Photon Blockade

Photon blockade takes the anharmonic energy ladder of the Jaynes–Cummings model — one two-level atom strongly coupled to one quantized cavity mode, the workhorse Hamiltonian of cavity quantum electrodynamics — and turns it into a valve for single photons. It is the optical cousin of the Coulomb blockade of mesoscopic electronics: just as the charging energy of a small island forbids a second electron from tunnelling on while the first sits there, a strong optical nonlinearity forbids a second photon from joining a mode that already holds one. The nonlinearity comes from a single quantum emitter — an atom, quantum dot, or superconducting qubit — whose coupling makes the combined light–matter levels unequally spaced. Because each transition frequency depends on how many quanta are present, a drive tuned to the empty-to-one-photon transition is off-resonant for the one-to-two-photon transition, and the second photon is turned away. The blockade is dynamical, not static: the first photon must be present to shift the resonance, so it is the light itself that gates the light. That is why the emitted stream is antibunched — after a photon leaks out the cavity resets to vacuum and admits another single photon, one at a time, like a turnstile. The consequence is nonclassical light with a second-order coherence g(2)(0)g^{(2)}(0) far below unity, sub-Poissonian statistics, and a negative Mandel QQ — certified by a Hanbury Brown–Twiss measurement, recalled here by name and developed in the articles that follow.

Key takeaways
  • Photon blockade is a strong-coupling cavity-QED effect: absorbing one photon shifts the next transition out of resonance, so the second photon is blocked from entering the mode.
  • It rides on the anharmonic Jaynes–Cummings ladder, whose nn-th manifold splits by 2gn2g\sqrt{n} rather than into evenly spaced rungs — the n\sqrt{n} nonlinearity is the essential ingredient.
  • Conventional blockade needs strong coupling g≫κ,γg \gg \kappa,\gamma, so the vacuum Rabi splitting beats the linewidths and the two-photon rung is resolved.
  • The signature is strong antibunching, g(2)(0)≪1g^{(2)}(0) \ll 1, converting a weak coherent drive into a stream of well-separated single photons — a photon turnstile — with Mandel Q<0Q<0.
  • A second flavour, unconventional (interference) blockade, cancels the two-photon amplitude by interference and works even with weak nonlinearity, but gives a narrow, tuning-sensitive dip; blockade underpins single-photon sources and single-photon nonlinear optics.
  • Key idea: The Jaynes–Cummings ladder is anharmonic with rung splittings ∝n\propto \sqrt{n}; when the anharmonicity of order gg exceeds the linewidths κ,γ\kappa,\gamma, a drive tuned to the one-photon transition is detuned from the two-photon transition, so the presence of one photon blocks the second — yielding g(2)(0)≪1g^{(2)}(0)\ll 1.

Where this lives today

The blockade has migrated from single trapped atoms to solid-state and superconducting platforms, where it does engineering work. Semiconductor quantum dots in micropillar and photonic-crystal cavities behave as artificial atoms with large dipole moments and reach strong coupling on a chip; driven near blockade, the best emit single photons with g(2)(0)g^{(2)}(0) below 0.010.01 and near-unity indistinguishability — the front-runner for the deterministic single-photon sources photonic quantum computers need in bulk. In circuit QED, a superconducting qubit coupled to a microwave resonator reaches g/2πg/2\pi of tens to hundreds of MHz with far smaller loss, making blockade robust and a primitive for microwave single-photon sources and photon detectors on superconducting processors. A different modern route drops the cavity entirely. In Rydberg-mediated schemes, photons stored as slow-light polaritons in an ultracold gas inherit the long-range interaction of Rydberg atoms, so one stored photon blockades a whole micron-scale volume against a second — the Rydberg blockade imported into optics. These experiments have produced strongly interacting, antibunched photons and even photon–photon bound states, extending "one photon blocks the next" from a single mode to a propagating field.

The physical picture

Picture a staircase whose steps are labelled by photon number. For a bare, linear cavity the steps are evenly spaced, so a resonant drive climbs every rung and the field grows into a coherent state. Coupling the cavity to a single atom warps the staircase: because the vacuum Rabi splitting of the nn-th manifold scales as n\sqrt{n}, the second step is a different height than the first. A drive tuned to the first step then misses the second, and the cavity refuses to hold two photons. The first figure makes this explicit.

