Start here: how to use these notes
- 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 only | P1 → 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 already | P2 (motivation), L5, L7–L10 (the project physics), L13 (the bench) |
| are building the bench now | L13 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
| Topic | Convention here |
|---|---|
| Units | SI, 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 frequency | ν 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 frequency | Ω 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. |
| Detuning | Δ = ωlaser − ωatom. The two-photon (Raman) detuning is δ. |
| Circular polarization | σ⁺ 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 depth | OD 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 tags | paper 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?
Q2. What is the frequency of 795 nm light?
Q3. What are the eigenvalues of the matrix [[0, 1], [1, 0]]?
Q4. For the state (|g⟩ + i|e⟩)/√2, what is the probability of finding |g⟩?
Q5. What are 1 mW and 1 µW in 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.
A short history: from light quanta to stored light
- 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.
- 1900Planck proposes that energy is exchanged in discrete amounts to explain the spectrum of thermal radiation (Planck 1901).
- 1905Einstein proposes that light itself comes in quanta, using the photoelectric effect as the test (Einstein 1905).
- 1913Bohr’s atom: discrete energy levels, spectral lines from jumps between them (Bohr 1913).
- 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.
- 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.
- 1923Compton scattering of X-rays supports the idea that a light quantum carries momentum (Compton 1923).
- 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).
- 1927Dirac quantizes the electromagnetic field and derives spontaneous emission from first principles (Dirac 1927); this is the root of P5.
- 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).
- 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.
- 1956Hanbury Brown and Twiss measure correlations between photons in two beams (BROWN & TWISS 1956): the technique behind g(2)(0) of L11.
- 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.
- 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).
- 1972Happer’s review of optical pumping (HAPPER 1972) collects the methods for preparing atoms in chosen sublevels.
- 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.
- 1977Kimble, Dagenais and Mandel observe photon antibunching in resonance fluorescence (Kimble et al. 1977): the first observation of this signature of non-classical light.
- 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.
- 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.
- 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.
- 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).
- 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).
- 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).
- 2008–09The vision of a quantum internet (Kimble 2008) and the review of optical quantum memory (Lvovsky et al. 2009).
- 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).
- 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.
- 2022Nobel Prize in Physics to Aspect, Clauser and Zeilinger for experiments with entangled photons and the pioneering of quantum information science (Nobel 2022).
- 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.
Why this project: quantum memories and quantum networks
- 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).
What a good memory needs
| Figure of merit | Meaning | Why it matters for a repeater |
|---|---|---|
| Efficiency η | probability that a stored photon comes back | loss in each memory multiplies along the chain |
| Fidelity ℱ | how closely the returned state matches the input | errors accumulate with every step |
| Storage time | how long the state survives before η falls | must exceed the time to learn that the neighbour succeeded (light travel time plus processing) |
| Bandwidth | the spectral width of pulses it can store | must match the photon source and the repetition rate |
| Multimode capacity | number of distinguishable pulses held at once | raises 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.
Q1. A fibre link is 200 km long with 0.2 dB/km loss. What fraction of photons arrives?
Q2. Why can an amplifier not rescue a quantum signal?
Q3. Why does a memory with high efficiency but a short storage time not help a long link?
Where it shows up: project framingquantum memory metrics (L10)Objective 3 context (L12)
Maths toolkit: complex numbers, matrices, Dirac notation, Fourier
- 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).
P3.2 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”.
P3.3 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.
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⟩.
P3.5 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).
