rho(\nu)N_2+B_{12}\rho(\nu)N_1,\qquad g_1B_{12}=g_2B_{21},\qquad \frac{A_{21}}{B_{21}}=\frac{8\pi h\nu^3}{c^3},\qquad \Gamma=A_{21}=\frac1\tau. \]
P5.4\[ \Gamma=\frac{\omega_0^3\,|d|^2}{3\pi\epsilon_0\hbar c^3}\ \ \Big(\text{two-level atom; for D1 with }J=J'=\tfrac12\ \text{the statistical factor is }1\Big). \]
Worked example · from a dipole moment to the Rb D1 lifetime

Steck gives the reduced dipole matrix element of the D1 line as ⟨J = ½‖er‖J′ = ½⟩ = 2.5377 × 10⁻²⁹ C·m and ω₀ = 2π × 377.107 THz = 2.369 × 10¹⁵ rad/s Steck. Then ω₀³ = 1.330 × 10⁴⁶, |d|² = 6.440 × 10⁻⁵⁸, and the denominator 3πε₀ħc³ = 2.372 × 10⁻¹⁹, so Γ = (1.330 × 10⁴⁶ × 6.440 × 10⁻⁵⁸)/(2.372 × 10⁻¹⁹) = 3.61 × 10⁷ s⁻¹. That agrees with the tabulated 36.129 × 10⁶ s⁻¹ (lifetime 27.679 ns, Γ/2π = 5.750 MHz). The whole natural linewidth of the atom is fixed by one matrix element and one frequency.

P5.3 Line shapes: natural, Doppler and pressure

MechanismShapeFWHM for ⁸⁷Rb D1 at 60 °CWhere covered
Natural (spontaneous emission)LorentzianΓ/2π = 5.750 MHz SteckL4
Doppler (thermal motion)Gaussian(1/λ)√(8 ln 2 · kBT/m) ≈ 529 MHz derived (σ/2π ≈ 225 MHz, Fig. 6 of the paper uses 230 MHz)L9
Pressure (buffer-gas collisions)Lorentzian≈ 10 MHz per Torr, so ~100 MHz at 10 Torr paperL9
Transit time (atoms crossing the beam)≈ Lorentzian~1/(2π × time in beam): tens of kHz for a beam of about 1 mm without buffer gas (L9)L9

The combination of a Lorentzian and a Gaussian is a Voigt profile. Two numbers explain why EIT is such a clever trick in a warm vapour: the Doppler width (~500 MHz) is about a hundred times the natural width (5.75 MHz), yet EIT opens a window only tens of kHz wide inside it, because the two lasers see the same Doppler shift and the two-photon transition is almost free of it (L9).

Q1. A coherent state has n̄ = 100. What is the relative photon-number uncertainty?
ΔN/N̄ = √100/100 = 10 %. For n̄ = 10⁴ it is 1 %. The relative noise falls as 1/√n̄.
Q2. If a transition’s dipole moment doubles (same frequency), what happens to its lifetime?
Γ ∝ |d|², so Γ rises by 4 and the lifetime falls by a factor of 4.
Q3. Why does the Doppler width not simply wash out EIT?
For a Λ system with nearly co-propagating beams, an atom moving with velocity v sees both frequencies shifted almost equally, so the difference (the two-photon detuning) hardly changes. EIT is a two-photon effect and so survives the one-photon Doppler broadening (L9).

Further reading: Gerry & Knight and Fox 2006 for an accessible route; Loudon for the full treatment; Steck, Quantum and Atom Optics for free notes with the two-level atom worked in detail; and Steck, Rb-87 data for all the numbers.

L1

Light as waves and photons

Learning goals
  • Describe light as an electromagnetic wave with wavelength, frequency and wavevector.
  • Explain energy quantization and compute the photon energy at 795 nm.
  • Convert optical power into photon rate, the bridge between “mW” and “single photons”.

Classically, a laser beam is an oscillating electric field. At 795 nm it oscillates about 3.8 × 10¹⁴ times per second, far too fast for any detector to follow, so detectors measure time-averaged power. Quantum mechanically, that energy arrives in indivisible packets, photons, each carrying hν. Both pictures are right. The wave picture explains interference and polarization (the waveplates of Zeeman EIT); the photon picture explains why a detector clicks and why a quantum memory must preserve single quanta.

L1.1\[ E(z,t)=E_0\cos(kz-\omega t),\qquad k=\frac{2\pi}{\lambda},\quad \omega=2\pi\nu,\quad c=\lambda\nu;\qquad E_{\rm photon}=h\nu=\frac{hc}{\lambda},\qquad \Phi=\frac{P}{h\nu}. \]
Worked example · 795 nm

λ = 794.979 nm Steck ⇒ ν = c/λ ≈ 377.107 THz. E = hc/λ = (6.626×10⁻³⁴ J s)(2.998×10⁸ m/s)/(7.950×10⁻⁷ m) ≈ 2.499 × 10⁻¹⁹ J ≈ 1.560 eV.

A 1 µW probe carries 10⁻⁶ / 2.499×10⁻¹⁹ ≈ 4.0 × 10¹² photons/s, and 1 nW carries 4.0 × 10⁹ photons/s. A 10 µs pulse at 1 µW holds ≈ 4 × 10⁷ photons: a long way from one.

Interactive · photon counterE = hc/λ, Φ = P/E
Q1. How many photons per second are in a 1 pW beam at 795 nm?
1×10⁻¹² W / 2.499×10⁻¹⁹ J ≈ 4.0 × 10⁶ photons/s. Even a picowatt is millions of photons per second.
Q2. Why can the photodiode in Zeeman EIT not see individual 795 nm photons?
An ordinary photodiode with a transimpedance amplifier integrates current. Its noise is equivalent to many photons per measurement time, so single quanta are hidden. Counting single photons needs single-photon detectors (e.g. avalanche photodiodes), which are not in the current equipment plan.
Go deeper · photons, momentum, field strength and what “power” hides
Photon momentum and spin

A photon of wavelength λ carries momentum p = h/λ (Compton 1923). When a ⁸⁷Rb atom absorbs a 795 nm photon it recoils at about 5.78 mm/s Steck, which is why a cloud can be laser-cooled but is irrelevant against the ~180 m/s thermal speed of a warm vapour (L9). A photon also carries intrinsic spin angular momentum ±ħ along its direction of travel for circular polarization (σ⁺ or σ⁻), and linear light is an equal superposition of the two. That spin is what transfers angular momentum to an atom and gives the selection rules of L5.

From power to field
L1.2\[ I=\tfrac12\,c\,\epsilon_0E_0^2,\qquad E_0=\sqrt{\frac{2I}{c\,\epsilon_0}},\qquad \Phi=\frac{P}{h\nu}. \]

The paper’s weaker control intensity, 1.3 mW/cm² = 13 W/m², corresponds to E₀ = √(2 × 13/(2.998 × 10⁸ × 8.854 × 10⁻¹²)) ≈ 99 V/m. A power in mW is not an intensity: the same power in a smaller beam is more intense. This is why beam size (L13) matters as much as the power.

Pitfalls
Vacuum or air? The D1 wavelength is 794.979 nm in vacuum and 794.766 nm in air Steck. The 0.2 nm difference is about 100 GHz, far larger than any linewidth: use the vacuum value in calculations and check which one your wavemeter reports.
h versus ħ. E = hν = ħω. Mixing ν and ω gives errors of 2π. Photon energy in eV is 1239.84/λ[nm].
Sources

Einstein 1905 and Compton 1923 for the photon concept; Hecht and Saleh & Teich for waves, intensity and polarization; Steck, Rb-87 data for all the rubidium numbers; Fox 2006 for a gentle quantum-optics start.

Where it shows up: laser safety and power levelspulse energies in storage

L2

Quantum states, superposition and measurement

Learning goals
  • Write states in Dirac notation and normalise them.
  • Distinguish probability amplitudes from probabilities.
  • See why relative phase is physical and evolves in time.

A quantum state is a vector |ψ⟩. For a two-state system with basis {|g⟩, |e⟩}, any state is a superposition with complex amplitudes. Measurement in that basis gives g or e with probabilities |cg|² and |ce|², and leaves the system in the outcome state. The relative phase between cg and ce does not change those probabilities, but it decides how the state interferes later. EIT is built entirely on such a phase (L7).

L2.1\[ |\psi\rangle=c_g|g\rangle+c_e|e\rangle,\qquad |c_g|^2+|c_e|^2=1,\qquad P(e)=|\langle e|\psi\rangle|^2=|c_e|^2,\qquad c_j(t)=c_j(0)\,e^{-iE_jt/\hbar}. \]
Worked example · hyperfine superposition

Prepare (|F=1⟩ + |F=2⟩)/√2 in ⁸⁷Rb. The relative phase advances at νhfs ≈ 6.834 683 GHz: a full turn every 1/νhfs ≈ 146.3 ps. A hyperfine (clock-type) Λ scheme would have to follow that rotation with a microwave field near 6.8 GHz; the Zeeman superposition rotates only at kHz (70 kHz at 50 mG, a 14 µs period).

Q1. Is (|g⟩ + i|e⟩)/√2 different from (|g⟩ + |e⟩)/√2 if you only measure in the {g, e} basis?
No. Both give 50/50. They differ in relative phase (90°), which shows up when the state interferes with something else, e.g. after another light pulse.
Q2. Why does a global phase eiφ|ψ⟩ not matter, while a relative phase does?
All probabilities involve |amplitude|², which is unchanged by a common factor eiφ. A relative phase changes how the amplitudes add when they are projected onto a different basis.
Go deeper · the Bloch sphere, measurement in other bases, and Ramsey interference
Two angles describe everything
L2.2\[ |\psi\rangle=\cos\tfrac\theta2\,|e\rangle+e^{i\varphi}\sin\tfrac\theta2\,|g\rangle,\qquad (u,v,w)=(\sin\theta\cos\varphi,\ \sin\theta\sin\varphi,\ \cos\theta),\qquad P(\hat n)=\tfrac12\big(1+\vec r\cdot\hat n\big). \]

The polar angle θ of the sphere is twice the angle that appears in the state, so orthogonal states (|e⟩ and |g⟩) sit at opposite poles. A measurement along any axis n̂ gives “+” with probability (1 + r⃗·n̂)/2. In the {g, e} basis only the height w = cos θ is visible; the azimuth φ becomes visible only if the state is first rotated, for instance by a laser pulse. Use the 3D illustration above to see this: sliding φ never changes P(e).

Interference of amplitudes: Ramsey’s method

Apply a π/2 pulse (|g⟩ goes to the equator), let the state precess freely for a time T at detuning Δ, then apply a second π/2 pulse. The final excited-state probability is P(e) = ½(1 + cos ΔT) for ideal pulses: it depends on the phase ΔT accumulated between the pulses, not on any population. This is the same relative-phase physics that makes EIT possible, and the origin of the narrowest spectroscopy and atomic clocks.

Superposition, mixture and measurement

A superposition has a definite phase between its parts and interferes; a mixture is a statistical ensemble of states and does not (L4). Whether the change on measurement is a physical collapse or a loss of coherence to the environment is an interpretation question on which textbooks differ (Griffiths & Schroeter; Sakurai & Napolitano); the predictions you will use are the same.