Figure
The Jaynes–Cummings ladder is anharmonic: the n-th manifold splits by 2g√n. A drive at ω_c − g fills the first rung, but the second sits 0.586 g too high — for one strongly coupled atom 2g/2π ≈ 68 MHz makes the gap ≈ 19.9 MHz, far above the linewidths, so the second photon is blocked
A √n ladder, not a uniform one — the second rung is out of reach energy |0⟩ ħω_c |1,+⟩ |1,−⟩ 2g 2ħω_c |2,+⟩ |2,−⟩ 2√2 g drive ω_c − g where an equal step lands gap 0.586 g → blocked splitting grows as √n → the second rung is detuned from the drive

The blockade is dynamical: the first photon must be present to shift the resonance, so the light gates the light. And it survives only in strong coupling — the anharmonic shift is of order gg, but the rungs are resolvable only if gg beats the blur of loss κ\kappa and decay γ\gamma; in weak coupling the ladder smears into one line and blockade fails. The second figure shows the resolved doublet in the cavity transmission of a strongly coupled atom.

Figure
Vacuum Rabi doublet in cavity transmission: instead of one peak at ω_c the spectrum splits into polariton peaks at ω_c ± g, here ±34 MHz for a 68 MHz splitting. Parking the weak drive on the lower peak at ω_c − g admits one photon at a time, so the emitted light is antibunched, g⁽²⁾(0) ≪ 1
One peak splits into two — the resolved vacuum Rabi doublet at ω_c ± g 1.0 0.5 0 empty cavity ω_c − g ω_c + g −34 0 +34 probe detuning (ω − ω_c)/2π (MHz) 2g/2π = 68 MHz weak drive here → g⁽²⁾(0) ≪ 1 transmission

The core equations

The whole subject is carried by one model: a single two-level emitter exchanging quanta with one cavity mode. In the rotating-wave approximation this is the Jaynes–Cummings Hamiltonian, from which every result follows.

H^JC=ℏωc a^†a^+12ℏωa σ^z+ℏg (a^†σ^−+a^ σ^+)(1)\hat H_{\mathrm{JC}} = \hbar\omega_c\,\hat a^\dagger\hat a + \tfrac{1}{2}\hbar\omega_a\,\hat\sigma_z + \hbar g\,(\hat a^\dagger\hat\sigma_- + \hat a\,\hat\sigma_+) \qquad (1)

where: a^,a^†\hat a,\hat a^\dagger — cavity photon operators; σ^z,σ^±\hat\sigma_z,\hat\sigma_\pm — atomic inversion and raising/lowering operators; ωc,ωa\omega_c,\omega_a — cavity and atomic frequencies; gg — single-photon (vacuum Rabi) coupling. The third term swaps a photon for an atomic excitation and is the only nonlinear term. Because H^JC\hat H_{\mathrm{JC}} conserves the total excitation number it splits into independent 2×22\times2 blocks, one per manifold, each diagonalizing into a doublet of dressed states (polaritons) whose energies are the backbone of the blockade.

En,±=ℏωc n±ℏ2δ2+4g2n,δ=ωa−ωc(2)E_{n,\pm} = \hbar\omega_c\, n \pm \tfrac{\hbar}{2}\sqrt{\delta^2 + 4g^2 n},\qquad \delta=\omega_a-\omega_c \qquad (2)

where: n≥1n\ge 1 — total excitation number; En,±E_{n,\pm} — upper/lower dressed states of the nn-th manifold; δ\delta — atom–cavity detuning. On resonance (δ=0\delta=0) the manifold sits at ℏωcn±ℏgn\hbar\omega_c n \pm \hbar g\sqrt{n}, so the splitting 2ℏgn2\hbar g\sqrt{n} grows as n\sqrt{n} — the anharmonicity. The lowest manifold (n=1n=1) is what a linear transmission scan probes, and its splitting is the fingerprint of strong coupling.