P3.6 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
| Quantity | Value or conversion | Use |
|---|---|---|
| Photon energy vs wavelength | E[eV] = 1239.84 / λ[nm]; at 794.979 nm, E = 1.5596 eV | photon counting (L1) |
| Energy vs frequency | 1 eV ↔ 241.80 THz; 1 THz ↔ 4.1357 meV; 1 GHz ↔ 4.1357 µeV | comparing optical and hyperfine scales |
| Thermal energy | kBT at 333 K (60 °C) = 28.7 meV = 6.9 THz × h | why a hot vapour is thermal but still far below the optical photon energy |
| Rb D1 line | λ = 794.979 nm; ν = 377.107 THz; Γ/2π = 5.750 MHz (Steck) | everything |
| ⁸⁷Rb ground hyperfine splitting | 6.834 683 GHz (Steck) | Λ-system energy scale (L5) |
| Zeeman scale | µB/h = 1.3996 MHz/G, so gF = ½ gives 0.70 MHz/G per mF | shielding requirement (L5, L13) |
| Power in dBm | dBm = 10 log₁₀(P / 1 mW): 1 mW = 0 dBm, 1 µW = −30 dBm, +3 dB = ×2 | RF chain, photodiode signals (L13) |
| Optical depth | OD(e) = 2.303 × OD(10); 1 OD(e) = 4.34 dB; transmission = e−OD | cell, filters (L6, L13) |
| Intensity | 1 mW/cm² = 10 W/m² | control and probe intensities (L1, L3) |
Q1. Show that multiplying z = 1 by eiπ/2 gives i. What does that do to the arrow?
Q2. A two-level state has amplitudes (cos θ, sin θ). Are the two basis states’ amplitudes properly normalised?
Q3. A pulse has a Gaussian envelope of FWHM 5 µs. What is its minimum FWHM bandwidth?
Q4. Convert 3.77 × 10¹⁴ Hz to an energy in 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.
Basic quantum mechanics for atoms and photons
- 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 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 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 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 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.
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?
Q2. Why can a photon not take an atom from S to D in a single electric-dipole step?
Q3. What is the zero-point energy of a mode of frequency 377 THz, and why can it not be removed?
Where it shows up: L2 states and measurementL5 atomic structureP5 quantized light
Basic quantum optics: photons, coherent states and emission
- 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 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).
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.
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
| Mechanism | Shape | FWHM for ⁸⁷Rb D1 at 60 °C | Where covered |
|---|---|---|---|
| Natural (spontaneous emission) | Lorentzian | Γ/2π = 5.750 MHz Steck | L4 |
| 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 paper | L9 |
| 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?
Q2. If a transition’s dipole moment doubles (same frequency), what happens to its lifetime?
Q3. Why does the Doppler width not simply wash out EIT?
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.
Light as waves and photons
- 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.
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.
Q1. How many photons per second are in a 1 pW beam at 795 nm?
Q2. Why can the photodiode in Zeeman EIT not see individual 795 nm photons?
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
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
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
Quantum states, superposition and measurement
- 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).
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?
Q2. Why does a global phase eiφ|ψ⟩ not matter, while a relative phase does?
Go deeper · the Bloch sphere, measurement in other bases, and Ramsey interference
Two angles describe everything
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.
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
The two-level atom: dipole coupling, RWA, Rabi oscillations, Bloch sphere
- 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.
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.
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?
Q2. Why is the RWA safe for Rb D1 driven by a mW laser?
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
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
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
Open systems: density matrix, decay and dephasing
- 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.
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?
Q2. Why is γ₁₂ (ground coherence) potentially millions of times smaller than γ₁₃?
Go deeper · T₁, T₂, saturation and the scattering rate
The optical Bloch equations
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:
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).
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
Atomic structure for alkalis
- 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.
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?
Q2. Why is D1 preferred over D2 for clean Λ systems?
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)
| Quantity | Value |
|---|---|
| D1 line, 5S₁/₂ → 5P₁/₂ | λ = 794.978 851 nm (vacuum); ν = 377.107 463 THz; photon energy 1.559 591 eV |
| D2 line, 5S₁/₂ → 5P₃/₂ | λ = 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 spin | I = 3/2 (⁸⁷Rb, natural abundance 27.83 %) |
| gF factors | 5S₁/₂: +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.
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
Light–matter response: susceptibility, absorption, dispersion
- 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.
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?
Q2. Why does a narrow absorption feature imply a strong dispersion feature?