Pitfalls. (1) A superposition (|g⟩ + |e⟩)/√2 is not “half excited atoms and half ground-state atoms”: that would be a mixture. (2) The unknown quantum state cannot be copied, so you cannot “measure it first and keep a copy” (no-cloning; see Nielsen & Chuang 2000).
Sources

The geometrical picture is from Feynman et al. 1957 and Bloch 1946; Nielsen & Chuang 2000 uses it for qubits; Allen & Eberly 1975 applies it to optical resonance.

Where it shows up: dark state

L3

The two-level atom: dipole coupling, RWA, Rabi oscillations, Bloch sphere

Learning goals
  • Write the dipole Hamiltonian and apply the rotating-wave approximation.
  • Predict Rabi oscillations, including the effect of detuning.
  • Picture the state on the Bloch sphere.

An atom with transition frequency ω₀ in a laser field E cos ωt feels the energy −d·E. Moving to a frame rotating at ω and dropping terms oscillating at 2ω (the RWA) leaves a simple 2×2 problem that depends only on the detuning Δ = ω − ω₀ and the Rabi frequency Ω. Here Ω = d·E₀/ħ is the full Rabi frequency, the rate of population cycling on resonance. The EIT paper defines Ω = µẼ/ħ with its own field convention; always check factors of 2 when comparing sources.

L3.1\[ \hat H_{\rm RWA}=-\hbar\Delta\,|e\rangle\langle e|+\frac{\hbar\Omega}{2}\big(|e\rangle\langle g|+|g\rangle\langle e|\big),\qquad P_e(t)=\frac{\Omega^2}{\Omega^2+\Delta^2}\,\sin^2\!\Big(\frac{\sqrt{\Omega^2+\Delta^2}}{2}\,t\Big). \]
L3.2\[ \vec r=(u,v,w),\quad w=\rho_{ee}-\rho_{gg},\qquad \dot{\vec r}=\vec\Omega_{\rm eff}\times\vec r\ \ \text{(no decay)},\qquad \vec\Omega_{\rm eff}=(\Omega,0,-\Delta). \]
Interactive · Rabi oscillation & Bloch sphereoptical Bloch equations, RK4, starts in |g⟩

Equations: u̇ = Δv − (Γ/2)u, v̇ = −Δu + Ωw − (Γ/2)v, ẇ = −Ωv − Γ(w+1). With decay on, oscillations damp toward a steady state: the reason continuous lasers on a two-level atom give absorption rather than endless Rabi cycling.

Worked example · how big is Ω in Zeeman EIT?

A common two-level estimate is Ω = Γ√(I/(2Isat)). With Γ/2π = 5.750 MHz and the D1 far-detuned π-polarized Isat ≈ 4.488 mW/cm² Steck, the paper’s 1.3 mW/cm² control gives Ω/2π ≈ 5.750 × √(1.3/8.975) ≈ 2.2 MHz. The paper quotes Ωc/2π = 1.9 MHz: the same order, with the difference coming from Clebsch–Gordan factors and Rabi-frequency conventions. A π-pulse at Ω/2π = 2 MHz takes π/Ω = 250 ns.

Q1. With Δ = Ω, what is the maximum excited population?
Ω²/(Ω²+Ω²) = 1/2.
Q2. Why is the RWA safe for Rb D1 driven by a mW laser?
The dropped terms oscillate at ≈ 2 × 377 THz, while Ω and Δ are MHz to GHz. Their effect averages out (the Bloch–Siegert shift is of order Ω²/ω, utterly negligible here).
Go deeper · where the RWA comes from, dressed states and π-pulses
Derivation sketch of the rotating-wave approximation

With the field E₀ cos ωt, the coupling term is ħΩ cos(ωt)(|e⟩⟨g| + |g⟩⟨e|). Writing the cosine as ½(eiωt + e−iωt) and moving to a frame rotating at the laser frequency (|e⟩ acquires e−iωt), the coupling splits into two parts: a slowly varying one of size ħΩ/2, and a part that oscillates at 2ω. The fast part averages out. That leaves the time-independent HRWA of L3.1. The leading correction is the Bloch–Siegert shift of order Ω²/4ω₀: for Ω/2π = 2 MHz and ν₀ = 377 THz it is about 3 mHz, utterly negligible.

Dressed states and the Autler–Townes splitting
L3.3\[ E_\pm=\frac{\hbar}{2}\Big(-\Delta\pm\sqrt{\Delta^2+\Omega^2}\Big),\qquad \Omega_{\rm gen}=\sqrt{\Omega^2+\Delta^2},\qquad P_e^{\max}=\frac{\Omega^2}{\Omega^2+\Delta^2},\qquad t_\pi=\frac{\pi}{\Omega}. \]

The eigenstates of HRWA are the “dressed” states of atom plus field. On resonance they are split by exactly ħΩ, and a strong control field splits a level this way: the Autler–Townes doublet of L7. The population oscillates at the difference of the two dressed energies, √(Ω² + Δ²).

Pulses

A π pulse (area Ωt = π) transfers an atom from |g⟩ to |e⟩; a π/2 pulse puts it on the equator, in an equal superposition. With Ω/2π = 2 MHz, tπ = π/Ω = 250 ns. Pulse area, not just power, sets the result: that is the area theorem of coherent optics (Allen & Eberly 1975).

Pitfalls
The factor 2. Some books define Ω with the coupling ħΩ, so their Rabi oscillation runs at 2Ω; the EIT tutorial does this (Finkelstein et al. 2023). Always check the definition before using a formula.
Rabi flopping in a warm vapour. It is hard to see: the Doppler spread gives every atom a different Δ, and spontaneous emission damps it (L4, L9). EIT works with steady-state dark states, not Rabi flopping.
Sources

Rabi 1937 (the original magnetic-resonance problem); Feynman et al. 1957 (the vector picture); Allen & Eberly 1975 (a whole book on exactly this model); Steck, Rb-87 data for Isat and Γ; Steck, Quantum and Atom Optics for a free derivation.

Where it shows up: Rabi frequencies Ωp, Ωccontrol intensity vs width

L4

Open systems: density matrix, decay and dephasing

Learning goals
  • Use the density matrix for mixed states.
  • Distinguish populations from coherences.
  • Read a Lindblad master equation and identify Γ, Γ/2 and pure dephasing.

Real atoms leak energy (spontaneous emission) and lose phase (collisions, fields, motion). A state vector cannot describe a statistical mixture, but a density matrix can. Diagonal elements are populations (how many atoms are where); off-diagonal elements are coherences (how well-defined the relative phase is across the ensemble). EIT and memories live in coherences, so coherence lifetimes are the central figure of merit of the whole project.

L4.1\[ \hat\rho=\begin{pmatrix}\rho_{ee}&\rho_{eg}\\ \rho_{ge}&\rho_{gg}\end{pmatrix},\qquad \dot{\hat\rho}=-\frac{i}{\hbar}[\hat H,\hat\rho]+\Gamma\Big(\hat\sigma\hat\rho\hat\sigma^\dagger-\tfrac12\{\hat\sigma^\dagger\hat\sigma,\hat\rho\}\Big),\qquad \hat\sigma=|g\rangle\langle e|. \]
Worked example · from lifetime to linewidth

τ(5P₁/₂) = 27.679 ns Steck ⇒ Γ = 1/τ = 3.613 × 10⁷ s⁻¹ ⇒ Γ/2π = 5.750 MHz, matching Steck’s quoted natural linewidth. The optical coherence decays at Γ/2 (γ₁₃ ≈ 2π × 2.87 MHz without collisions). With 10 Torr of buffer gas, pressure broadening (~10 MHz/Torr, paper) dominates, at ~100 MHz.

Q1. A state has ρee = ρgg = ½ and ρeg = 0. Is it a superposition?
No. It is a 50/50 statistical mixture with no coherence. A superposition (|g⟩+|e⟩)/√2 would have |ρeg| = ½.
Q2. Why is γ₁₂ (ground coherence) potentially millions of times smaller than γ₁₃?
Ground states do not decay radiatively. γ₁₂ comes only from slow processes (transit, collisions, field gradients), typically kHz or less, while γ₁₃ includes the MHz radiative decay and collisional broadening.
Go deeper · T₁, T₂, saturation and the scattering rate
The optical Bloch equations
L4.2\[ \dot u=\Delta v-\gamma_\perp u,\qquad \dot v=-\Delta u+\Omega w-\gamma_\perp v,\qquad \dot w=-\Omega v-\Gamma(w+1),\qquad \gamma_\perp=\frac\Gamma2+\gamma_{\rm deph}. \]

These are L3.2 plus damping. Population decays at Γ (the time T₁ = 1/Γ) and the coherence at γ⊥ (T₂ = 1/γ⊥), with 1/T₂ = 1/(2T₁) + 1/T₂* where T₂* collects pure dephasing. So T₂ can never exceed 2T₁. In the steady state, set the derivatives to zero:

L4.3\[ w_{\rm ss}=-\frac1{1+s},\qquad s=\frac{2\Omega^2}{\Gamma^2+4\Delta^2}\ \ (\gamma_{\rm deph}=0),\qquad R_{\rm sc}=\frac\Gamma2\,\frac{s}{1+s}. \]

s is the saturation parameter, equal to I/Isat on resonance. At s = 1 the excited-state population reaches ¼ and the scattering rate is Γ/4; for s ≫ 1 the transition saturates at Γ/2 (Steck, Quantum and Atom Optics). Use the 3D decay illustration above: the violet dot is this steady state, and changing Ω moves it toward the centre of the sphere.

Homogeneous and inhomogeneous dephasing

Homogeneous dephasing (collisions, spontaneous emission) is irreversible for each atom. Inhomogeneous dephasing arises because atoms differ (different Doppler shifts or field strengths) and can be partly undone: the spin echo (Hahn 1950) rephases it by reversing the evolution. In a rubidium cell the ground-state coherence is limited by atom–atom and atom–buffer-gas collisions, by atoms leaving the beam, and by magnetic-field gradients (L9, L13).

Pitfalls. (1) “Linewidth in MHz” is Γ/2π, not Γ. (2) Do not confuse coherence time (how long phase survives) with storage time (how long the retrieved efficiency stays useful): the second also depends on the first protocol’s losses. (3) The optical coherence decays at Γ/2 or faster: collisions only add to it.
Sources

Bloch 1946 (the original phenomenological equations); Allen & Eberly 1975 and Scully & Zubairy 1997 (density matrix treatments); Steck, Quantum and Atom Optics (free, careful derivation); Hahn 1950 (spin echoes).

Where it shows up: master equation in the Λ systemdecoherence budget

L5

Atomic structure for alkalis

Learning goals
  • Build fine, hyperfine and Zeeman structure from angular-momentum addition.
  • Apply dipole selection rules for σ⁺, σ⁻ and π light.
  • Locate the Zeeman Λ system of Zeeman EIT in ⁸⁷Rb, and see how a hyperfine Λ system would differ.

Rubidium’s single valence electron has orbital L and spin S = ½, which combine to J (fine structure: 5P₁/₂ vs 5P₃/₂, the D1 vs D2 lines). The nucleus has spin I = 3/2 for ⁸⁷Rb, and J and I combine to F (hyperfine). In a field B each F splits into 2F+1 sublevels mF. Light carries angular momentum: σ⁺ adds +1 to mF, σ⁻ subtracts 1, and π (polarized along B) adds 0.