E1,±=ℏωc±ℏg(δ=0)(3)E_{1,\pm} = \hbar\omega_c \pm \hbar g \qquad (\delta=0) \qquad (3)

where: ±g\pm g — displacement of the two lowest polaritons from the bare cavity frequency ωc\omega_c. A single empty-cavity resonance becomes a doublet split by 2g2g; resolving it (Figure 2) is what strong coupling means. The blockade lives in the mismatch between the first and second rungs of the lower branch: comparing the one- and two-photon transition energies gives the anharmonicity.

A≡∣ (E2,−−E1,−)−(E1,−−E0) ∣=ℏg (2−2)≈0.586 ℏg(4)A \equiv \bigl|\,(E_{2,-}-E_{1,-}) - (E_{1,-}-E_0)\,\bigr| = \hbar g\,(2-\sqrt{2}) \approx 0.586\,\hbar g \qquad (4)

where: AA — detuning between the one- and two-photon transitions on the lower branch; E0=0E_0=0 — ground-state energy. Blockade requires AA to exceed the linewidths ℏκ,ℏγ\hbar\kappa,\hbar\gamma; then the one-photon drive leaves the two-photon rung dark. Whether blockade is working is read off the emitted light, not the levels — the normalized zero-delay second-order coherence is the standard metric, counting photon pairs relative to a coherent reference.

g(2)(0)=⟨a^†a^†a^a^⟩⟨a^†a^⟩2=⟨n^(n^−1)⟩⟨n^⟩2(5)g^{(2)}(0) = \frac{\langle \hat a^\dagger\hat a^\dagger\hat a\hat a\rangle}{\langle \hat a^\dagger\hat a\rangle^2} = \frac{\langle \hat n(\hat n-1)\rangle}{\langle \hat n\rangle^2} \qquad (5)

where: g(2)(0)g^{(2)}(0) — normalized zero-delay intensity correlation; n^=a^†a^\hat n=\hat a^\dagger\hat a. Coherent light gives 11, thermal light 22 (bunched), blockaded light <1<1 (antibunched), ideally →0\to0. For a weakly driven cavity the steady state is mostly vacuum with small one- and two-photon admixtures, and g(2)(0)g^{(2)}(0) reduces to a ratio of amplitudes.

g(2)(0)≈2 ∣c2∣2∣c1∣4,∣ψ⟩≈c0∣0⟩+c1∣1⟩+c2∣2⟩(6)g^{(2)}(0) \approx \frac{2\,|c_2|^2}{|c_1|^4},\qquad |\psi\rangle \approx c_0|0\rangle + c_1|1\rangle + c_2|2\rangle \qquad (6)

where: cnc_n — amplitude of the nn-photon component, with ∣c0∣≈1≫∣c1∣≫∣c2∣|c_0|\approx1\gg|c_1|\gg|c_2|. Blockade drives c2→0c_2\to0 while c1c_1 stays finite, so the ratio collapses; a coherent state has c2=c12/2c_2=c_1^2/\sqrt{2}, reproducing g(2)(0)=1g^{(2)}(0)=1. The same statistics collapse into one signed number, the Mandel parameter, certifying nonclassicality from the number variance.

Q=⟨n^⟩(g(2)(0)−1)=⟨(Δn^)2⟩−⟨n^⟩⟨n^⟩(7)Q = \langle\hat n\rangle\bigl(g^{(2)}(0)-1\bigr) = \frac{\langle(\Delta\hat n)^2\rangle - \langle\hat n\rangle}{\langle\hat n\rangle} \qquad (7)

where: QQ — Mandel parameter, negative for sub-Poissonian (nonclassical) light; ⟨(Δn^)2⟩\langle(\Delta\hat n)^2\rangle — photon-number variance. Q<0Q<0 means a distribution narrower than Poissonian, which no classical field can produce; blockade always gives Q<0Q<0. Blockade only exists under drive and dissipation, so the honest description is a driven-dissipative master equation: a coherent drive H^drive=ℏη(a^†e−iωLt+a^ e+iωLt)\hat H_{\rm drive}=\hbar\eta(\hat a^\dagger e^{-i\omega_L t}+\hat a\,e^{+i\omega_L t}) pumps the cavity while two loss channels remove excitation.