Go deeper · susceptibility, absorption coefficient, group index and the EIT susceptibility
From χ to what you measure
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
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).
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
Three-level interference: dark states, CPT, EIT, Autler–Townes
- 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]).
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?
Q2. Halving the control intensity halves which term of γEIT?
Go deeper · the Autler–Townes convention, telling EIT from AT, and what dark states are used for
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
- Slow and stored light (L8): the subject of this project (Fleischhauer & Lukin 2000; Phillips et al. 2001).
- CPT atomic clocks: the narrow dark resonance is used as a frequency reference (Vanier 2005).
- Magnetometry: the resonance shifts with magnetic field, and optical magnetometers use that sensitivity (Budker & Romalis 2007).
- EIT analogues in solids, superconducting circuits and optomechanics (Turukhin et al. 2001; Abdumalikov et al. 2010; Safavi-Naeini et al. 2011; Weis et al. 2010).
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
Slow and stopped light: group velocity, polaritons, storage
- 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.
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)?
Q2. Why must the control be turned off while the pulse is fully inside the cell?
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).
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
Thermal vapour realities: Doppler, transit, collisions, buffer gas
- 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.
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?
Q2. A beam angle of 0.1 mrad between probe and control: roughly how much residual broadening without buffer gas?
Go deeper · numbers for a warm cell, buffer gas, Dicke narrowing and its costs
The numbers
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.
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
Quantum memories: metrics, repeaters, networks
- 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.
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?
Q2. Why does the project first benchmark with classical (attenuated) light?
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)
| Platform | What it generally offers | Examples |
|---|---|---|
| Warm atomic vapour | simplest apparatus, room temperature; limited by atomic motion and noise | Reim et al. 2010; Namazi et al. 2017; Wolters et al. 2017; Finkelstein et al. 2023 |
| Cold atomic ensembles | long coherence times and high reported efficiencies; needs laser cooling and vacuum | Cho et al. 2016; Vernaz-Gris et al. 2018 |
| High-efficiency and multiplexed demonstrations | show what the best memories achieve (efficiency, polarization qubits, many memory cells); check each paper for its medium and definitions | Hsiao et al. 2018; Wang et al. 2019; Pu et al. 2017 |
| Rare-earth-doped crystals | very long coherence and multimode storage at cryogenic temperature | Hedges et al. 2010; Zhong et al. 2015; Longdell et al. 2005; Afzelius et al. 2009 |
| Entanglement-based repeaters with ensembles | DLCZ-type schemes using atomic ensembles | Duan 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.
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
Quantum states of light: coherent, Fock, single photons, g⁽²⁾(0)
- 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.
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?
Q2. Why does storing true single photons demand much better control filtering than storing a µW probe?
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|² | 1 | Poisson |
| Thermal | n̄ | 2 | geometric (Bose–Einstein) |
| Fock |n⟩, n ≥ 1 | n | 1 − 1/n (0 for n = 1) | exactly n |
| Squeezed vacuum | sinh²r | 3 + 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
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).
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
Strong coupling, cavity QED and polaritons in solids: the bridge to Objective 3
- 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”).
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?
Q2. Does a large Rabi splitting imply a good quantum memory?
Go deeper · the Jaynes–Cummings ladder, polaritons in solids, and what the project plan does and does not establish
The Jaynes–Cummings model
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
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
Lab fundamentals for the project: polarization, Gaussian beams, AOMs, locking, cells, detectors, safety
- 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).
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.
Q1. What does an HWP at 22.5° do to horizontal light?
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?
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.
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?
Q2. Why is a beam that is 1.5 mm in diameter at the AOM aperture often focused in the crystal?
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.
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).
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?
Q2. Why is a high-power RF amplifier needed at all?
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).
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.
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?
Q2. Why is the heater wound bifilar (current flowing out and back in adjacent wires)?
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.
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?
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.
