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Optional unit · institution-dependent · Interactive lesson

The Born-Markov master equation for an atom in vacuum

Weisskopf and Wigner followed one amplitude out of one pure state. Here the field is traced out instead, so the atom gets an equation of motion for its entire density matrix, superpositions and mixtures included. The real work is seeing which three approximations buy that equation, and what each of them costs.

UAQM-14.03 · Lesson 3 of 9 in this unit. Position is not a completion score.
Starting model: The Born-Markov master equation for an atom in vacuumLeft: the excited population ρₑₑ (solid) and the coherence |ρ_eg| (dashed) against Γt, for ρₑₑ(0) = 0.75 and |ρ_eg(0)| set to 1.0 times the largest that population allows. Right: the Bloch vector in the frame rotating at ω₀′, sliding along a parabola into |g⟩. At Γt = 0.7, ρₑₑ = 0.372 and |ρ_eg| = 0.305.solid ρₑₑ, dashed |ρeg|Γt = 0.7 |r| = 0.6610Γt = 5|e⟩|g⟩
Start with a picture. Change the model in the lab below.

Optional unit · institution-dependent. Units 14 and 15 are the course’s optional extension into open systems and quantum gases. Unit 14 builds on radiation and decay; Unit 15 builds on second quantisation. Keep the fifteen-unit numbering and follow your institution’s required syllabus. Optional work is not a required completion gate.

1

Build the model

Trace out the field, name three approximations, and the whole density matrix decays.

The key idea

The Born-Markov master equation is the closed equation of motion for an atom's density matrix once the vacuum field has been traced out: unitary motion at the observed frequency, plus a dissipator that empties |e⟩ into |g⟩ at the rate Γ.

Example. Hydrogen 2p → 1s has Γ = 6.27 × 10⁸ s⁻¹. Start in (|e⟩ + |g⟩)/√2; at t = 1/Γ = 1.60 ns the master equation gives ρₑₑ = 0.5/e = 0.184 and |ρeg| = 0.5/√e = 0.303, a mixed state that no wavefunction describes.

The complete physical model and assumptions

An atom is closed only together with the radiation field, whose infinitely many modes nobody will ever measure. The master equation is what is left once they are traced out. Iterate the exact von Neumann equation for atom plus field once in the interaction picture and trace over the field: the first-order term dies because the vacuum has ⟨E⟩ = 0, and the second-order term sees the field only through its vacuum correlation function. Three approximations then turn an exact but useless memory integral into a local equation. Born: the field the atom meets stays in its vacuum, uncorrelated with the atom, which is fair for a reservoir whose photons leave at c and never come back. Markov: the vacuum correlations die within about 1/ω₀, some 10⁷ times faster than the atom decays, so the slowly varying interaction-picture state comes outside the integral. Secular: terms turning at 2ω₀ average away over a decay time. The result, derived, is dρ/dt = −(i/ħ)[H′, ρ] + Γ(σ₋ρσ₊ − ½(σ₊σ₋, ρ)), whose Γ is Unit 12's A coefficient and whose H′ carries the principal-value shift. It reproduces Weisskopf-Wigner for |e⟩ and extends it to every ρ. It stops where its approximations stop: before about 1/ω₀, where decay starts quadratically; in a cavity whose coupling outruns its losses, where the photon returns; and in any reservoir whose spectrum is structured on the scale of Γ.

1Iterate the von Neumann equation and trace out the field

Units are SI throughout; nothing here is relativistic, and where the course's covariant forms are recalled the metric is diag(1, −1, −1, −1). The model is Unit 11's: a two-level atom at the origin, HA = ħω₀σ₊σ₋, coupled to every mode k, a wavevector with one of its two polarisations, of a box of volume L³ through HI = −d⋅E(0), counter-rotating terms kept. In the interaction picture the joint state obeys dρ̃ₜₒₜ/dt = −(i/ħ)[HI(t), ρ̃ₜₒₜ(t)]. Integrate from 0 to t, substitute back, and trace over the field: dρ̃/dt = −(i/ħ)TrF[HI(t), ρₜₒₜ(0)] − (1/ħ²)∫₀t TrF[HI(t), [HI(t′), ρ̃ₜₒₜ(t′)]] dt′. That is still exact. If the atom starts uncorrelated with an empty field, ρₜₒₜ(0) = ρ(0) ⊗ |0⟩⟨0|, the first term carries ⟨0|E|0⟩ = 0 and vanishes. The field then enters only through ⟨0|E(t)E(t′)|0⟩ = Σₖ (ħωₖ/(2ε₀L³)) εₖεₖ e(−iωₖ(t − t′)): the only ordering to survive is a photon created at t′ and destroyed at t.