ρ^˙=−iℏ[H^,ρ^]+κ D[a^]ρ^+γ D[σ^−]ρ^(8)\dot{\hat\rho} = -\tfrac{i}{\hbar}[\hat H,\hat\rho] + \kappa\,\mathcal{D}[\hat a]\hat\rho + \gamma\,\mathcal{D}[\hat\sigma_-]\hat\rho \qquad (8)

where: D[c^]ρ^=c^ρ^c^†−12{c^†c^,ρ^}\mathcal{D}[\hat c]\hat\rho = \hat c\hat\rho\hat c^\dagger-\tfrac12\{\hat c^\dagger\hat c,\hat\rho\} — Lindblad dissipator; κ\kappa — cavity decay rate; γ\gamma — atomic spontaneous-emission rate; η,ωL\eta,\omega_L — drive amplitude and frequency (ωL=ωc−g\omega_L=\omega_c-g for blockade). Solving for the steady state and evaluating equation (5) is exactly what a numerical study of blockade computes.

Derivation AThe anharmonic ladder and the conventional blockade condition

The goal is to show, from the dressed-state energies alone, that the Jaynes–Cummings ladder is genuinely anharmonic and to pin down when a laser tuned to the lower polariton blockades the second photon. We follow the lower branch, compute the one- and two-photon transition frequencies, and ask when their mismatch survives the linewidths — turning "one photon blocks the next" into g≫κ,γg\gg\kappa,\gamma.

Step 1. On resonance (δ=0\delta=0) equation (2) collapses to En,±=ℏωcn±ℏgnE_{n,\pm}=\hbar\omega_c n \pm \hbar g\sqrt{n}, so the lower states sit at En,−=ℏ(ωcn−gn)E_{n,-}=\hbar(\omega_c n - g\sqrt{n}), with E0=0E_0=0. Why: setting δ=0\delta=0 isolates the coupling effect — every deviation from an even ladder comes from the n\sqrt{n}.

Step 2. The first rung costs ω0→1,−=(E1,−−E0)/ℏ=ωc−g\omega_{0\to1,-}=(E_{1,-}-E_0)/\hbar=\omega_c-g, so a drive at ωL=ωc−g\omega_L=\omega_c-g is resonant with the lower polariton and one photon enters freely. Why: this fixes where we park the laser, so blockade shows up as the failure of the next step.

Step 3. The next rung costs ω1,−→2,−=(2ωc−2 g)−(ωc−g)=ωc−(2−1)g=ωc−0.414 g\omega_{1,-\to2,-}=(2\omega_c-\sqrt{2}\,g)-(\omega_c-g)=\omega_c-(\sqrt2-1)g=\omega_c-0.414\,g. Why: a second photon needs this frequency, which differs from the first because the splitting grew from 2g2g to 22 g2\sqrt2\,g.

Step 4. The two-photon detuning seen by the drive is Δ2=ωL−ω1,−→2,−=(ωc−g)−(ωc−0.414 g)=−0.586 g\Delta_2=\omega_L-\omega_{1,-\to2,-}=(\omega_c-g)-(\omega_c-0.414\,g)=-0.586\,g, matching A=ℏg(2−2)A=\hbar g(2-\sqrt2). Why: the drive is off resonance for the second step by a fixed 0.586 g0.586\,g — that offset does the blocking.

Step 5. The offset blocks only if ∣Δ2∣=0.586 g|\Delta_2|=0.586\,g exceeds the polariton linewidth ∼(κ+γ)/2\sim(\kappa+\gamma)/2 — the strong-coupling condition g≫κ,γg\gg\kappa,\gamma. Why: a level you cannot resolve is one you cannot avoid — in weak coupling the broadened rung overlaps the drive and blockade washes out.

Step 6. With the two-photon manifold unpopulated, c2→0c_2\to0 and equation (6) gives g(2)(0)→0g^{(2)}(0)\to0: strong antibunching, single photons on demand. Why: resolved rungs become suppressed pairs in the emitted light, what an experiment measures.