- 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.
| Stage | Measure | What to expect (reference bench) | If not |
|---|---|---|---|
| Laser and isolator | power 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 SAS | fraction reaching the SAS photodiode | a few percent, set by the first half-wave plate | rotate the plate; check the PBS orientation |
| Control/probe split | power in each arm | probe ≈ 10 %, control the rest | rotate the second half-wave plate |
| AOM efficiency | first-order power / input power per pass | tens of percent per pass; η² double-pass | reoptimize the Bragg angle and RF power; focus in the crystal |
| Double-pass return | does the returning beam walk as the RF changes? | no walk when the cat’s-eye is right | adjust the lens and mirror position |
| Recombination | overlap in the cell (two beam positions and angles) | overlapping to a small fraction of the beam size, parallel to well below a milliradian | walk the beams with the last two mirrors in each arm |
| Polarizations in the cell | circular purity with a rotating analyser | opposite circular states for probe and control | trim the plate angles; check mirror reflections |
| Field in the shield | fluxgate reading vs coil current | linear; residual far below the bias | degauss 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
- Jones calculus, waveplates and Gaussian beams: Jones 1941, Kogelnik & Li 1966, Saleh & Teich, Hecht, Siegman 1986.
- Double-pass AOM: Donley et al. 2005. General AOM physics: Saleh & Teich, Siegman 1986.
- Saturated absorption and diode-laser locking: Preston 1996, MacAdam et al. 1992, Wieman & Hollberg 1991, Black 2001, Drever et al. 1983, Demtröder.
- Vapour-cell EIT practice (cells, buffer gas, shielding, alignment): Finkelstein et al. 2023; optical pumping and optical magnetometry (atomic ground-state coherence sensitive to magnetic fields): HAPPER 1972, Budker & Romalis 2007.
- Data: Steck, Rb-87 data; constants: CODATA 2018.
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
- First quantum mechanics. Griffiths & Schroeter; Feynman et al. (free online); Sakurai & Napolitano (more advanced). P3, P4, L2.
- Quantum optics, gentle to rigorous. Fox 2006; Gerry & Knight; Garrison & Chiao 2008; Loudon; Scully & Zubairy 1997; Walls & Milburn; Meystre & Sargent; Agarwal 2013. P5, L1, L4, L6, L7, L11.
- Atoms and light. Foot 2005; Metcalf & van der Straten; Allen & Eberly 1975; Haroche & Raimond 2006. L3, L4, L5, L12.
- Optics, lasers and photonics. Hecht; Saleh & Teich; Siegman 1986; Boyd; Demtröder. L6, L13.
- Slow light. Milonni 2005. L8.
- Quantum information. Nielsen & Chuang 2000; Kok & Lovett 2010. P2, L2, L10, L11.
- Free resources. Steck, Quantum and Atom Optics (lecture notes with detailed derivations); Steck, Rb-87 data (data); CODATA 2018; NIST ASD.
Original papers (history)
- Quantization and the photon: Planck 1901, Einstein 1905, Bohr 1913, Einstein 1917, Compton 1923.
- Quantum mechanics and field quantization: Heisenberg 1925, Schrödinger 1926, Born 1926, Dirac 1927.
- Two-level dynamics: Rabi 1937, Bloch 1946, Feynman et al. 1957, Jaynes & Cummings 1963.
- Lasers and coherence: Gordon et al. 1954, Schawlow & Townes 1958, MAIMAN 1960, BROWN & TWISS 1956, Glauber 1963, Glauber 1963, Kimble et al. 1977.
- Coherent population trapping and EIT: Alzetta et al. 1976, Boller et al. 1991, Harris 1997, Fleischhauer et al. 2005, Arimondo 1996, Anisimov et al. 2011.
Slow light, storage and memories
- Hau et al. 1999, Kash et al. 1999, Budker et al. 1999: slow light.
- Fleischhauer & Lukin 2000, Fleischhauer & Lukin 2002, Lukin 2003: dark-state polaritons and memories.