L5.1\[ |I-J|\le F\le I+J\ \Rightarrow\ F\in\{1,2\}\ (I=\tfrac32,\ J=\tfrac12),\qquad \Delta E_{\rm Z}=g_F\,\mu_B\,m_F\,B,\qquad \Delta F=0,\pm1,\quad \Delta m_F=0\ (\pi),\ \pm1\ (\sigma^\pm). \]
Worked example · counting and shifting

⁸⁷Rb 5S₁/₂ has 3 + 5 = 8 sublevels. With gF ≈ +½ (F=2), the shift is 0.70 MHz/G per mF Steck. Earth’s field (roughly half a gauss) would shift mF=+2 by about 0.7 MHz, enormous compared with a 10 kHz EIT line. That is why the cell sits inside µ-metal. Zeeman EIT uses the mF=+2/0 pair (1.40 kHz/mG); a hyperfine scheme would use F=1/F=2 clock pairs (m=0↔0, quadratic only).

Q1. Why can σ⁺ light on F=2→F′=1 never excite mF=+2?
It would need mF′=+3, which does not exist in F′=1 (maximum +1). mF=+1 is also dark, since F′=1 has no mF′=+2.
Q2. Why is D1 preferred over D2 for clean Λ systems?
5P₁/₂ has only two excited hyperfine levels (F′=1, 2), well resolved compared with 5P₃/₂’s four. That means fewer competing excitation paths and cleaner dark states.
Go deeper · real ⁸⁷Rb numbers, relative strengths, optical pumping and the clock shift
The D lines and the level structure (Steck, revision 2.3.4)
QuantityValue
D1 line, 5S₁/₂ → 5P₁/₂λ = 794.978 851 nm (vacuum); ν = 377.107 463 THz; photon energy 1.559 591 eV
D2 line, 5S₁/₂ → 5P₃/₂λ = 780.241 210 nm (vacuum); ν = 384.230 484 THz
Ground hyperfine splitting (F = 2 to F = 1)6.834 682 610 904 290 GHz
D1 excited hyperfine splitting (F′ = 2 to F′ = 1)814.5(13) MHz
Nuclear spinI = 3/2 (⁸⁷Rb, natural abundance 27.83 %)
gF factors5S₁/₂: +½ (F = 2), −½ (F = 1), i.e. ±0.70 MHz/G; 5P₁/₂: +1/6 (F′ = 2), −1/6 (F′ = 1), i.e. ±0.23 MHz/G
Clock-transition Zeeman shift (mF = 0 ↔ 0)2π × 575.15 Hz/G² (quadratic)
Relative strengths of the D1 hyperfine components

The strength factors SFF′ sum to 1 over F′ for each F. For D1 they are: from F = 2, to F′ = 1 and to F′ = 2, ½ each; from F = 1, to F′ = 1, 1/6, and to F′ = 2, 5/6 Steck. So the F = 2 → F′ = 1 transition used in Zeeman EIT has the same total strength as F = 2 → F′ = 2. Within a transition the sublevel strengths follow Clebsch–Gordan coefficients, which is why different mF couple with different Rabi frequencies.

Optical pumping and the dark ends of the ladder

Circularly polarized light moves population toward one end of the mF ladder because each absorption raises mF and spontaneous emission returns the atom on average to a slightly higher mF (HAPPER 1972). When the end states cannot absorb (as with σ⁺ light on F = 2 → F′ = 1, L5 Q1), the atoms collect there and the cell becomes transparent: optical pumping is itself a form of dark-state physics, and it competes with EIT in a multilevel atom (L7).

When is the Zeeman shift linear?

The linear formula ΔE = gFµBmFB holds while µBB is small compared with the hyperfine splitting: the Breit–Rabi formula gives the full dependence (Steck, Rb-87 data). Here B must be well below the ~5 kG at which 1.4 MHz/G × B reaches 6.8 GHz, so for any shielded cell the linear regime is excellent. The clock transition between mF = 0 states has no linear shift and only the small quadratic one: 575 Hz/G² means 575 Hz at 1 G but just 0.6 mHz at 1 mG.

Pitfalls. (1) The F = 1 level has gF = −½, so its sublevels run the opposite way from F = 2. (2) Selection rules refer to the quantization axis, which is the magnetic-field direction, not the beam direction (they coincide in Zeeman EIT because the solenoid field is along the beams). (3) Hyperfine levels of the excited state are only 814 MHz apart, close to the Doppler width: neighbouring levels contribute at the edges of the line (L9).
Sources

Steck, Rb-87 data (all numbers above); Foot 2005 (angular momentum, fine and hyperfine structure); HAPPER 1972 (optical pumping); Metcalf & van der Straten (practical level-structure diagrams).

Where it shows up: Zeeman EIT level scheme

L6

Light–matter response: susceptibility, absorption, dispersion

Learning goals
  • Relate χ to refractive index and absorption.
  • Use Beer’s law and optical depth.
  • State the Kramers–Kronig link between absorption and dispersion.

Many atoms together respond to light with a polarization P = ε₀χE. The real part of χ slows the phase (refractive index); the imaginary part removes energy (absorption). Beer’s law follows: intensity falls exponentially with distance, and the exponent at resonance is the optical depth.

L6.1\[ \chi=\chi'+i\chi'',\qquad n\simeq1+\tfrac12\chi',\qquad I(L)=I_0\,e^{-\mathrm{OD}},\ \ \mathrm{OD}=\int_0^L n_{\rm at}\,\sigma\,dz,\qquad \chi'(\omega)=\frac{2}{\pi}\,\mathcal P\!\!\int_0^\infty\frac{\omega'\chi''(\omega')}{\omega'^2-\omega^2}\,d\omega'. \]
Lab connection: keeping the laser on the lineThe same absorption physics gives the laser its reference. In saturated absorption spectroscopy a strong pump burns narrow sub-Doppler dips into a reference cell’s absorption. A lock box turns the dip into a dispersive error signal (zero on the line, opposite signs either side, like a derivative of the dip) and feeds a correction back to the laser current. See the SAS → lock box → laser controller → DFB loop.
Worked example · how opaque is the cell?

The paper’s cell had OD ~10 at ~60 °C paper. Without EIT, T = e⁻¹⁰ ≈ 4.5 × 10⁻⁵, so 1 µW in gives 45 pW out. Our vapour-pressure estimate gives n ≈ 3 × 10¹¹ cm⁻³ at 60 °C design estimate, inside the paper’s typical 10¹¹–10¹² cm⁻³.

Q1. OD doubles from 5 to 10. By what factor does resonant transmission change?
e⁻¹⁰/e⁻⁵ = e⁻⁵ ≈ 6.7 × 10⁻³: about 150 times less light.
Q2. Why does a narrow absorption feature imply a strong dispersion feature?
Kramers–Kronig: the refractive-index change scales with the absorption strength divided by its width, so narrower features give steeper index slopes. This is the root of slow light under EIT.
Go deeper · susceptibility, absorption coefficient, group index and the EIT susceptibility
From χ to what you measure
L6.2\[ \alpha_{\rm abs}=\frac{\omega}{c}\,\chi''\ \ (n\approx1),\qquad n_g=n+\omega\frac{dn}{d\omega}\approx1+\frac{\omega}{2}\frac{d\chi'}{d\omega},\qquad \chi(\Delta)\propto\frac{i}{\gamma_{13}-i\Delta}\ \ (\text{two-level, weak probe}). \]

Intensity decays as e−αabsz. The paper writes the optical depth as OD = 2α₀L, where α₀ is the field (amplitude) attenuation coefficient (Finkelstein et al. 2023); either way the intensity transmission is e−OD. The group index ng grows with the slope of the dispersion: a steep dχ′/dΔ means a slow pulse. For a plain Lorentzian absorber the dispersion slope at line centre is negative (anomalous dispersion: n falls as frequency rises, so ng < 1). In an EIT window the slope is steep and positive (normal dispersion), so ng is large. The 3D illustration above shows this reversal directly.

The susceptibility with a control field
L6.3\[ \chi(\Delta)\propto\frac{i\,(\gamma_{12}-i\Delta)}{(\gamma_{13}-i\Delta)(\gamma_{12}-i\Delta)+\Omega_c^2/4},\qquad \Omega_c\to0:\ \ \chi\to\frac{i}{\gamma_{13}-i\Delta}. \]

This is the standard weak-probe, resonant-control result (with the Ω/2 convention of L3). At Δ = 0 and Ω_c ≫ γ₁₂ the numerator is small and the denominator large, so χ′ and χ″ both nearly vanish: the medium is transparent. The residual absorption is set by γ₁₂ (Fleischhauer et al. 2005; Finkelstein et al. 2023).

Doppler broadening in practice

In a warm vapour the one-photon resonance is smeared over ~530 MHz, so the peak absorption per atom is reduced by roughly the ratio of the natural to the Doppler width; optical depths of ~10 are reached by combining a long cell and high density (L9). The EIT calculation in a Doppler-broadened medium replaces γ₁₃ by an effective width (the lab above uses W) (Finkelstein et al. 2023).

Kramers–Kronig, in one sentence

Because the medium cannot respond before the field arrives (causality), the real and imaginary parts of χ are not independent: each is an integral transform of the other. A narrow absorption feature therefore must come with a narrow, steep dispersion feature; and when EIT cuts a narrow hole in absorption, the dispersion there becomes steep, so group velocities drop (Loudon; Boyd).

Pitfalls. (1) OD defined with base 10 (filters) or base e (atoms). (2) The sign of χ′ below and above resonance depends on the convention for Δ; check the figure’s axis labels. (3) Group velocity can be slower than c or faster, even negative, for an absorbing medium: it is not the speed of information.
Sources

Loudon (response functions and Kramers–Kronig); Boyd and Saleh & Teich (susceptibility and dispersion); Fleischhauer et al. 2005 (EIT susceptibility); Finkelstein et al. 2023 (vapour version); Milonni 2005 (slow and fast light).

Where it shows up: susceptibility and ODOD trade-offs

L7

Three-level interference: dark states, CPT, EIT, Autler–Townes

Learning goals
  • Compare Λ, V and ladder schemes.
  • Derive the dark state and the EIT window.
  • Distinguish EIT (interference) from Autler–Townes splitting (level shifting).

Add a second ground state and a second laser. Two excitation routes now lead to the same excited state, and their amplitudes can cancel. The cancelling superposition is the dark state. If the control is strong and the probe weak, the probe sees a narrow transparency window: EIT. With two comparable fields, atoms are trapped in the dark state: CPT. A strong control also splits the excited state into an Autler–Townes doublet (at ±Ωc in the paper’s convention, ±Ωc/2 in ours: see the note in “Go deeper”), which also reduces absorption at line centre, but without interference, so some residual absorption remains (paper refs [29], [30]).

L7.1\[ |D\rangle=\frac{\Omega_p|2\rangle-\Omega_c|1\rangle}{\sqrt{|\Omega_p|^2+|\Omega_c|^2}},\qquad \gamma_{\rm EIT}=\gamma_{12}+\frac{|\Omega_c|^2}{\gamma_{13}},\qquad E_\pm=\pm\hbar\Omega_c\ \ (\text{Autler–Townes, paper Eq. 23, paper's Rabi convention}). \]
Interactive · the EIT windowpaper Eq. 13 with γ₁₃ → W (effective optical width)
transmissionphase (right axis)no control
Worked example · width at the paper’s control power

Ωc/2π = 1.9 MHz, effective optical width W/2π ≈ 300 MHz design estimate, γ₁₂/2π = 1 kHz. Then γEIT/2π ≈ 1 + 1900²/300 000 kHz ≈ 13 kHz (HWHM), i.e. FWHM ≈ 26 kHz. The paper measured 7.3 kHz FWHM at this control intensity, so the crude formula overestimates here by a factor of ~3. That is a reminder to measure, not assume.