Go deeper · Derivation B · 1 minUnconventional blockade from destructive interference
Derivation BUnconventional blockade from destructive interference

Conventional blockade demands a large anharmonicity, g≫κ,γg\gg\kappa,\gamma, which is experimentally hard. The goal here is a second, quite different route — unconventional blockade — in which g(2)(0)≪1g^{(2)}(0)\ll1 arises from destructive interference between two excitation pathways to the two-photon state, and works even when the nonlinearity UU is far smaller than the linewidth. We expand a weakly driven Kerr cavity and find the tuning that cancels c2c_2.

Step 1. Model loss with an effective non-Hermitian Hamiltonian H^eff=(Δ−iκ/2)a^†a^+U2a^†a^†a^a^+η(a^†+a^)\hat H_{\rm eff}=(\Delta-i\kappa/2)\hat a^\dagger\hat a+\tfrac{U}{2}\hat a^\dagger\hat a^\dagger\hat a\hat a+\eta(\hat a^\dagger+\hat a), with Δ=ωc−ωL\Delta=\omega_c-\omega_L and a −iκ/2-i\kappa/2 decay per photon. Why: in the weak-drive trajectory picture dissipation is an imaginary energy, so the steady state is the null vector of H^eff\hat H_{\rm eff} — a small linear-algebra problem.

Step 2. Truncate to ∣ψ⟩=c0∣0⟩+c1∣1⟩+c2∣2⟩|\psi\rangle=c_0|0\rangle+c_1|1\rangle+c_2|2\rangle, valid for η≪κ\eta\ll\kappa. Why: blockade only cares about the two-photon amplitude, so states up to ∣2⟩|2\rangle capture everything relevant.

Step 3. Order by order, c1≈−η/(Δ−iκ/2)c_1\approx -\eta/(\Delta-i\kappa/2) and c2≈η2/[(Δ−iκ/2)(2Δ+U−iκ)]c_2\approx \eta^2/[(\Delta-i\kappa/2)(2\Delta+U-i\kappa)] — fed by two contributions, a direct two-photon drive and a sequential 0→1→20\to1\to2 climb. Why: two additive amplitudes are the whole point; two can cancel, one never could.

Step 4. Choose Δ\Delta (and, in coupled-mode versions, an auxiliary mode) so the two contributions are equal and opposite: c2=0c_2=0, and equation (6) gives g(2)(0)→0g^{(2)}(0)\to0 though UU resolved nothing. Why: this is interference, not level repulsion — the two-photon state stays accessible, but the amplitude to reach it cancels.

Step 5. The character differs sharply: the dip is narrow and tuning-sensitive, suppressing only the zero-delay amplitude, so the light is not a clean single-photon stream; for U≫κU\gg\kappa it crosses over to conventional blockade. Why: interference blockade is cheaper to reach but gives lower-purity photons.

Limiting cases

Blockade needs an anharmonicity that beats the linewidths; the useful regimes fall out of the equations above.

CaseResultMeaning
Strong coupling (conventional blockade)g≫κ,  γg \gg \kappa,\; \gammaRabi doublet resolved, anharmonicity ∼g\sim g beats the broadening; drive the lower polariton for g(2)(0)≪1g^{(2)}(0)\ll1. A genuine turnstile.
Weak coupling (no blockade)g≲κ,  γg \lesssim \kappa,\; \gammaRungs merge into one broadened line; two-photon transition overlaps the drive. Nearly linear, g(2)(0)→1g^{(2)}(0)\to1. Blockade lost.
Weak-drive limitη≪g,  κ\eta \ll g,\; \kappaTwo-photon manifold barely populated; g(2)(0)g^{(2)}(0) minimal and Q<0Q<0. Raising η\eta saturates the system and washes out blockade.
Kerr / unconventionalU≲κU \lesssim \kappa, tuned Δ\DeltaWeak nonlinearity; interference of two pathways gives sharp g(2)(0)≪1g^{(2)}(0)\ll1 at one detuning, despite unresolved levels. Narrow-band.
Harmonic / empty cavityg=0, U=0g=0,\ U=0Evenly spaced ladder; a resonant drive climbs every rung, field is coherent, g(2)(0)=1g^{(2)}(0)=1. No blockade.

