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University Quantum Field Theory I · Vacuum Polarisation, Charge Renormalisation and the Running of alpha · 13.4

The imaginary part of vacuum polarisation is pair creation

Here a loop stops being an algebraic correction and becomes something a detector counts. Watch the iε give Π̂₂ an imaginary part above q² = 4m², identify it with the rate of e⁺e⁻ → μ⁺μ⁻, then run the argument backwards, so that measured rates, R(s) for hadrons, can be fed into the photon propagator.

01

Build the model

Connect the measurement to the mechanism.

Π̂₂(q²) is an analytic function, not just a correction factor, and its imaginary part is the most physical thing about it. The Feynman propagators' iε survives in the Feynman-parameter logarithm as m² − x(1 − x)q² − iε. Below q² = 4m², every spacelike q² included, that argument is positive for all x and Π̂₂ is real.

Above it a window of x opens where the argument is negative, the logarithm acquires −iπ, and Im Π̂₂ = −(α/3)β(1 + 2m²/q²), with β the speed of each lepton in the pair's rest frame. Unitarity reads that number as a rate: topic 5.07's optical theorem turns −(4πα/s) Im Π̂₂ into σ(e⁺e⁻ → f f̄), and for a muon loop the result is topic 9.06's tree-level cross-section, mass factor and all. Analyticity then runs the argument backwards. Π̂₂ has no singularity off the cut, so Cauchy's theorem rebuilds the real part from the imaginary part, with one subtraction at q² = 0 that is exactly the definition of α.

The relation outlives the formula behind it: insert a measured R(s) in place of β(3 − β²)/2 and hadrons, which no perturbative loop describes at low energy, enter the photon propagator as data. The one-loop imaginary part itself fails close to threshold, where Coulomb attraction between the slow leptons changes the rate at relative order πα/(2β), and every further channel, a heavier lepton or a hadronic state, opens its own cut with its own threshold and cusp.

Simple definition
The imaginary part of the renormalised photon self-energy Π̂₂(q²) is the piece that exists only above q² = 4m², where a virtual photon is heavy enough to become a real lepton pair; the optical theorem makes it the rate for producing that pair.
Example
At q² = 9m², β = 0.745 and Im Π̂₂ = −2.22 × 10⁻³ for any lepton. For a muon loop that is √s = 317 MeV, and −(4πα/s) Im Π̂₂ = 788 nb, the cross-section σ(e⁺e⁻ → μ⁺μ⁻) there, 91% of the point-like 864 nb.
Imaginary part above thresholdIm Π̂₂(q² + iε) = −(α/3)√(1 − 4m²/q²)(1 + 2m²/q²) for q² above 4m², and 0 below it

Derived from ln(Δ − iε) = ln|Δ| − iπ where Δ is negative. It tends to −α/3 = −2.43 × 10⁻³ far above threshold and vanishes like β at it.

Π̂₂ dimensionless; q² and m² in GeV²; α = 1/137.036; real at every spacelike q²

The window where Δ is negativeΔ(x) = m² − x(1 − x)q² is negative for x between (1 − β)/2 and (1 + β)/2

Derived. Over this window ∫ x(1 − x) dx = β(3 − β²)/12, and −2α times it is Im Π̂₂. The window shuts at threshold, which is why the rate starts from zero.

x the Feynman parameter, 0 to 1; β = √(1 − 4m²/q²), the lepton speed in the pair rest frame, in units of c

Optical theorem for the bubbleσ(e⁺e⁻ → f f̄) = −(4πα/s) Im Π̂₂(f)(s)

Derived from the forward amplitude −e²Π̂₂(s) and Im ℳ = sσ. It reproduces topic 9.06's (4πα²/3s) × β(3 − β²)/2 term by term: checked.

s in GeV²; σ in GeV⁻², times 0.3894 mb GeV² for barns; electrons massless; f a unit-charge lepton

Once-subtracted dispersion relationΠ̂₂(q²) = (q²/π) ∫ ds Im Π̂₂(s)/[s(s − q² − iε)], s from 4m² to ∞

Derived from Cauchy's theorem for Π̂₂(z)/z. Without the subtraction the integral diverges like ∫ds/s, because Im Π̂₂ tends to −α/3.