Q1. In the dark state with Ωp ≪ Ωc, where is almost all the population?
In |1⟩, the state coupled by the weak probe. Weight of |1⟩ = |Ωc|²/(|Ωc|²+|Ωp|²) ≈ 1. That is exactly why the result is counter-intuitive.
Q2. Halving the control intensity halves which term of γEIT?
The power-broadening term |Ωc|²/γ₁₃ (Ω² ∝ intensity). γ₁₂ is unchanged.
Go deeper · the Autler–Townes convention, telling EIT from AT, and what dark states are used for
Convention check: the size of the Autler–Townes doubletThe EIT tutorial writes the strong-control dressed states as E± = ±ħΩc (its Eq. 23) because it defines the Rabi frequency with coupling ħΩ (Finkelstein et al. 2023). With the convention used in these notes (coupling ħΩ/2, so Ω is the on-resonance oscillation rate) the same doublet is at ±ħΩc/2, and the splitting between the two components is ħΩc (L3.3). The physics is identical; only the definition of Ωc differs by a factor 2. For example, the paper’s Ωc/2π = 1.9 MHz would be 3.8 MHz in the convention of L3. L7.1 above is stated in the paper’s convention; use the other whenever you compare with L3.
How the dark state arises

For probe and control resonant with |1⟩ → |3⟩ and |2⟩ → |3⟩, the interaction Hamiltonian is (ħ/2)(Ωp|3⟩⟨1| + Ωc|3⟩⟨2| + h.c.). Write a general ground-state superposition a|1⟩ + b|2⟩. It couples to |3⟩ with strength proportional to Ωpa + Ωcb. This vanishes for (a, b) ∝ (Ωc, −Ωp): the dark state of L7.1. The orthogonal combination, the bright state, couples with strength √(Ωp² + Ωc²) and decays as usual. Atoms optically pumped into the dark state stay there (coherent population trapping, Alzetta et al. 1976; Arimondo 1996), until the ground-state coherence decays at rate γ₁₂.

EIT or Autler–Townes?

A strong control opens a dip in the probe absorption in both cases, so the dip alone does not tell you which mechanism acts. In the Autler–Townes picture the dip is the gap between two displaced absorption lines; in EIT it is a quantum-interference hole whose width can be much narrower than any of the lines. Anisimov, Dowling and Sanders showed how to distinguish them objectively by comparing how well each model fits the measured spectrum (Anisimov et al. 2011); in a Doppler-broadened vapour the two often coexist (Finkelstein et al. 2023).

What dark states are used for
Pitfalls. (1) The EIT window needs the two fields to be phase-coherent relative to each other (here guaranteed by deriving both from one laser through AOMs). (2) “Transparent” does not mean lossless: the residual absorption is ~γ₁₂/(γ₁₂ + Ω²/γ₁₃). (3) In real ⁸⁷Rb the dark state is one of many sublevels; leakage to other sublevels reduces the contrast below the three-level prediction (L5).
Sources

Boller et al. 1991 (first observation); Harris 1997 (overview); Fleischhauer et al. 2005 (standard review); Arimondo 1996 (CPT review); Anisimov et al. 2011; Finkelstein et al. 2023 (practical).

Where it shows up: Zeeman EIT dark stateEIT linewidth

L8

Slow and stopped light: group velocity, polaritons, storage

Learning goals
  • Compute group velocity and delay from an EIT spectrum.
  • Describe the dark-state polariton and its mixing angle.
  • Explain storage and retrieval as adiabatic transfer between light and spin wave.

The steep dispersion inside the EIT window makes the group index huge, so a pulse crawls through the cell. In the Fleischhauer–Lukin picture (paper ref. [11]) the propagating excitation is a dark-state polariton, a superposition of the probe field and the collective spin coherence. Its mixing angle θ is set by the control. Lower the control adiabatically to zero and θ → 90°: the excitation becomes purely atomic and stops. Raise it again and the light returns.

L8.1\[ v_g=\frac{c}{n_g}\approx c\cos^2\theta,\qquad \hat\Psi=\cos\theta\,\hat{\mathcal E}-\sin\theta\,\sqrt{N}\,\hat\rho_{12},\qquad \tan^2\theta=\frac{g^2N}{\Omega_c^2},\qquad \tau_{\rm delay}=\frac{\mathrm{OD}_{\rm EIT}}{\gamma_{\rm EIT}}. \]
Worked example · slow light in numbers

Take ODEIT ≈ 9.6 and γEIT/2π ≈ 21 kHz (the simulator’s Zeeman EIT reference, illustrative). τ = 9.6/(2π × 21 × 10³ s⁻¹) ≈ 73 µs. In an assumed 7.5 cm cell that is vg ≈ 0.075 m / 73 µs ≈ 1 km/s, about 3 × 10⁵ times slower than c. A 47 µs pulse is 14 km long in vacuum but ≈ 5 cm inside the cell: it fits, so it can be stored.

Q1. What happens to vg if you halve the control intensity (power-broadening-dominated regime)?
γEIT roughly halves, so the delay ODEIT/γEIT roughly doubles and vg roughly halves. Transparency (ODEIT) may also drop, which is the trade-off.
Q2. Why must the control be turned off while the pulse is fully inside the cell?
Only the part of the pulse inside the medium is converted to spin wave. Anything already out (or not yet in) is lost or unstored. That is why the delay must exceed the pulse length (time-bandwidth product ≈ √ODEIT > 1).
Go deeper · group velocity, adiabatic storage and what limits retrieval
Why slow

The group velocity of a pulse is vg = c/ng with ng = n + ω dn/dω (L6.2). Inside the EIT window dn/dω is large and positive, so ng can reach 10⁵–10⁷ or more in a vapour. The 17 m/s of the famous ultracold-gas experiment (Hau et al. 1999), and the metre-per-second to hundreds-of-metres-per-second speeds reported soon after in warm vapours (Kash et al. 1999; Budker et al. 1999), show that the effect does not need ultracold atoms. The pulse is also compressed in space by vg/c as it enters, so a pulse that is kilometres long in vacuum fits inside a cell centimetres long.

Why “stored light” is not “frozen photons”

At θ → 90° the dark-state polariton is entirely atomic: the quantum state of the field has been transferred to the collective coherence ρ₁₂ of all atoms, a spin wave whose phase pattern copies the pulse’s envelope (Fleischhauer & Lukin 2000; Fleischhauer & Lukin 2002). Storing and retrieving light were first demonstrated in a vapour and in an atomic medium by Phillips et al. 2001 and Liu et al. 2001, and the same idea works for single photons (Chanelière et al. 2005; Eisaman et al. 2005).

What makes it adiabatic

The control must change slowly compared with the inverse of the EIT window (the pulse’s spectrum must fit inside the window) so that the state follows the dark state without exciting the bright one. If the control is switched off too fast, part of the pulse is converted to bright-state population and lost to spontaneous emission. Shaping the control to maximize efficiency for a given OD is an optimization problem solved in Gorshkov et al. 2007.

What limits storage and retrieval
  • Optical depth. Inefficiency scales as 1/ODEIT (L10): a bigger OD is the main resource.
  • Bandwidth. A pulse longer than 1/(window width) fits inside the window; one that is too short leaks.
  • Spin-wave decay. The coherence decays at γ₁₂ and the spin-wave pattern is washed out by atoms diffusing across its wavelength. In Zeeman EIT both fields have almost the same wavelength, so the spin wave has a very long period and is almost unaffected by motion along the beam.
  • Control leakage. A mW control next to a nW signal: the Glan–Taylor, spectral and timing filters (L11, L13).
Pitfalls. (1) The delay ODEIT/γEIT is an estimate; measure it. (2) A pulse that is not fully inside when the control turns off is only partly stored. (3) The light is a dark-state polariton, not a photon sitting still, and energy is not created: the control field supplies none of the stored excitation.
Sources

Fleischhauer & Lukin 2000, Fleischhauer & Lukin 2002, Lukin 2003 (the theory); Novikova et al. 2011 (warm-atom experiments, a review); Hau et al. 1999, Phillips et al. 2001, Liu et al. 2001 (the experiments); Milonni 2005; Finkelstein et al. 2023 (practical limits).

Where it shows up: Zeeman EIT slow & stored lightstorage timing

L9

Thermal vapour realities: Doppler, transit, collisions, buffer gas

Learning goals
  • Estimate Doppler width and transit time for warm Rb.
  • Explain why co-propagating Λ beams cancel Doppler broadening.
  • Describe what a buffer gas buys and what it costs.

Atoms in a warm cell move at hundreds of metres per second. Each motional effect is a time-of-flight T across a length l, giving broadening ≈ 1/T (paper Eq. 29). Over an optical wavelength this is Doppler broadening; across the beam it is transit broadening; across the two-photon wavelength it determines whether EIT survives motion.

L9.1\[ v_{\rm th}=\sqrt{\frac{k_BT}{m}},\qquad \sigma_{\rm Dop}=v_{\rm th}k,\qquad \Gamma_{tt}\sim\frac{v_{\rm th}}{w_0}\ \text{(ballistic)},\ \ \frac{D}{w_0^2}\ \text{(diffusive)},\qquad \delta_{\rm Dop}^{(2)}=(\vec k_p-\vec k_c)\cdot\vec v. \]
Worked example · ⁸⁷Rb at 60 °C

m = 86.909 u Steck, T = 333 K ⇒ vth ≈ 179 m/s. σDop/2π = vth/λ ≈ 225 MHz (the paper’s Fig. 6 uses 230 MHz). Ballistic crossing of a 0.75 mm beam radius takes ≈ 4.2 µs. With D ≈ 10 cm²/s (paper, 10 Torr), diffusion across it takes w₀²/D ≈ 0.56 ms, about 130 times longer derived.

Q1. Why does a ladder (cascade) scheme prefer counter-propagating beams, while Λ prefers co-propagating?
In Λ one photon is absorbed and one emitted, so the effective wavevector is kp − kc, which is small when the beams travel together. In a ladder both photons are absorbed, so it is kp + kc, which is minimised by opposite directions (paper Fig. 9 inset).
Q2. A beam angle of 0.1 mrad between probe and control: roughly how much residual broadening without buffer gas?
σDopθ ≈ 225 MHz × 10⁻⁴ ≈ 20 kHz: “tens of kHz”, as the paper says. With buffer gas, Dicke narrowing makes it quadratic in θ and much smaller.
Go deeper · numbers for a warm cell, buffer gas, Dicke narrowing and its costs
The numbers
L9.2\[ f(v)\propto e^{-mv^2/2k_BT},\qquad \Delta\omega=-\vec k\cdot\vec v,\qquad n_{\rm at}=\frac{P_{\rm vap}}{k_BT}. \]

Rubidium’s vapour pressure at 25 °C is 3.92 × 10⁻⁷ Torr Steck, which is 5.2 × 10⁻⁵ Pa: the ideal-gas law gives n = 5.2 × 10⁻⁵/(1.381 × 10⁻²³ × 298) = 1.3 × 10¹⁶ m⁻³ = 1.3 × 10¹⁰ cm⁻³. The density rises roughly exponentially with temperature, so raising the cell from 25 °C to 60 °C raises it by about 20 to 25 times design estimate: the heater is an optical-depth knob. At the higher density atom–atom collisions (spin exchange) start to limit the coherence, which is the trade-off the paper describes (Finkelstein et al. 2023).