Worked examples

1 · A real strong-coupling cavity: does it blockade? (confidence builder)

A single caesium atom in a high-finesse cavity has (g,κ,γ)/2π=(34, 4.1, 2.6)(g,\kappa,\gamma)/2\pi=(34,\,4.1,\,2.6) MHz. Find the vacuum Rabi splitting, the blockade anharmonicity, and the cooperativity, and decide whether blockade appears.

Step 1. The vacuum Rabi doublet (equation 3) is split by 2g2g, so 2g/2π=2×34=68 MHz2g/2\pi = 2\times34 = \mathbf{68\ MHz} — the peak-to-peak separation in Figure 2. It dwarfs κ/2π=4.1\kappa/2\pi=4.1 MHz, so the doublet is cleanly resolved: the sign of strong coupling.

Step 2. The blockade offset is the anharmonicity A=ℏg(2−2)A=\hbar g(2-\sqrt2) (equation 4), i.e. A/h=0.5858×34=19.9 MHzA/h=0.5858\times34=\mathbf{19.9\ MHz}. This is how far the drive at ωc−g\omega_c-g misses the two-photon transition, and it exceeds both linewidths (κ/2π=4.1\kappa/2\pi=4.1, γ/2π=2.6\gamma/2\pi=2.6 MHz).

Step 3. The single-atom cooperativity is C=g2/(2κγ)=342/(2×4.1×2.6)=54C=g^2/(2\kappa\gamma)=34^2/(2\times4.1\times2.6)=\mathbf{54}. Since C≫1C\gg1 and gg beats κ,γ\kappa,\gamma individually, the system is deep in strong coupling.

Step 4. The critical photon number n0=γ2/(2g2)=2.62/(2×342)=2.9×10−3n_0=\gamma^2/(2g^2)=2.6^2/(2\times34^2)=\mathbf{2.9\times10^{-3}} is far below one, so a single photon already saturates the nonlinearity. A 68 MHz doublet, a 19.9 MHz anharmonicity beating few-MHz linewidths, and C≈54C\approx54 with n0≪1n_0\ll1: this cavity blockades, and driving the lower polariton gives antibunched output g(2)(0)≪1g^{(2)}(0)\ll1.

2 · From suppressed pairs to g(2)(0)g^{(2)}(0) and Mandel QQ

A weakly driven blockade cavity has mean photon number ⟨n⟩=0.01\langle n\rangle=0.01. Without the nonlinearity it would be coherent (g(2)(0)=1g^{(2)}(0)=1); the blockade suppresses the two-photon amplitude to a fraction f=0.1f=0.1 of its coherent value. Find g(2)(0)g^{(2)}(0) and the Mandel QQ.

Step 1. For weak drive ⟨n⟩≈∣c1∣2=0.01\langle n\rangle\approx|c_1|^2=0.01. A coherent state has c2=c12/2c_2=c_1^2/\sqrt2, giving the reference g(2)(0)=2∣c2∣2/∣c1∣4=1g^{(2)}(0)=2|c_2|^2/|c_1|^4=1 — the baseline we are beating.

Step 2. Blockade rescales c2→f c2cohc_2\to f\,c_2^{\rm coh}, and since g(2)(0)∝∣c2∣2g^{(2)}(0)\propto|c_2|^2 (equation 6) it scales as f2f^2: g(2)(0)=f2×1=0.12=0.01g^{(2)}(0)=f^2\times1=0.1^2=\mathbf{0.01}. Suppressing the amplitude tenfold cuts the pair probability, and g(2)(0)g^{(2)}(0), a hundredfold.

Step 3. The Mandel parameter (equation 7) is Q=⟨n⟩(g(2)(0)−1)=0.01×(0.01−1)=−9.9×10−3Q=\langle n\rangle(g^{(2)}(0)-1)=0.01\times(0.01-1)=\mathbf{-9.9\times10^{-3}}. The negative sign certifies sub-Poissonian light; the small magnitude reflects the tiny mean number, since Q≥−⟨n⟩Q\ge-\langle n\rangle.

Step 4. A hundredfold suppression of pairs is a strong turnstile; the same drive on a linear cavity gives Q=0Q=0. g(2)(0)=0.01g^{(2)}(0)=0.01 and Q=−9.9×10−3Q=-9.9\times10^{-3} — deep antibunching, with Q<0Q<0 the nonclassicality certificate.