- Phillips et al. 2001, Liu et al. 2001, Chanelière et al. 2005, Eisaman et al. 2005, Gorshkov et al. 2007: storage and retrieval.
- Reviews: Lvovsky et al. 2009, Hammerer et al. 2010, Novikova et al. 2011, Bussières et al. 2013, Heshami et al. 2016, Ma et al. 2017, Wei et al. 2022.
- Quantum networks: Duan et al. 2001, Briegel et al. 1998, Sangouard et al. 2011, Kimble 2008, Gisin & Thew 2007, Bennett & Brassard 2014.
The project’s main reference
- Finkelstein et al. 2023 (open access as Finkelstein et al. (arXiv)). The reference design for Zeeman EIT (Fig. 10). Read Sections II–V in full.
Strong coupling and polaritons
- Hopfield 1958, Weisbuch et al. 1992, Kasprzak et al. 2006, Basov et al. 2020, Törmä & Barnes 2014, Ebbesen 2016, Frisk Kockum et al. 2019, Forn-Díaz et al. 2019, Ma et al. 2018, Nagarajan et al. 2020.
Lab methods
- Jones 1941, Kogelnik & Li 1966, Donley et al. 2005, Preston 1996, MacAdam et al. 1992, Wieman & Hollberg 1991, Black 2001, Drever et al. 1983, Dicke 1953, HAPPER 1972, Hahn 1950.
- Safety: IEC 60825-1; ANSI Z136.1.
Collected links collected
- Wikipedia: Electromagnetically induced transparency (quick orientation only).
- Video (YouTube) ykWIOBJZ0OE · Video (YouTube) OVIwu10N5lM: lecture or demonstration videos (titles not confirmed).
- “Photonic Quantum Technologies: Science and Applications” (a book named in an earlier collected link; publisher details not verified, so prefer your library’s catalogue record).
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.
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.
| Quantity | Value |
|---|---|
| Speed of light c | 299 792 458 m/s (exact) |
| Planck constant h | 6.626 070 15 × 10⁻³⁴ J·s (exact); 4.135 667 696… × 10⁻¹⁵ eV·s |
| Reduced Planck constant ħ | 1.054 571 817… × 10⁻³⁴ J·s |
| Elementary charge e | 1.602 176 634 × 10⁻¹⁹ C (exact) |
| Boltzmann constant kB | 1.380 649 × 10⁻²³ J/K (exact) |
| Vacuum permittivity ε₀ | 8.854 187 817… × 10⁻¹² F/m |
| Bohr magneton µB | 9.274 010 078 3(28) × 10⁻²⁴ J/T; µB/h = 1.399 624 493 61(42) MHz/G |
| Atomic mass unit u | 1.660 539 066 60(50) × 10⁻²⁷ kg |
| ⁸⁷Rb mass | 86.909 180 520(15) u |
| ⁸⁷Rb nuclear spin; abundance | I = 3/2; 27.83(2) % |
| D1 line (5S₁/₂ → 5P₁/₂): vacuum wavelength | 794.978 851 156(23) nm (794.766 477 6 nm in air) |
| D1 frequency; photon energy | 377.107 463 380(11) THz; 1.559 591 154 eV |
| D1 lifetime τ; decay rate Γ | 27.679(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 velocity | 5.7754 mm/s |
| D2 line (5S₁/₂ → 5P₃/₂): wavelength; Γ/2π | 780.241 209 686(13) nm; 6.0666(18) MHz |
| Ground hyperfine splitting | 6.834 682 610 904 290(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 shift | 2π × 575.15 Hz/G² |
| Vapour pressure at 25 °C | 3.92(20) × 10⁻⁷ Torr |
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.
| Where | What was found | What was done |
|---|---|---|
| L3, L4, interactive lab, Appendix B | Γ/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, L3 | The 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. |
| L12 | A 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, L5 | Leftover references to “Method B” (removed from the guide). | Rewritten as a general hyperfine (clock-state) Λ scheme. |
| Reading list | Some 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 examples | Re-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 checked | Illustrative 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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