What a buffer gas does and costs

A few Torr of an inert gas (here neon) make the active atoms diffuse instead of flying straight, which keeps them in the beam far longer (diffusion D ≈ 10 cm²/s at 10 Torr, paper) and, when the mean free path is shorter than the relevant wavelength, narrows the Doppler contribution (Dicke narrowing, Dicke 1953). For the two-photon coherence the relevant length is the microwave or Zeeman wavelength, which is centimetres or longer, so narrowing is complete; for the one-photon optical transition it is not (Finkelstein et al. 2023). The costs: pressure broadening of the optical line (~10 MHz/Torr, so ~100 MHz at 10 Torr, about 17 times the natural width), a lower peak absorption per atom (so a higher temperature may be needed for the same OD), and collisional dephasing of the ground states that grows with pressure.

Alternatives to a buffer gas

Anti-relaxation wall coatings (paraffin-type coatings) preserve ground-state coherence through wall collisions and allow very long lifetimes in small cells, at the price of a limited temperature range. Slow light in a vapour with slow ground-state relaxation was reported by Budker et al. 1999. Which is better depends on the target: coatings favour long storage in small cells, buffer gas favours simplicity and tolerance of beam size.

Pitfalls. (1) A small angle between probe and control gives residual two-photon Doppler broadening of ~σDopθ without buffer gas: 0.1 mrad is already ~20 kHz. (2) Thermal gradients in the cell make the coldest spot (the stem) set the density. (3) Temperature stability matters as much as accuracy: OD drifts with T.
Sources

Finkelstein et al. 2023 (the best single source); Dicke 1953; HAPPER 1972; Budker et al. 1999; Novikova et al. 2011; Steck, Rb-87 data (vapour-pressure model and data).

Where it shows up: Zeeman EIT hot-vapour effects

L10

Quantum memories: metrics, repeaters, networks

Learning goals
  • Define efficiency, fidelity, storage time, bandwidth and multimode capacity.
  • Explain why repeaters need memories.
  • Place the project’s Rb platform among memory goals.

A quantum memory stores a quantum state of light and releases it on demand. Photon loss in fibre grows exponentially with distance and a quantum state cannot be copied, so long-distance links need repeaters. Repeaters create entanglement over short segments and connect them, and they need memories to hold one segment’s success while the others try. The DLCZ proposal (paper ref. [47]) used atomic ensembles for exactly this. Published Rb and Cs ensemble memories report high efficiencies and fidelities (e.g. Hsiao et al. 2018, paper ref. [114]); read the originals for the numbers.

L10.1\[ \eta=\frac{E_{\rm out}}{E_{\rm in}},\qquad \mathcal F=|\langle\psi_{\rm in}|\psi_{\rm out}\rangle|^2\ \ (\text{pure states}),\qquad \eta(\tau)\approx\eta_0\,e^{-\tau/T_{\rm mem}},\qquad 1-\eta_0\propto\frac{1}{\mathrm{OD}_{\rm EIT}},\qquad B\tau_{\rm delay}\approx\sqrt{\mathrm{OD}_{\rm EIT}}. \]
Worked example · how many pulses fit?

With ODEIT ≈ 9.6 the time–bandwidth product is √9.6 ≈ 3. Only about three distinguishable pulses fit in the medium at once. Raising it to 30 gives ≈ 5.5. This is why OD is the resource (paper Sec. IV). The exponential storage-decay form above is a simple model; real decay curves can be non-exponential (e.g. diffusion).

Q1. Can a memory have 99 % fidelity and 10 % efficiency?
Yes. Fidelity (conditional on retrieval) and efficiency are separate figures of merit. Many demonstrations report both.
Q2. Why does the project first benchmark with classical (attenuated) light?
Efficiency, delay, bandwidth and storage time can be measured with weak classical pulses on standard photodiodes. That calibrates the platform before single-photon sources and detectors (L11, Objective 3) are introduced.
Go deeper · platforms, protocols and how to compare memories fairly
Protocols in one line each
  • EIT memory (this project): resonant, control-field driven, narrow bandwidth, long storage in suitable media (Fleischhauer & Lukin 2000; Ma et al. 2017).
  • Raman memory: off-resonant, broad bandwidth, noise from the strong control to be filtered (Reim et al. 2010).
  • Atomic frequency comb and related rare-earth schemes: multimode storage in an inhomogeneously broadened solid (Afzelius et al. 2009).
Platforms (examples; read the papers for the numbers)
PlatformWhat it generally offersExamples
Warm atomic vapoursimplest apparatus, room temperature; limited by atomic motion and noiseReim et al. 2010; Namazi et al. 2017; Wolters et al. 2017; Finkelstein et al. 2023
Cold atomic ensembleslong coherence times and high reported efficiencies; needs laser cooling and vacuumCho et al. 2016; Vernaz-Gris et al. 2018
High-efficiency and multiplexed demonstrationsshow what the best memories achieve (efficiency, polarization qubits, many memory cells); check each paper for its medium and definitionsHsiao et al. 2018; Wang et al. 2019; Pu et al. 2017
Rare-earth-doped crystalsvery long coherence and multimode storage at cryogenic temperatureHedges et al. 2010; Zhong et al. 2015; Longdell et al. 2005; Afzelius et al. 2009
Entanglement-based repeaters with ensemblesDLCZ-type schemes using atomic ensemblesDuan et al. 2001; Kuzmich et al. 2003; Chanelière et al. 2005; Sangouard et al. 2011
Comparing numbers across papers

Reported efficiencies are not all the same quantity. Some are internal (inside the medium), some end-to-end (including all losses). Fidelities may be conditional on a photon being retrieved. Bandwidth and storage time trade off against each other. Always check what was measured, with what input (classical pulses or single photons), and in what basis. The reviews define these carefully (Lvovsky et al. 2009; Heshami et al. 2016; Bussières et al. 2013; Hammerer et al. 2010); for the networking context see Kimble 2008, Wei et al. 2022.

Why efficiency improves with optical depth

The stored pulse must be compressed to fit in the medium and then absorbed into the spin wave with little loss. Both need a large ODEIT (the number of absorption lengths the control “opens up”): inefficiency scales as 1/ODEIT and the time–bandwidth product as √ODEIT (Finkelstein et al. 2023; Gorshkov et al. 2007). That is why this project treats OD, γEIT and the coherence time as the three numbers to measure and optimize.

Pitfalls. (1) A memory benchmark must include the noise floor: classical light stored with high efficiency says nothing about the noise at the single-photon level (L11). (2) Storage time depends on the definition of when efficiency has “decayed”: say 1/e or 50 %. (3) Do not compare a nanosecond-bandwidth Raman memory with a kHz-bandwidth EIT memory on efficiency alone.
Sources

Reviews: Lvovsky et al. 2009, Hammerer et al. 2010, Heshami et al. 2016, Bussières et al. 2013, Ma et al. 2017, Novikova et al. 2011. Original proposals: Duan et al. 2001, Fleischhauer & Lukin 2002. Early demonstrations: Julsgaard et al. 2004, Chanelière et al. 2005, Eisaman et al. 2005.

Where it shows up: project framingwhat limits storagestorage audit step O2.8

L11

Quantum states of light: coherent, Fock, single photons, g⁽²⁾(0)

Learning goals
  • Contrast coherent states (lasers) with Fock states (single photons).
  • Use Poisson statistics to analyse attenuated laser pulses.
  • Interpret the second-order correlation g⁽²⁾(0).

A laser, however strongly attenuated, emits a coherent state: the photon number in a pulse is Poisson-distributed. Attenuation lowers the mean but never removes the chance of two photons. A true single-photon source (e.g. the α-MoO₃ emitters planned for Objective 3 in the project plan; see the source note in L12) ideally emits a Fock state |1⟩ with zero chance of two. The Hanbury Brown–Twiss measurement of g⁽²⁾(0) tells them apart.

L11.1\[ P(n)=e^{-\bar n}\frac{\bar n^{\,n}}{n!},\qquad g^{(2)}(0)=\frac{\langle\hat a^\dagger\hat a^\dagger\hat a\hat a\rangle}{\langle\hat a^\dagger\hat a\rangle^2}=\begin{cases}1&\text{coherent}\\ 2&\text{thermal}\\ 0&\text{single-photon Fock state}\end{cases} \]
Worked example · attenuated probe pulses

A 10 µs, 1 µW pulse at 795 nm holds ≈ 4.0 × 10⁷ photons (L1). For n̄ = 1, attenuate by 4 × 10⁷ (ND ≈ 7.6). At n̄ = 0.1: P(0) = 0.905, P(1) = 0.090, P(≥2) = 0.0047. About 5 % of non-empty pulses still contain two or more photons, which is why “single-photon-level” classical probes are not single photons.

Q1. What g⁽²⁾(0) would you measure for the Zeeman EIT probe laser?
≈ 1 (coherent light), regardless of attenuation.
Q2. Why does storing true single photons demand much better control filtering than storing a µW probe?
The signal is ~1 photon per pulse, while a mW control leaks, scatters and fluoresces. Even a 10⁻⁵ extinction (Glan–Taylor) leaves many control photons per pulse. Spectral filtering and timing gates are then needed too.
Go deeper · measuring photon statistics, sources of single photons, and the numbers for attenuated pulses
The Hanbury Brown–Twiss measurement

Send the light to a 50:50 beamsplitter with a detector on each output and count coincidences. Independent (Poissonian) arrivals give coincidences at the rate expected from chance; bunched (thermal) light gives more; a single photon cannot go to both detectors and gives none. The ratio is g(2)(0). The method originates with BROWN & TWISS 1956 (correlations between photons in two beams); the quantum theory is Glauber’s (Glauber 1963; Glauber 1963, Nobel Prize 2005, Nobel 2005); antibunching was first observed in resonance fluorescence by Kimble et al. 1977.

State⟨n⟩g(2)(0)Photon-number distribution
Coherent |α⟩|α|²1Poisson
Thermaln̄2geometric (Bose–Einstein)
Fock |n⟩, n ≥ 1n1 − 1/n (0 for n = 1)exactly n
Squeezed vacuumsinh²r3 + 1/⟨n⟩even photon numbers only

The 3D Wigner-function illustration above shows what each of these looks like in phase space; the numbers it reports are exactly this table.

Why attenuation never makes a single-photon source
L11.2\[ P(\ge2)=1-e^{-\bar n}(1+\bar n)\simeq\frac{\bar n^2}{2}\ \ (\bar n\ll1),\qquad \frac{P(\ge2)}{P(\ge1)}\simeq\frac{\bar n}{2}. \]

At n̄ = 0.1, P(≥2) = 0.0047 and the fraction of non-empty pulses with two or more photons is ≈ n̄/2 = 5 %: reducing n̄ lowers the multi-photon probability only in proportion, while the empty pulses (90 %) increasingly dominate. A real single-photon source suppresses multi-photon events without making most pulses empty.

Real single-photon sources

Heralded sources detect one photon of a pair to announce the other, including atomic-ensemble sources (Kuzmich et al. 2003). Single quantum emitters (quantum dots, defects, molecules) emit one photon per excitation cycle (Michler et al. 2000); solid-state emitters are reviewed in Aharonovich et al. 2016. For each, the figures of merit are g(2)(0) (purity), brightness, indistinguishability and bandwidth. Matching the emitter’s photons in colour, bandwidth and timing to a memory is a major challenge (L10 and L12).