Physics of the portrait

Photon blockade is where the abstract Jaynes–Cummings ladder became laboratory reality — and no one did more to force that transition than the physicist who first resolved the vacuum Rabi splitting for a single atom, then watched one atom turn a laser into single photons.

Origins · 1 minH. Jeffrey Kimble and how this was discovered
HJ
H. Jeffrey Kimble
born 1949 · cavity QED, strong coupling, and the first photon-blockade experiment

H. Jeffrey Kimble spent four decades turning the strong-coupling regime of cavity QED from a theorist's idealization into a working platform. In 1992, with Thompson and Rempe, he resolved the vacuum Rabi doublet for a single atom in an optical cavity — the first time the ∣1,±⟩|1,\pm\rangle splitting of equation (3) was seen for one emitter, proving that a lone atom and mode exchange a single quantum coherently before either decays. That doublet is the entry ticket to blockade: without a resolved 2g2g there is no resolved anharmonicity. Photon blockade had been proposed in 1997 by Imamoğlu and co-workers as "strongly interacting photons" in a nonlinear cavity, but it took Kimble's group until 2005 to realize it — Birnbaum and colleagues trapped one caesium atom, drove the lower polariton, and measured g(2)(0)g^{(2)}(0) well below unity, showing that the presence of one photon really does keep the next one out. Kimble also framed the larger program these tools serve — the quantum internet, in which single-photon sources like a blockaded cavity are essential hardware.

History
1963
— Jaynes and Cummings solve the single-atom single-mode model exactly, giving the dressed-state ladder
1992
— Thompson, Rempe and Kimble resolve the vacuum Rabi doublet for one atom in an optical cavity
1997
— Imamoğlu and co-workers propose photon blockade in a strongly nonlinear cavity
2005
— Birnbaum and the Kimble group demonstrate photon blockade with one trapped atom
2010
— Liew and Savona introduce unconventional interference blockade at weak nonlinearity

Going further

Texts. Loudon, The Quantum Theory of Light, 3rd ed., Ch. 6–7 (Jaynes–Cummings, resonance fluorescence, correlations) · Saleh & Teich, Fundamentals of Photonics, 3rd ed., Ch. 13–14 (photon statistics, cavity QED) · Foot, Atomic Physics, Ch. 7–9 (two-level atom, dressed states) · Birnbaum et al., Nature 436, 87 (2005) — photon blockade with one atom in a cavity · Kimble, Physica Scripta T76, 127 (1998) — strong coupling and vacuum Rabi splitting.

Provenance. The dressed-state energies and vacuum Rabi doublet are standard Jaynes–Cummings results (Loudon Ch. 6–7; Foot Ch. 7). A verifier should recompute the 2×22\times2 block diagonalization, confirm g(2−2)=0.5858 gg(2-\sqrt2)=0.5858\,g and 2−1=0.4142 g\sqrt2-1=0.4142\,g, and check g(2)(0)=2∣c2∣2/∣c1∣4g^{(2)}(0)=2|c_2|^2/|c_1|^4 and Q=⟨n⟩(g(2)(0)−1)Q=\langle n\rangle(g^{(2)}(0)-1) (Saleh & Teich Ch. 13). The parameters (g,κ,γ)/2π=(34,4.1,2.6)(g,\kappa,\gamma)/2\pi=(34,4.1,2.6) MHz in Worked Example 1 are the single-atom values of Birnbaum et al., Nature 436, 87 (2005); from them 2g/2π=682g/2\pi=68 MHz, anharmonicity 19.919.9 MHz, C≈54C\approx54, and n0≈2.9×10−3n_0\approx2.9\times10^{-3} follow directly. The interference condition matches the Liew–Savona / Bamba treatments; dissipators follow the standard Lindblad form.

Prerequisites. Fock States and the Photon Number Basis · Coherent States · Photon Statistics and the Mandel Q Parameter · Coherence Functions and the Degree of Coherence · Quantization of the Electromagnetic Field. Leads to. Photon Antibunching · Single-Photon Sources · Hanbury Brown–Twiss Experiment · Squeezed States of Light.