2Born: a reservoir that does not remember the atom

The equation is not closed yet, because ρ̃ₜₒₜ(t′) is the joint state at earlier times. The Born approximation replaces it by ρ̃(t′) ⊗ |0⟩⟨0|. That does not claim that no photon is emitted. It claims that whatever the atom emitted has gone: a photon created at the atom is a wave packet moving off at c, 30 cm away after 1 ns, and the modes the atom couples to later are, to the order kept, still empty. The factorised equation is already second order in d, and the atom-field correlations it drops change it only at higher order, by a relative amount of order Γ/ω₀. The approximation fails when the reservoir is small enough to remember. A single high-finesse cavity mode hands its photon back to the atom, and that is Unit 11's Jaynes-Cummings problem, a reversible exchange, not a decay.

3Markov: forget faster than the atom changes

Put τ = t − t′. After the trace, the kernel multiplying σ₊σ₋ρ̃ is Σₖ |gₖ|² e(i(ω₀ − ωₖ)τ). Its spectrum, |gₖ|² times the mode density, rises as ω³ and is smooth through ω₀, so the kernel is a spike no more than about 1/ω₀ wide, as topic 12.05 found. Now the interaction picture matters: ρ̃ has had the fast phase e(−iω₀t) taken out and changes only at the rate Γ, so across the spike ρ̃(t − τ) → ρ̃(t) with a relative error of order Γ/ω₀. For hydrogen's 2p level 1/ω₀ = 6.45 × 10⁻¹⁷ s and 1/Γ = 1.60 ns, a ratio of 4.0 × 10⁻⁸. For t ≫ 1/ω₀ the upper limit goes to infinity, and ∫₀^∞ e(ixτ) dτ = πδ(x) + iP(1/x), quoted from topic 12.06, splits the kernel into Γ/2 plus iδₑ. The same step in the Schrödinger picture would be wrong: there ρeg turns over in 1/ω₀, exactly the width of the spike.

4Secular: drop what turns at 2ω₀

Put d(t) = deg σ₊ e(iω₀t) + deg* σ₋ e(−iω₀t) into the double commutator. Products such as σ₊σ₊ vanish for two levels, but the sandwiched terms do not. σ₋ρ̃σ₊ comes with e(iω₀τ) alone and is slow; σ₋ρ̃σ₋ and σ₊ρ̃σ₊ carry e(∓2iω₀t). Over one hydrogen 2p lifetime those turn about 8 × 10⁶ times, and their integrated effect is of relative size Γ/(2ω₀) = 2.0 × 10⁻⁸, so the secular approximation drops them. The counter-rotating part of the coupling survives only as a shift of |g⟩. Transform back with HA and the formula card's equation follows, derived. Two checks cost a line each. Trace: d(ρₑₑ + ρgg)/dt = −Γρₑₑ + Γρₑₑ = 0. Dimensions: ω₀³|deg|²/(ε₀ħc³) is s⁻³ (C m)² over (C² J⁻¹ m⁻¹)(J s)(m³ s⁻³), which is s⁻¹, as a rate must be. Keep the 2ω₀ terms and the equation is of Redfield type, which need not keep ρ positive.

5Rate and shift: Unit 12's values, Unit 13's divergence

The real part of the kernel gives Γ = 2π Σₖ |gₖ|² δ(ωₖ − ω₀), topic 12.02's golden-rule sum. Turn Σₖ into (L³/8π³)∫d³k, sum |deg⋅ε|² over the two polarisations and average it over all directions to get (2/3)|deg|², set k = ω₀/c, and L³ cancels: Γ = ω₀³|deg|²/(3πε₀ħc³), the A coefficient. For hydrogen 2p → 1s, ħω₀ = (3/4)(13.606 eV) = 10.204 eV and the integral between the 1s and 2p orbitals gives |⟨g|r|e⟩|² = (2¹⁵/3¹⁰)a₀² = 0.555 a₀², so Γ = 6.27 × 10⁸ s⁻¹ and 1/Γ = 1.60 ns, the measured lifetime. The imaginary parts give δₑ = PΣₖ|gₖ|²/(ω₀ − ωₖ) and, from the counter-rotating terms, δg = −PΣₖ|gₖ|²/(ω₀ + ωₖ). Both grow without bound with the mode cutoff, as Unit 13 found; that part is absorbed into the observed ω₀′. The finite remainder for a real atom needs every level, not two: Bethe's logarithm, cut off near mc², gives 1040 MHz for the splitting of hydrogen's 2s₁/₂ and 2p₁/₂ levels against the measured 1058 MHz, an estimate quoted from Unit 13 and not the full QED value.