Pitfalls. (1) Background light and detector dark counts raise g(2)(0) above its true value, so “g(2) < 0.5” alone is not proof of a single emitter without care. (2) “Single-photon level” attenuated pulses are still coherent states. (3) A detector’s dead time and timing jitter limit the shortest delays you can resolve.
Sources

Loudon, Gerry & Knight, Fox 2006, Garrison & Chiao 2008, Kok & Lovett 2010; originals: BROWN & TWISS 1956, Glauber 1963, Kimble et al. 1977; sources: Michler et al. 2000, Aharonovich et al. 2016, Kuzmich et al. 2003.

Where it shows up: probe attenuation & separation

L12

Strong coupling, cavity QED and polaritons in solids: the bridge to Objective 3

Learning goals
  • Define the strong-coupling condition and cooperativity.
  • See how an ensemble gives collective enhancement g√N.
  • Understand, without overclaiming, how microcavity polaritons relate to this project.

Put an emitter in an optical cavity. If the emitter–photon coupling g beats both the cavity loss κ and the emitter decay γ, energy oscillates back and forth and the spectrum splits into two polariton peaks separated by the vacuum Rabi splitting. N emitters coupled to the same mode act collectively with g√N. The EIT paper makes the same point for vapours: strong light–matter coupling arises from collective enhancement of a large ensemble, and “no high-quality cavity is required”.

Objective 3 concerns solid-state systems. The solid-state literature includes studies of P3HT under ultrastrong coupling (Nagarajan et al. 2020) and of low-loss phonon polaritons in α-MoO₃ (Ma et al. 2018). Whether such systems can support EIT-like storage at room temperature is precisely the open question the calibrated Rb platform is meant to help test. Nothing here should be read as a claim that they do (see the source note in “Go deeper”).

L12.1\[ g\gg\kappa,\gamma\ \ (\text{strong coupling}),\qquad C=\frac{4g^2}{\kappa\gamma},\qquad \hbar\Omega_R=2\hbar g\sqrt{N}\ \ (\text{collective vacuum Rabi splitting}),\qquad \frac{g}{\omega}\gtrsim0.1\ \ (\text{a common ultrastrong criterion}). \]
Worked example · same idea, different scales

In the Rb cell, the “coupling” that matters is collective: OD ≈ 10 means the ensemble absorbs strongly without any cavity. In ultrastrong-coupling studies of solids the Rabi splitting is a sizeable fraction of the transition energy itself (the criterion g/ω ≳ 0.1 in L12.1), whereas in the Rb cell the collective coupling is tiny compared with the 1.56 eV (377 THz) photon energy of L1 and it is the optical depth, not a large splitting, that matters. These are very different physical regimes, which is why Objective 3 begins with careful calibration on the Rb platform.

Q1. Why does an atomic ensemble not need a cavity to reach strong collective coupling?
The relevant figure, OD, grows with atom number. Many atoms each weakly coupled add up (g√N, or OD ∝ N L), so a single pass through a dense cell gives strong light–matter interaction.
Q2. Does a large Rabi splitting imply a good quantum memory?
No. A memory also needs a long-lived, controllable coherence (like γ₁₂ in Rb) and a way to switch the coupling on and off. Splitting measures coupling strength, not storage time.
Go deeper · the Jaynes–Cummings ladder, polaritons in solids, and what the project plan does and does not establish
The Jaynes–Cummings model
L12.2\[ \hat H_{\rm JC}=\hbar\omega_c\hat a^\dagger\hat a+\hbar\omega_a\hat\sigma^\dagger\hat\sigma+\hbar g\big(\hat a\hat\sigma^\dagger+\hat a^\dagger\hat\sigma\big),\qquad E_{n,\pm}=\hbar\omega\Big(n+\tfrac12\Big)\pm\hbar g\sqrt{n+1}\ \ (\text{on resonance; }n=\text{photons in the }g\text{ component}). \]

One two-level emitter and one mode (Jaynes & Cummings 1963; the cavity-QED experiments are reviewed in Haroche & Raimond 2006 and the Nobel lecture Haroche 2013). On resonance the states split into doublets with a gap 2g√(n + 1): for the first excitation, the vacuum Rabi splitting 2g. The ladder’s square-root spacing is a purely quantum signature. N identical emitters sharing the mode give √N-enhanced coupling, which is the collective strong coupling of an atomic ensemble and of molecular or excitonic layers in cavities (Törmä & Barnes 2014; Ebbesen 2016). The 3D avoided-crossing illustration shows the semiclassical two-mode limit of the same physics.

Polaritons in solids

A polariton is a mixed light–matter excitation. In a crystal, the coupling of light to excitons gives exciton polaritons (Hopfield 1958); in a semiconductor microcavity the exciton–photon mode splitting was reported by Weisbuch et al. 1992 and polariton condensation by Kasprzak et al. 2006. In polar crystals the matter part can be a lattice vibration (phonon polaritons): for example the low-loss, in-plane anisotropic phonon polaritons in α-MoO₃ (Ma et al. 2018). The wider literature on strong and ultrastrong coupling between light and matter, including the criteria g/ω ≳ 0.1 for ultrastrong coupling, is reviewed in Frisk Kockum et al. 2019 and Forn-Díaz et al. 2019; a broad overview of polaritons across materials is Basov et al. 2020. Organic semiconductors such as P3HT have been studied under ultrastrong coupling in the context of conductivity and photoconductivity (Nagarajan et al. 2020).

What this does and does not tell you about Objective 3
Be careful with claimsA large splitting shows that light and matter are strongly coupled, not that the system can store a quantum state: a memory also needs a long-lived coherence that can be switched on and off (L7, L8, L10). In a room-temperature solid the relevant coherences are generally much shorter-lived than the ground-state coherence of an atomic vapour, so whether EIT-like storage can work in a given material is an open experimental question. Light-matter coupling has been demonstrated, and EIT-type transparency has been seen in several solid-state systems (Turukhin et al. 2001; Longdell et al. 2005), but not at room temperature in the specific materials of the project’s next stage; this page makes no claim that it will. Source check: an earlier version of this lecture quoted a Rabi splitting of ~0.6 eV for P3HT from the project plan. That value could not be matched to the literature consulted for this revision, so it has been removed; the cited publications should be checked directly. Likewise the use of α-MoO₃ as a single-photon emitter is the project plan’s own statement: the α-MoO₃ literature cited here concerns phonon polaritons, so check the plan’s source for the emitter claim.
Pitfalls. (1) Strong coupling needs g > κ and γ: a large g with a lossy cavity or emitter shows no resolved splitting. (2) A Rabi splitting seen in a transmission spectrum can also come from effects that do not involve strong coupling (for example overlapping absorption and cavity lines); compare with the criteria in the reviews. (3) Do not carry numbers between platforms: a collective vapour coupling and a single quantum emitter in a cavity are in different regimes.
Sources

Jaynes & Cummings 1963, Haroche & Raimond 2006, Haroche 2013; polaritons: Hopfield 1958, Weisbuch et al. 1992, Kasprzak et al. 2006, Basov et al. 2020; strong and ultrastrong coupling: Törmä & Barnes 2014, Frisk Kockum et al. 2019, Forn-Díaz et al. 2019, Ebbesen 2016; materials: Ma et al. 2018, Nagarajan et al. 2020; EIT in solids: Turukhin et al. 2001, Longdell et al. 2005, Abdumalikov et al. 2010.

Where it shows up: project framing (next stage)platform choice

L13

Lab fundamentals for the project: polarization, Gaussian beams, AOMs, locking, cells, detectors, safety

Learning goals
  • Predict how waveplates, PBSs and Glan–Taylor polarizers turn H and V light into σ⁺ and σ⁻, and why the order matters.
  • Calculate beam size, Rayleigh range, intensity and Rabi frequency from a power and a waist.
  • Explain how an acousto-optic modulator and a double pass set the two-photon detuning.
  • Understand saturated-absorption locking, the field requirement for the cell, and the noise of a photodiode.
  • Work safely with an invisible 795 nm beam.

Lectures L1–L12 explain the atomic physics. This lecture explains the bench: the optical and electronic tools that turn the physics into a measurement, in the same order that the 3D bench simulator lays them out. Each part ends with what to check on the real bench, because every number in the model has to be measured, not assumed.

L13.1 Polarization: Jones vectors, waveplates and the Poincaré sphere

Light that is fully polarized is described by a two-component Jones vector (the amplitudes along horizontal and vertical, with their relative phase; Jones 1941). Optical elements are 2×2 matrices acting on it. A half-wave plate at angle θ to horizontal reflects the polarization about its fast axis: linear light at angle φ leaves at 2θ − φ. A quarter-wave plate turns linear light at 45° to its axis into circular light and vice versa. A polarizing beamsplitter transmits H and reflects V. Zeeman EIT uses all three: an HWP and PBS to set the probe/control split, a QWP to make σ⁺ and σ⁻, and a Glan–Taylor polarizer, whose extinction is of order 10⁵ (the paper), to remove the control after the cell (a PBS manages only about 10³).

L13.1\[ \mathbf J_{\rm H}=\begin{pmatrix}1\\0\end{pmatrix},\ \ \mathbf J_{\rm V}=\begin{pmatrix}0\\1\end{pmatrix},\ \ \mathbf J_{\sigma^\pm}=\tfrac1{\sqrt2}\begin{pmatrix}1\\ \pm i\end{pmatrix},\qquad \mathbf M_{\rm HWP}(\theta)=\begin{pmatrix}\cos2\theta&\sin2\theta\\ \sin2\theta&-\cos2\theta\end{pmatrix},\qquad \mathbf M_{\rm QWP}(\theta)=\mathbf R(-\theta)\begin{pmatrix}1&0\\0&i\end{pmatrix}\mathbf R(\theta). \]
L13.2\[ S_0=|E_H|^2+|E_V|^2,\quad S_1=|E_H|^2-|E_V|^2,\quad S_2=2\,\mathrm{Re}(E_H^*E_V),\quad S_3=2\,\mathrm{Im}(E_H^*E_V),\qquad S_1^2+S_2^2+S_3^2=S_0^2\ \ (\text{fully polarized}). \]
Worked example · why the plate angles are what they are

With the convention of L13.1 (field E = Re[J e−iωt], so σ⁺ rotates counter-clockwise about the beam), a QWP at +45° gives M = ½[[1+i, 1−i], [1−i, 1+i]]. Then H = (1, 0) → ½(1+i, 1−i) ∝ (1, −i)/√2 = σ⁻, and V = (0, 1) → ½(1−i, 1+i) ∝ (1, i)/√2 = σ⁺. The probe (H) and the control (V) therefore enter the cell with opposite circular polarizations, as the Λ system needs (L5, L7). After the cell, a second QWP at −45° maps σ⁺/σ⁻ back to V/H, and a Glan–Taylor set to pass the probe’s polarization removes the control. The same QWP at +45° would turn a σ⁺ beam into H. Which circular state is which depends on the sign convention of the quantization axis and on whether a mirror has reflected the beam, so always check the sense with the experiment (or the simulator’s Stokes readout) rather than relying on a label.