Ask the tutor: Ask me to walk through how the n\sqrt{n} splitting of the dressed states turns into the 0.586 g0.586\,g offset that blocks the second photon, or to compare conventional and unconventional blockade for a cavity you specify.

Why does an empty, linear cavity show no photon blockade?

Because its ladder is perfectly evenly spaced. A bare cavity mode is a harmonic oscillator, so the 0→10\to1 transition has the same frequency as 1→21\to2 and every higher step. A drive tuned to one rung is tuned to all of them, so nothing stops the field from climbing — it builds into a coherent state with g(2)(0)=1g^{(2)}(0)=1. Blockade needs anharmonicity, something that makes the second step a different height than the first. Coupling the cavity to a single emitter supplies exactly this, warping the ladder so the splittings grow as n\sqrt n and the second photon is pushed out of resonance.

What is the difference between the vacuum Rabi splitting and the blockade anharmonicity?

They are related but not equal. The vacuum Rabi splitting is the full separation of the two lowest polaritons, 2g2g, seen as a doublet in a linear transmission scan. The blockade anharmonicity is the mismatch between the one- and two-photon transitions, A=g(2−2)≈0.586 gA=g(2-\sqrt2)\approx0.586\,g, arising because the splitting grows from 2g2g at n=1n=1 to 22 g2\sqrt2\,g at n=2n=2. Resolving the 2g2g doublet tells you that you are in strong coupling; the smaller 0.586 g0.586\,g offset is what actually blocks the second photon, and it is this offset — not the full splitting — that must beat the linewidths.

Is a bare single atom not already a perfect single-photon emitter?

It is antibunched, but it is neither photon blockade nor a good engineered source. A driven two-level atom emits resonance fluorescence one photon at a time with g(2)(0)=0g^{(2)}(0)=0, because it must be re-excited between emissions. But that light radiates into the full 4π4\pi solid angle, so collecting it is hard, and the atom cannot gate a mode of light — there is no cavity level for it to shift. Blockade puts the atom in a cavity so its saturation transfers to the transmitted mode: the single photons then emerge in one direction out of a mirror, with high collection efficiency.

Why does g(2)(0)<1g^{(2)}(0)<1 not by itself prove photon blockade?

Because g(2)(0)g^{(2)}(0) measures photon statistics, not their cause. Antibunching can arise from any single-emitter effect — ordinary resonance fluorescence gives it — so a low value certifies that pairs are suppressed but not why. To claim blockade you must show the suppression comes from the resolved anharmonic ladder (or the interference condition): that the transmission resonances are photon-number selective with the n\sqrt n scaling, and that the antibunching strengthens as g/κg/\kappa grows. There is also a normalization subtlety — g(2)(0)g^{(2)}(0) is insensitive to transmission and detection efficiency, so it says nothing about brightness.

How can unconventional blockade work if the levels are not resolved?

By interference rather than energy. In a weakly driven Kerr cavity the two-photon state is reached by two pathways — a direct two-photon drive and a sequential 0→1→20\to1\to2 climb — each a complex amplitude. Tuning the detuning (and, in coupled-mode versions, an auxiliary mode) makes these equal and opposite, so they cancel and c2c_2 vanishes even though the two-photon level was never displaced. This gives g(2)(0)≪1g^{(2)}(0)\ll1 with only a small nonlinearity U≲κU\lesssim\kappa. The price is a narrow, tuning-sensitive dip, and the light is not a clean single-photon stream — only the zero-delay coincidence is suppressed.

What does the master equation add that the dressed states alone do not?

The dressed-state ladder is a spectrum — it says where the rungs are, not what a driven, leaky cavity does in steady state. Real blockade exists only under continuous drive and dissipation: photons pumped in at rate η\eta, lost at rates κ\kappa and γ\gamma. The master equation (8) balances these, and its steady-state density matrix is what you feed into equation (5) to get the measured number. It also captures what the bare ladder cannot — the linewidths that decide whether the 0.586 g0.586\,g offset is resolved, and the saturation that ruins blockade at strong drive. The levels give the mechanism; the master equation gives the observable.

Before this

Where this leads