6Solve it for any initial state

In the basis |e⟩, |g⟩ the master equation is three linear equations: dρₑₑ/dt = −Γρₑₑ, dρgg/dt = +Γρₑₑ and dρeg/dt = −(Γ/2 + iω₀′)ρeg. Population flows from |e⟩ to |g⟩ at Γ, while the coherence, reached only by the anticommutator at half strength, decays at Γ/2: T₁ = 1/Γ and T₂ = 2/Γ, the radiative limit of topic 14.02. Nothing in the solution asked whether ρ(0) was pure. The limits check out. Γ → 0 returns the von Neumann equation. ρ(0) = |e⟩⟨e| gives ρₑₑ = e(−Γt), the |cₑ|² of topic 12.06. Every initial state ends in |g⟩⟨g|, the only steady state, as it must in a vacuum at zero temperature. Positivity survives too: ρₑₑρgg − |ρeg|² = e(−Γt)[ρₑₑ(0)(1 − ρₑₑ(t)) − |ρeg(0)|²], which is never below its starting value times e(−Γt). A pure start other than |g⟩ does not stay pure: the Bloch vector leaves the sphere and comes back to it only at |g⟩.

2

Key equations

Read the units, assumptions and limits before substituting.

Second order, with the Born factorisation

dρ̃/dt = −(1/ħ²) ∫₀t TrF[HI(t), [HI(t′), ρ̃(t′) ⊗ |0⟩⟨0|]] dt′

Derived: the iterated von Neumann equation is exact, and only ρ̃ₜₒₜ(t′) → ρ̃(t′) ⊗ |0⟩⟨0| is assumed. It still has memory: every earlier ρ̃(t′) enters.

ρ̃: atom, interaction picture; HI(t) = −d(t)⋅E(t, 0) in J; TrF traces the field; ⟨0|E|0⟩ = 0 kills first order

Markov step: the one-sided kernel

∫₀^∞ Σₖ |gₖ|² e(i(ω₀ − ωₖ)τ) dτ = Γ/2 + iδₑ

A rate from the real part and a shift from the imaginary part of one integral. Allowed because the kernel dies in about 1/ω₀ while ρ̃ moves only at the rate Γ.

ħgₖ = √(ħωₖ/(2ε₀L³)) deg⋅εₖ, gₖ in s⁻¹; τ = t − t′ in s; δₑ = P Σₖ |gₖ|²/(ω₀ − ωₖ) in s⁻¹

The master equation

dρ/dt = −(i/ħ)[H′, ρ] + Γ(σ₋ρσ₊ − ½(σ₊σ₋, ρ))

Derived, once terms turning at 2ω₀ are dropped. Unitary motion at the shifted frequency, a term σ₋ρσ₊ that feeds |g⟩, and an anticommutator that drains |e⟩.

Schrödinger picture; σ₋ = |g⟩⟨e|, σ₊ = |e⟩⟨g|; H′ = ħω₀′σ₊σ₋ with ω₀′ = ω₀ + δₑ − δg; Γ in s⁻¹

Its rate is Unit 12's A coefficient

Γ = 2π Σₖ |gₖ|² δ(ωₖ − ω₀) = ω₀³|deg|²/(3πε₀ħc³)

The real part of the kernel is topic 12.02's golden-rule sum, and Unit 11's mode density evaluates it, so the master equation adds no free parameter.

deg = ⟨e|d|g⟩ in C m, ω₀ in rad s⁻¹; hydrogen 2p → 1s: Γ = 6.27 × 10⁸ s⁻¹, so 1/Γ = 1.60 ns, as measured

Populations: exponential from any start

ρₑₑ(t) = ρₑₑ(0) e(−Γt)

Derived, for mixtures and superpositions alike. For ρ(0) = |e⟩⟨e| it is the |cₑ(t)|² of Weisskopf-Wigner: the one-excitation limit agrees.

ρₑₑ = ⟨e|ρ|e⟩, dimensionless; ρgg = 1 − ρₑₑ because the trace is conserved; T₁ = 1/Γ

Coherence: half the rate

ρeg(t) = ρeg(0) e(−(Γ/2 + iω₀′)t)

Derived: only the anticommutator reaches ρeg, at half strength. This is the radiative limit T₂ = 2T₁, and the line it Fourier-transforms into has full width Γ.

ρeg = ⟨e|ρ|g⟩; T₂ = 2/Γ = 2T₁. Sodium's measured 16.25 ns lifetime gives T₂ = 32.5 ns
3

Interactive lab

Predict first. Explore the model. Compare the result.

Explore the model

0.75
0 to 1; steps of 0.05.
1.0
0 to 1; steps of 0.1.
0.7
0 to 5; steps of 0.1.

Try this. Set f = 1 and step Γt: the arrow drops inside the circle, is shortest at Γt = 0.7, near ln 2, and reaches the rim again only at |g⟩. At Γt = 2 the dashed curve is at e⁻¹ of its start, the solid one at e⁻². Set f = 0: ρₑₑ decays exactly as before.