Pitfalls. (1) Reflection from a mirror reverses the helicity relative to the propagation direction. (2) A waveplate’s “zero order, 780 nm” design is close to, but not exactly, a quarter-wave at 795 nm: check the retardance and tune the angle for best circular purity. (3) Polarization-maintaining fibre carries only the axes it is aligned to: a few degrees of misalignment leaks power into the wrong polarization and into the SAS reference.
Q1. What does an HWP at 22.5° do to horizontal light?
It rotates the polarization by 2 × 22.5° = 45°: H → D (+45° linear), a point on the S₂ axis of the Poincaré sphere.
Q2. In Zeeman EIT the control power fraction is set by an HWP before a PBS. If the plate angle is θ and the input is H, what fraction goes to the transmitted (H) port?
cos²(2θ), and the reflected (V) port gets sin²(2θ), with θ measured from horizontal. In the reference bench the light reaching this plate is pure H (the pick-off PBS has already cleaned it), and a plate at 10° sends sin²(20°) ≈ 12 % to the probe port.

L13.2 Gaussian beams: size, focus, intensity

A laser beam in free space is a Gaussian beam: its intensity across the beam is a Gaussian, and its radius w(z) (where the intensity has fallen to 1/e² of the peak) is smallest at the waist w₀ and grows on either side (Kogelnik & Li 1966; Siegman 1986; Saleh & Teich). The distance over which the beam stays roughly collimated is the Rayleigh range zR. These few formulas decide four things on the bench: the intensity that sets the Rabi frequency (L3), the time atoms spend in the beam (L9), whether the beam fits through an AOM crystal, and how to focus into the cat’s-eye of a double pass.

L13.3\[ w(z)=w_0\sqrt{1+(z/z_R)^2},\qquad z_R=\frac{\pi w_0^2}{\lambda},\qquad I_0=\frac{2P}{\pi w_0^2},\qquad w_0'=\frac{\lambda f}{\pi w}\ \ (\text{beam of radius }w\text{ focused by a lens of focal length }f). \]
Worked example · from power to Rabi frequency

For a collimated beam of waist w₀ = 0.75 mm at 794.979 nm: zR = π(0.75 mm)²/λ = 2.2 m, so the beam stays nearly parallel over the whole table; the half-angle divergence is λ/(πw₀) = 0.34 mrad. Its peak intensity for P = 1 mW is 2P/(πw₀²) = 113 mW/cm². The paper’s control intensities were 1.3 and 5.5 mW/cm² (Finkelstein et al. 2023); for a beam of radius 2.55 mm (the value used in the simulator) these correspond to only P = I₀πw²/2 ≈ 0.13 mW and 0.56 mW. With Γ/2π = 5.750 MHz and the far-detuned π-light Isat = 4.488 mW/cm² Steck, the two-level estimate of L3 gives Ω/2π = (Γ/2π)√(I/2Isat) ≈ 2.2 MHz at 1.3 mW/cm² (the paper quotes 1.9 MHz). A lens of f = 100 mm focuses a beam of w = 0.75 mm to w₀′ = λf/(πw) ≈ 34 µm, with zR ≈ 4.5 mm: tight focusing is only forgiving over millimetres, which is why the position of the AOM crystal and of the cat’s-eye mirror matters.

Q1. Doubling the waist radius at constant power changes the peak intensity by what factor?
I₀ ∝ 1/w₀², so it falls by 4. The Rabi frequency ∝ √I falls by 2.
Q2. Why is a beam that is 1.5 mm in diameter at the AOM aperture often focused in the crystal?
The crystal’s useful aperture is about as large as the beam, so an unfocused beam clips at the edges and loses efficiency. Focusing inside the crystal shrinks the beam so it fits easily (and a smaller beam also gives a faster rise time, see L13.3). The price is a larger divergence, which the following lens must re-collimate.

L13.3 Acousto-optic modulators and the double pass

In an AOM a radio-frequency signal drives a transducer that launches a sound wave through a crystal. The sound is a moving diffraction grating: light entering at the Bragg angle is diffracted into a first order that is shifted in frequency by the sound frequency (Siegman 1986; Saleh & Teich). The deflection angle depends on the RF frequency, which is a nuisance when the beam must stay aligned. The double pass (Donley et al. 2005) fixes it: the first order is focused by a lens onto a mirror at the lens focus (a cat’s-eye), which sends it back through the AOM along its own path. The returning beam is diffracted a second time onto the original axis, so the output direction no longer depends on the RF frequency, and the total shift is doubled. A quarter-wave plate crossed twice turns the polarization by 90°, so a polarizing beamsplitter can lift the returning beam out of the input path. Zeeman EIT uses one such double pass per arm.

L13.4\[ \theta_{\rm defl}\simeq\frac{\lambda f_{\rm RF}}{v_s},\qquad \Delta\nu_{\rm out}=\pm2f_{\rm RF}\ \ (\text{double pass}),\qquad \delta=2\big(f_{\rm RF,c}-f_{\rm RF,p}\big)=\mu_Bg\,\Delta m\,B/h,\qquad t_{\rm rise}\approx0.64\,\frac{D}{v_s}. \]
Worked example · numbers for the 80 MHz TeO₂ AOMs

The slow shear acoustic mode of TeO₂ has a sound velocity of about 0.62 km/s (617 m/s along ⟨110⟩ in the literature on TeO₂ acousto-optic devices); this low velocity is what gives the large deflection angles. For λ = 795 nm and fRF = 80 MHz the deflection is θ ≈ λf/vs = (795 nm × 80 MHz)/617 m/s ≈ 0.10 rad ≈ 6° estimate: check the device data sheet. That is why the simulator draws the first order at an exaggerated 8°. A beam of diameter D = 1.5 mm has a rise time of about 0.64 × D/vs ≈ 1.6 µs rule of thumb, which limits how fast the control can be switched in the storage sequence (L8). In the reference bench the control RF is 80.000 MHz and the probe RF 79.965 MHz, so after the double pass they differ by 2 × 35 kHz = 70 kHz, equal to the Zeeman splitting 1.40 kHz/mG × 50 mG of the mF = +2 and 0 pair (L5). Both beams are also shifted by about +160 MHz from the laser, so the laser lock must be planned with that offset in mind (see the Zeeman EIT architecture).

Pitfalls. (1) Align the cat’s-eye by watching the returning beam while sweeping the RF frequency: when it is right, the returning beam does not walk. (2) Never run the RF amplifier without the AOM (or a 50 Ω load) attached. (3) The 0th-order and the unwanted returning-pass light must go to beam dumps; otherwise they scatter onto the detector. (4) Leave the RF on during alignment: thermal changes in the crystal shift the optimum angle.
Q1. The control AOM runs at 80.000 MHz and the probe AOM at 79.950 MHz, both double-passed. What is the probe–control frequency difference?
2 × (79.950 − 80.000) MHz = −100 kHz. The sign depends on which order each AOM uses; in the reference bench both use the +1 order.
Q2. Why is a high-power RF amplifier needed at all?
The first-order efficiency depends on the acoustic power, and an AOM typically needs hundreds of milliwatts to a watt or two of RF for good efficiency (check the data sheet). The synthesizer outputs far less, so each arm has an attenuator/switch (to set the level and gate the arm) followed by an amplifier.

L13.4 Saturated-absorption spectroscopy and locking the laser

A free-running diode laser drifts by tens of MHz; Zeeman EIT needs the one-photon detuning stable to the MHz scale (L9, L7). The reference is the atom itself, read out by saturated-absorption spectroscopy (Preston 1996; MacAdam et al. 1992; Demtröder). A strong pump and a weak probe cross the same vapour from opposite directions. Atoms moving along the beam see the pump and probe at opposite Doppler shifts, so only atoms with nearly zero velocity along the beam are resonant with both. The pump saturates them, and the probe sees a narrow dip (as narrow as the natural width, here a few MHz) in the 500 MHz-wide Doppler absorption. Where two lines share a velocity class, a crossover resonance appears exactly midway between them.

To lock on such a dip you need an error signal that is zero on the line and changes sign across it: the derivative of the dip. A small current dither on the diode, with lock-in detection at the dither frequency, gives it. The lock box feeds the error back to the laser current, and slow drifts are removed by retuning the temperature, since a DFB has no piezo (Wieman & Hollberg 1991; the dither/lock-in and the Pound–Drever–Hall method are compared in Black 2001 and Drever et al. 1983).

L13.5\[ e(\Delta)\propto-\frac{d}{d\Delta}\,\mathcal L(\Delta)=\frac{2\Delta/(\Gamma/2)^2}{\big[1+(2\Delta/\Gamma)^2\big]^2},\qquad \Delta\nu_{\rm Dop}^{\rm FWHM}\approx530\ \mathrm{MHz}\ \gg\ \Gamma/2\pi=5.75\ \mathrm{MHz}. \]
Worked example · why the SAS shows resolved features on D1

For ⁸⁷Rb D1, the ground hyperfine splitting is 6 834.683 MHz and the excited-state splitting F′ = 1 to F′ = 2 is 814.5(13) MHz Steck. The Doppler FWHM is about 530 MHz, so the F = 2 and F = 1 absorption lines are completely separate, and each shows two Doppler dips (to F′ = 1 and F′ = 2), partly resolved, 814 MHz apart. Zeeman EIT locks near F = 2 → F′ = 1 (see the Zeeman EIT architecture). The AOM shifts (about +160 MHz in total) must be taken into account so that the beam reaching the cell, not just the SAS beam, ends up on the intended atomic resonance.

L13.5 The vapour cell, the field and the shield

The optical depth of the cell rises steeply with temperature, because the density of rubidium vapour follows the vapour pressure, which grows roughly exponentially with T (Steck, Rb-87 data, vapour-pressure model). At 25 °C the vapour pressure is 3.92 × 10⁻⁷ Torr, which with the ideal-gas law gives n = P/kBT ≈ 1.3 × 10¹⁰ cm⁻³ Steck; at 60 °C the density is roughly 20 to 25 times higher design estimate, in the range 10¹¹–10¹² cm⁻³ that the paper treats as typical (Finkelstein et al. 2023). Heating the cell is therefore the main OD knob.

Magnetic fields are the other. The two-photon resonance of Zeeman EIT moves by 1.40 kHz per milligauss (L5), while the EIT line is only about 7 to 26 kHz wide: a stray field of just 5 mG shifts the resonance by 7 kHz, which is as large as the linewidth. Earth’s field is roughly 0.5 G, a hundred times bigger. That is why the cell sits in a µ-metal shield (three nested layers in the paper) with a solenoid inside to provide a small, known, stable bias field along the beams, and why the shield must be degaussed after assembly: leftover magnetization otherwise sets the residual field.

L13.6\[ B=\mu_0\,\frac{N}{L_{\rm sol}}\,I,\qquad \delta_{\rm Zeeman}=\frac{2\,g_F\,\mu_B}{h}\,B=1.40\ \mathrm{kHz/mG}\times B\ \ (m_F=+2\leftrightarrow0,\ g_F=\tfrac12),\qquad n_{\rm at}=\frac{P_{\rm vap}}{k_BT}. \]
Worked example · the solenoid and its current source

A long solenoid with 1000 turns per metre produces B = μ₀(N/L)I = 12.6 mG for every milliampere. To make 50 mG you need I = 50/12.57 ≈ 4.0 mA. A current error of 1 µA changes B by 12.6 µG, which moves the two-photon resonance by 1.40 kHz/mG × 0.0126 mG ≈ 18 Hz: negligible against a 7 kHz line. But a 1 % drift (40 µA) shifts B by 0.5 mG, i.e. 0.7 kHz: a visible fraction of the linewidth. So the coil supply needs ~0.1 % stability, and the bias should be well above the residual field the shield leaves behind (otherwise the residual, not the coil, sets the resonance). A fluxgate magnetometer measures the residual and calibrates the coil.