s and q² in GeV²; the subtraction uses Π̂₂(0) = 0, the definition of α at q² = 0

The slope at q² = 0, from the cutdΠ̂₂/dq² at q² = 0: (1/π) ∫ ds Im Π̂₂(s)/s² = −α/(15πm²)

Derived, and equal to the −αq²/(15πm²) topic 13.02 found by expanding the logarithm: low-q² physics is made by pairs produced near threshold.

m in GeV, slope in GeV⁻²; 46% of the integral comes from √s/m below 3, and 95% from below 10

Hadrons enter through measured R(s)Im Π̂had(s) = −(α/3) R(s), with R(s) = σ(e⁺e⁻ → hadrons)/(4πα²/3s)

Derived by the optical theorem with any final state. In the dispersion relation it makes the hadronic Π̂ an integral over data, with no quark loop needed.

R dimensionless; 4πα²/3s = 86.85 nb ÷ (s in GeV²); free quarks would give R = 3Σqf²

01

The iε decides where the logarithm is complex

Natural units ħ = c = 1 and the metric (+, −, −, −) throughout. Topic 13.03 left Π̂₂(q²) = −(2α/π)∫₀¹ dx x(1 − x) ln[m²/(m² − x(1 − x)q² − iε)], the −iε being the Feynman propagators' m² − iε carried through the Feynman parameter. Since x(1 − x) ≤ 1/4, Δ = m² − x(1 − x)q² is positive at every x when q² is below 4m²: Π̂₂ is real in the whole spacelike region and up to threshold. Above 4m², Δ is negative on the window between x₋ and x₊, x± = (1 ± β)/2 with β = √(1 − 4m²/q²), and there ln(Δ − iε) = ln|Δ| − iπ. So Im Π̂₂ = −2α times ∫ x(1 − x) dx over the window. With x = 1/2 + y the integrand is 1/4 − y² for |y| below β/2, which integrates to β(3 − β²)/12, and since 3 − β² = 2(1 + 2m²/q²), Im Π̂₂(q² + iε) = −(α/3)β(1 + 2m²/q²), derived. At q² = 9m², β = 0.745 and Im Π̂₂ = −2.216 × 10⁻³, which a direct numerical integration of the logarithm reproduces. The sign is not a convention: the opposite iε would make the next section's cross-section negative.

02

Unitarity reads the imaginary part as a rate

Topic 5.07's optical theorem, Im ℳ(s, 0) = 2Ecm pcm σₜₒₜ, counts what a forward amplitude can produce, final state by final state. Take e⁺e⁻ → e⁺e⁻ forward through one s-channel photon, electrons massless, with the bubble of a heavier lepton f on the photon. The resummed propagator multiplies the tree by 1/(1 − Π̂), and the spin average of the two currents, (1/4)Σ Jμ Jμ† = −s, makes the forward amplitude ℳ = −e²/(1 − Π̂(s)); at order e⁴ its imaginary part is −e² Im Π̂₂(f)(s), derived. That bubble is the only order-e⁴ diagram with an f f̄ intermediate state, so with 2Ecm pcm = s the theorem gives σ(e⁺e⁻ → f f̄) = −(4πα/s) Im Π̂₂(f)(s) = (4πα²/3s)β(1 + 2m²/s). Topic 9.06 squared the tree diagram and found 4πα²/(3s) × β(3 − β²)/2, whose high-energy form PETRA tested, and (3 − β²)/2 = 1 + 2m²/s: the loop's cut and the tree's rate agree, checked. The −iπ of the logarithm was the pair being made on shell.

03

Threshold, high energy and the spin of the pair

Π̂₂ is a pure number, so −(4πα/s) Im Π̂₂ has dimension GeV⁻², an area, 0.3894 mb per GeV⁻². Just above threshold β(1 + 2m²/s) ≈ 3β/2: the rate rises linearly in β, the mark of an s wave, since a 1⁻⁻ photon makes the pair in ³S₁ with no centrifugal barrier. A spin-0 loop, quoted from scalar QED, gives −Im Π̂ = (α/12)β³ instead, a p wave, which is the point-like π⁺π⁻ rate R = β³/4: the threshold power measures the spin of what is made. Far above threshold β(1 + 2m²/s) = 1 − 6m⁴/s² + …, so −Im Π̂₂ → α/3 and σ → 86.85 nb ÷ (s in GeV²), with no m²/s correction at all. At q² = 0 there is no imaginary part: a real photon cannot decay into a pair. The one-loop rate fails near threshold, where Coulomb attraction of the slow pair multiplies it by the Sommerfeld factor (πα/β)/(1 − e(−πα/β)), quoted, about 1 + πα/(2β). BESIII's τ-mass scan fitted exactly this threshold, Coulomb and radiative factors included, and found mτ = 1776.9 MeV, quoted.