Live results

EXCITED POPULATION ρₑₑ
0.372
COHERENCE |ρeg|
0.305
PURITY Tr ρ²
0.719
TIME FOR HYDROGEN 2p
1.12 ns

Results follow this lesson’s model and assumptions. Displayed values are rounded.

Interactive Advanced Quantum Mechanics modelLeft: the excited population ρₑₑ (solid) and the coherence |ρ_eg| (dashed) against Γt, for ρₑₑ(0) = 0.75 and |ρ_eg(0)| set to 1.0 times the largest that population allows. Right: the Bloch vector in the frame rotating at ω₀′, sliding along a parabola into |g⟩. At Γt = 0.7, ρₑₑ = 0.372 and |ρ_eg| = 0.305.solid ρₑₑ, dashed |ρeg|Γt = 0.7 |r| = 0.6610Γt = 5|e⟩|g⟩
Left: the excited population ρₑₑ (solid) and the coherence |ρeg| (dashed) against Γt, for ρₑₑ(0) = 0.75 and |ρeg(0)| set to 1.0 times the largest that population allows. Right: the Bloch vector in the frame rotating at ω₀′, sliding along a parabola into |g⟩. At Γt = 0.7, ρₑₑ = 0.372 and |ρeg| = 0.305.

Predict → change one variable → check

Plan a change before running it. Every other input stays at the saved baseline.

Saved baseline. Initial excited population ρₑₑ(0): 0.75; Coherence, fraction of its maximum: 1.0; Time Γt: 0.7

Baseline 0.75; choose 0 to 1, in steps of 0.05.
4. Compared with the saved baseline, this result will…

This experiment is kept only while this page is open. It does not change saved course progress.

4

Catch the common trap

A tempting shortcut for a superposition α|g⟩ + β|e⟩ is to borrow Weisskopf-Wigner: let β fall as e(−Γt/2), leave α alone, and renormalise, giving a pure state that drifts towards |g⟩. It is wrong, and the numbers show it. Start from (|e⟩ + |g⟩)/√2 and wait until Γt = ln 2. The shortcut gives ρₑₑ = 1/3 with purity 1; the master equation gives ρₑₑ = 1/4 with purity Tr ρ² = 7/8. The shortcut forgets the photon. With probability 1/4 one has already been emitted and the atom is in |g⟩; with probability 3/4 none has, and only then is the atom in the renormalised state, so ρₑₑ = (3/4)(1/3) = 1/4. Because the emitted photon is entangled with the atom, the atom alone is mixed. The renormalised state is the no-jump state of topic 14.08's trajectories, not the ensemble.

5

Practice & worked examples

3 authored examples. Make an attempt, then reveal the reasoning one step at a time.

EasyExample 1

Treat sodium's 3p → 3s line as a two-level atom in the vacuum, with the measured lifetime 16.25 ns. The atom is prepared in a mixed state with ρₑₑ(0) = 0.60 and a real coherence ρeg(0) = 0.30. Find ρₑₑ, ρgg and |ρeg| at t = 20.0 ns, and check that the result is still a density matrix.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 4 steps revealed.

MediumExample 2

Rubidium-87's D2 line at λ = 780.24 nm has a measured upper-level lifetime of 26.24 ns, and its cycling transition behaves as a two-level atom. Use the master equation's rate to infer |deg| in units of ea₀, then give T₂, the natural full width Γ/2π, and the Markov ratio Γ/ω₀.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 5 steps revealed.

HardExample 3

A hydrogen atom on its 2p → 1s line (Γ = 6.27 × 10⁸ s⁻¹) is prepared in the pure state √p|e⟩ + √(1 − p)|g⟩. Show from the master equation that its state is most mixed at a time that does not depend on p. For p = 0.75, find that time, the Bloch-vector length, the purity Tr ρ², and the atom's von Neumann entropy in bits.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 5 steps revealed.

6

Quick check

Select an answer and explain it before checking.

A two-level atom in the vacuum field starts in the pure state (|e⟩ + |g⟩)/√2. According to the Born-Markov master equation, what are ρₑₑ and |ρeg| at t = 2/Γ?
7

Review & continue

The Born-Markov master equation is the closed equation of motion for an atom's density matrix once the vacuum field has been traced out: unitary motion at the observed frequency, plus a dissipator that empties |e⟩ into |g⟩ at the rate Γ.

  • Explain the relationship without looking at the equation.
  • Check a sign, a unit and a model assumption in your working.
  • Return to the lab or worked example if a step is still unclear.

Extra challenging questions

Connect several ideas, explore supplied data, and compare your reasoning with a worked solution.