Q1. Earth’s field is 0.5 G and the EIT line is 10 kHz wide. By what factor must the shield reduce the field to keep the shift below the line width?
0.5 G = 500 mG shifts the pair by 500 × 1.40 kHz = 700 kHz. To get below 10 kHz you need B ≲ 7 mG, a reduction by at least 70. In practice you want a much smaller shift (a small fraction of the line), so a shielding factor of several hundred or more.
Q2. Why is the heater wound bifilar (current flowing out and back in adjacent wires)?
The two opposite currents produce opposite magnetic fields that cancel at a distance. A single-wire winding of the same current would add a field of its own at the atoms and shift or broaden the resonance.

L13.6 Detectors and noise

A photodiode converts power P into a current I = RP with responsivity R = ηeλ/hc, about 0.64 A/W per unit quantum efficiency at 795 nm; silicon photodiodes are around 0.5 A/W near 800 nm (check the data sheet). The current is converted to a voltage by a transimpedance amplifier. Three noise sources compete: shot noise of the photocurrent itself, thermal (Johnson) noise of the feedback resistor, and amplifier noise (Saleh & Teich). At the microwatt power levels of the probe the resistor and shot noise are comparable, and below that the resistor noise wins, so the signal-to-noise ratio improves by averaging (the scope) or by using a lower bandwidth.

L13.7\[ I=RP,\quad R=\frac{\eta e\lambda}{hc}\approx0.64\,\eta\ \mathrm{A/W},\qquad i_{\rm shot}=\sqrt{2eI\,\Delta f},\qquad i_{\rm Johnson}=\sqrt{\frac{4k_BT\,\Delta f}{R_f}}. \]
Worked example · is the probe signal shot-noise limited?

Take R = 0.5 A/W, P = 1 µW and a measurement bandwidth Δf = 1 MHz. The photocurrent is 0.5 µA and the shot noise is √(2 × 1.602 × 10⁻¹⁹ × 0.5 × 10⁻⁶ × 10⁶) ≈ 0.40 nA (signal-to-noise 1250). A feedback resistor Rf = 100 kΩ at 300 K adds √(4 × 1.38 × 10⁻²³ × 300 × 10⁶/10⁵) ≈ 0.41 nA, the same size: at 1 µW the two are equal (the crossover is at I = 2kBT/(eRf) ≈ 0.52 µA). For the weaker probe powers typical of EIT the resistor noise wins, so a larger Rf (at the cost of bandwidth) or averaging is the way to gain, and single-photon work needs a different detector altogether (L1 Q2, L11). Also check the scope’s input: a 1 MΩ input with a long cable forms a low-pass filter that narrows the real bandwidth.

Q1. A probe of 10 nW at 795 nm on a silicon photodiode with R = 0.5 A/W gives what photocurrent, and what voltage through 1 MΩ?
I = 0.5 × 10⁻⁸ = 5 nA, so V = 5 nA × 1 MΩ = 5 mV. Small, but well above the shot noise; the amplifier and scope noise will decide visibility.

L13.7 Laser safety

The 795 nm beam is in the near infrared: invisible, but focused by the eye onto the retina like visible light. Because you cannot see it, the blink reflex does not protect you, and the damage is permanent. Beam powers of a few to tens of milliwatts in the experiment generally fall in laser classes 3R or 3B under the international standard (IEC 60825-1) and the corresponding American one (ANSI Z136.1); the exact class depends on power and wavelength-dependent limits, so confirm the classification with your institution’s laser safety officer and follow the local rules.

Habits that keep the bench safe
  • Wear eyewear whose optical density at 795 nm is marked on the glasses (OD 6 or more at the working power is typical): the marking must cover the exact wavelength, and the glasses are specific to the laser.
  • Keep all beams in the plane of the table and below eye level when seated or standing. Remove watches and reflective jewellery.
  • Align at low power. Use an IR viewing card or an IR camera, never your eye. Block every unused order and every leakage port with a beam dump; reflections from optics are beams too.
  • Enclose the beam path where possible. Put up warning signs and tell everyone entering when the laser is on.
  • Before changing anything in a beam path, block the beam. After changing it, re-check where every reflection goes.

L13.8 Alignment and measurement routines

The reference bench in the simulator is not just a diagram: it is a checklist. Three habits prevent most problems. First, fix the master axis with two mirrors and two irises before adding anything else: centre the beam on both irises by adjusting the mirrors alternately; every optic between them is then on axis. Second, measure each stage: the power after the isolator, the pick-off ratio, the control/probe split, the AOM efficiency (first-order power over input) and the double-pass efficiency, the polarization purity after each PBS, and the power at the cell. Compare each with what the simulator predicted for the same settings; a discrepancy is information. Third, change one thing at a time and write it down: plate angle, RF frequency, temperature, bias current. A logbook is the cheapest instrument in the lab.

StageMeasureWhat to expect (reference bench)If not
Laser and isolatorpower before and after≈ 80 % transmission of the 10 mW source (≈ 1 dB fibre-isolator loss plus connectors; simulator assumption)check polarization into the isolator and its direction
Pick-off to SASfraction reaching the SAS photodiodea few percent, set by the first half-wave platerotate the plate; check the PBS orientation
Control/probe splitpower in each armprobe ≈ 10 %, control the restrotate the second half-wave plate
AOM efficiencyfirst-order power / input power per passtens of percent per pass; η² double-passreoptimize the Bragg angle and RF power; focus in the crystal
Double-pass returndoes the returning beam walk as the RF changes?no walk when the cat’s-eye is rightadjust the lens and mirror position
Recombinationoverlap in the cell (two beam positions and angles)overlapping to a small fraction of the beam size, parallel to well below a milliradianwalk the beams with the last two mirrors in each arm
Polarizations in the cellcircular purity with a rotating analyseropposite circular states for probe and controltrim the plate angles; check mirror reflections
Field in the shieldfluxgate reading vs coil currentlinear; residual far below the biasdegauss again; check for magnetic parts near the shield

Where it shows up: Zeeman EIT architecture3D bench simulatorbring-up and audit protocolwiring diagramequipment list

Go deeper · sources for L13
R

Reading and sources

Every item below was checked against its publisher or library record: journal articles through their DOI (the full list with DOIs is under “References” at the end), and books by author, title, publisher and year. If you find an error, tell the group. Items marked collected were gathered earlier by the researcher and could not be fully verified; they are kept for completeness.

Textbooks by purpose

Original papers (history)

Slow light, storage and memories

The project’s main reference

Strong coupling and polaritons

Lab methods

Collected links collected

A

Appendix A · Symbols

The same definitions that appear when you hover over a symbol. Click a lecture link to jump to where the symbol is used first.

B

Appendix B · Constants and ⁸⁷Rb data used in these notes

Fundamental constants are the 2018 CODATA recommended values as tabulated in Steck, Rb-87 data (Table 1); atomic data are from the same document, revision 2.3.4 (8 August 2025). Digits in parentheses are the standard uncertainty in the last digits.

QuantityValue
Speed of light c299 792 458 m/s (exact)
Planck constant h6.626 070 15 × 10⁻³⁴ J·s (exact); 4.135 667 696… × 10⁻¹⁵ eV·s
Reduced Planck constant ħ1.054 571 817… × 10⁻³⁴ J·s
Elementary charge e1.602 176 634 × 10⁻¹⁹ C (exact)
Boltzmann constant kB1.380 649 × 10⁻²³ J/K (exact)
Vacuum permittivity ε₀8.854 187 817… × 10⁻¹² F/m
Bohr magneton µB9.274 010 078 3(28) × 10⁻²⁴ J/T; µB/h = 1.399 624 493 61(42) MHz/G
Atomic mass unit u1.660 539 066 60(50) × 10⁻²⁷ kg
⁸⁷Rb mass86.909 180 520(15) u
⁸⁷Rb nuclear spin; abundanceI = 3/2; 27.83(2) %
D1 line (5S₁/₂ → 5P₁/₂): vacuum wavelength794.978 851 156(23) nm (794.766 477 6 nm in air)
D1 frequency; photon energy377.107 463 380(11) THz; 1.559 591 154 eV
D1 lifetime τ; decay rate Γ27.679(27) ns; Γ = 36.129(35) × 10⁶ s⁻¹; Γ/2π = 5.7500(56) MHz
D1 saturation intensity (far-detuned, π-polarized)Isat = 4.4876(43) mW/cm²
D1 reduced dipole matrix element⟨J = ½‖er‖J′ = ½⟩ = 2.5377(12) × 10⁻²⁹ C·m (2.9931(14) ea₀)
D1 recoil velocity5.7754 mm/s
D2 line (5S₁/₂ → 5P₃/₂): wavelength; Γ/2π780.241 209 686(13) nm; 6.0666(18) MHz
Ground hyperfine splitting6.834 682 610 904 290(90) GHz
D1 excited hyperfine splitting (F′ = 2 to 1)814.5(13) MHz
gF: 5S₁/₂ F = 2, 1; 5P₁/₂ F′ = 2, 1+½, −½ (±0.70 MHz/G); +1/6, −1/6 (±0.23 MHz/G)
Nuclear g-factor gI−0.000 995 141 4(10)
Clock-transition quadratic Zeeman shift2π × 575.15 Hz/G²
Vapour pressure at 25 °C3.92(20) × 10⁻⁷ Torr
C

Appendix C · What was checked and corrected in this revision

The lecture notes were audited line by line against their sources before the primers and L13 were added. This record lets you see what changed and why.

WhereWhat was foundWhat was done
L3, L4, interactive lab, Appendix BΓ/2π = 5.746 MHz and τ = 27.70 ns, Isat = 4.484 mW/cm² come from an older data-sheet revision.Updated to Steck revision 2.3.4: Γ/2π = 5.7500 MHz, τ = 27.679 ns, Isat = 4.4876 mW/cm². The Rabi-frequency estimate (2.2 MHz) is unchanged to the digits quoted.
L7, L3The Autler–Townes doublet E± = ±ħΩc is in the paper’s Rabi convention (coupling ħΩ), while L3 defines Ω with coupling ħΩ/2: the two were not reconciled.Convention stated in P0 and in L7’s “Go deeper”; the paper’s Eq. 23 is labelled as such and the factor 2 is explained. Checked against the arXiv/NJP text.
L12A Rabi splitting of ~0.6 eV for P3HT was attributed to the project plan; it could not be matched to the literature consulted for this revision.The number was removed. The text now cites the verified publications and flags that the plan’s source should be checked directly. The α-MoO₃ literature found concerns phonon polaritons; the plan’s statement about single-photon emitters is flagged for source checking.
L2, L5Leftover references to “Method B” (removed from the guide).Rewritten as a general hyperfine (clock-state) Λ scheme.
Reading listSome items were paper-bibliography copies or unverified web links; one link pointed to a third-party copy of a book.Replaced by a verified list (each article checked against its DOI record, each book by author/title/publisher/year). Unverified web links are marked “collected”; the third-party copy link was removed.
All numerical examplesRe-derived: photon energy and flux (L1), thermal speed and Doppler width (L9), Poisson probabilities (L11), time–bandwidth product (L10), decay rate from the dipole moment (P5).No errors found other than those above. All derived values are labelled derived or estimate where appropriate.
Statements not checkedIllustrative numbers inherited from the simulator (storage efficiency, coherence time, EIT contrast scaling) remain labelled illustrative.Unchanged; measure them on the bench.
★

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