04

Analytic off the cut, so Cauchy's theorem applies

Continue q² to a complex z. The logarithm ln[1 − x(1 − x)z/m²] is singular only where its argument is real and not positive, which happens only for real z ≥ 4m², so Π̂₂(z) is analytic in the plane cut along the real axis from 4m² to ∞. It is real below threshold, so Π̂₂(z*) = Π̂₂(z)*, and the jump across the cut is Π̂₂(s + iε) − Π̂₂(s − iε) = 2i Im Π̂₂(s + iε). Apply Cauchy's theorem to Π̂₂(z)/z, which is regular at z = 0 because Π̂₂(0) = 0, on a contour that hugs the cut and closes on a large circle. Π̂₂ grows only like ln|z|, so the circle contributes nothing, and Π̂₂(q²) = (q²/π)∫ ds Im Π̂₂(s)/[s(s − q² − iε)], s from 4m² to ∞, derived. Without the division by z the integral would be ∫ ds Im Π̂₂(s)/(s − q²), which diverges logarithmically because Im Π̂₂ → −α/3: topic 13.02's pole in another form. Dividing by z is subtracting at q² = 0, and Π̂₂(0) = 0 is topic 13.03's definition of α. One subtraction, one counterterm, and no regulator anywhere.

05

Rebuilding the real part, three ways

Each limit of the dispersion relation reproduces something already derived. Small q²: with 1/(s − q²) ≈ 1/s, the slope at q² = 0 is (1/π)∫ ds Im Π̂₂/s² = −α/(15πm²), topic 13.02's result from the Feynman-parameter logarithm. Large spacelike q² = −Q²: the integrand per unit ln s is (α/3π)β(1 + 2m²/s)Q²/(s + Q²), zero at s = 4m², close to α/3π from a few times 4m² up to s ≈ Q² and small beyond, so Π̂₂(−Q²) ≈ (α/3π)[ln(Q²/4m²) − 0.280] = (α/3π)[ln(Q²/m²) − 5/3]. The logarithm is the length of that window in ln s, and 5/3 = ln 4 + 0.280: the late start at 4m², plus ∫[1 − β(1 + 2m²/s)] d ln s = 0.280 for the slow opening of the channel. At Q/m = 10 the integral gives 2.319 × 10⁻³, equal to the closed form, while the logarithm alone gives 2.275 × 10⁻³. Timelike, above threshold, the principal value gives Re Π̂₂ = (α/3π)[−5/3 − 4m²/s + β(1 + 2m²/s) ln((1 + β)/(1 − β))], which reaches −8α/(9π) = −2.06 × 10⁻³ at threshold with a square-root cusp, computed: a channel opening leaves a cusp in the real part.

06

Hadrons enter as measured R(s)

No perturbative quark loop describes what a virtual photon of 1 GeV makes: pion pairs and the ρ, ω and φ resonances. The dispersion relation never needs the loop, only Im Π̂, and the optical-theorem argument with any final state gives Im Π̂had(s) = −(α/3)R(s), derived, with R(s) = σ(e⁺e⁻ → hadrons)/(4πα²/3s). So Π̂had(q²) = −(αq²/3π)∫ ds R(s)/[s(s − q²)] from the hadronic threshold up, with R from experiment. Free quarks would give R = 3Σqf²: 2 below charm, 10/3 from charm up to the open-bottom threshold at 10.56 GeV, 11/3 above it; the measured values are about 2.2 at 2 to 3 GeV and 3.56 at 10.5 GeV, just below open bottom, quoted, the excess over 2 and 10/3 being roughly QCD's factor 1 + αₛ/π. The kernel decides which data matter. At small |q²| it weights by 1/s², so the region below 1 GeV dominates, and the hadronic part of the muon's g − 2, about 7 × 10⁻⁸ (quoted), is computed from e⁺e⁻ data with a kernel of the same kind. At Q = MZ every e-fold of s up to MZ² counts about equally, and topic 13.05 turns that integral into 1/α(MZ²).

02

Change one variable at a time

Make the relationship visible.

Interactive model
2.0
0.50

Raise Q/m from 1 to 3000: the dashed window stretches right and its area grows by one unit per e-fold of Q², so Π̂₂(−Q²) meets the large-Q² form once Q/m passes about 10. Drag the dot below 2 and both −Im Π̂₂ and the μ⁺μ⁻ cross-section fall to exactly zero.

Interactive physics modelSolid: −Im Π̂₂(s) ÷ (α/3) = β(3 − β²)/2, the pair-creation rate of a virtual photon of mass √s relative to its high-energy limit, against √s/m on a log scale: zero below the threshold at 2, rising to 1. Dashed: the same times Q²/(s + Q²) for Q/m = 100.0; its area measured in ln s, not in the log₁₀ units of the axis, times α/3π, is Π̂₂(−Q²). The dot sits at √s/m = 3.16, 334 MeV for a muon loop.Pair-creation rate and the dispersion weightsolid: −Im Π̂₂ ÷ (α/3) dashed: × Q²/(s + Q²)Q/m = 100.0: dashed area 7.54 in ln s√s = Q11210010⁴√s/m, log scale

−Im Π̂₂ AT THE DOT2.261 × 10⁻³

σ(e⁺e⁻ → μ⁺μ⁻) AT THE DOT723.171 nb

Π̂₂(−Q²) FROM THE CUT5.841 × 10⁻³

LARGE-Q² LOG FORM5.841 × 10⁻³

Live interpretation−Im Π̂₂ AT THE DOT: 2.261 × 10⁻³. σ(e⁺e⁻ → μ⁺μ⁻) AT THE DOT: 723.171 nb. Π̂₂(−Q²) FROM THE CUT: 5.841 × 10⁻³. LARGE-Q² LOG FORM: 5.841 × 10⁻³

03

Catch the common trap

Explain before calculating.

Deep-inelastic electron-proton scattering exchanges a photon with q² = −(100 GeV)², so |q²| is about 10¹⁰ times 4mₑ². At one loop, what is the imaginary part of the electron loop's Π̂₂ at this q²?

Choose an answer to test the model.

04

Practice & worked examples

Reason from the model, then test the result.

EasyA collider runs at √s = 4.00 GeV, above the τ-pair threshold. Find Im Π̂₂ for the τ loop (mτ = 1.77686 GeV) and for the muon loop at this energy, then use the optical theorem to obtain σ(e⁺e⁻ → τ⁺τ⁻) in nanobarns and compare it with the point-like 4πα²/(3s).
  1. s = 16.00 GeV² and 4mτ² = 12.629 GeV², so the τ cut is open. β = √(1 − 12.629/16.00) = √0.21069 = 0.4590, and 1 + 2mτ²/s = 1 + 6.3145/16.00 = 1.3947.
  2. Im Π̂₂ = −(α/3)β(1 + 2m²/s) = −(2.4325 × 10⁻³)(0.4590)(1.3947) = −1.557 × 10⁻³ for the τ loop.
  3. For the muon, mμ²/s = 6.98 × 10⁻⁴ and β(1 + 2m²/s) = 1 − 6(m²/s)² = 0.999997, so Im Π̂₂ = −2.432 × 10⁻³ = −α/3: this far above threshold the mass has dropped out to order m⁴/s².
  4. Optical theorem: σ = −(4πα/s) Im Π̂₂ = 0.091701 × 1.5572 × 10⁻³/(16.00 GeV²) = 8.925 × 10⁻⁶ GeV⁻², and with 0.3894 mb GeV² this is 3.475 × 10⁻⁶ mb = 3.475 nb.
  5. The point-like value is 86.85 nb/16.00 = 5.428 nb, so τ pairs come at 0.640 of it, which is β(3 − β²)/2 = 0.4590 × 2.7893/2 = 0.6402. Checks: σ is an area; it vanishes linearly in β at threshold and tends to the point-like value far above it.

AnswerIm Π̂₂ = −1.56 × 10⁻³ for the τ loop and −2.43 × 10⁻³ = −α/3 for the muon loop; σ(e⁺e⁻ → τ⁺τ⁻) = 3.48 nb, 0.640 of the point-like 5.43 nb.

MediumExpand the once-subtracted dispersion relation about q² = 0 to find the slope dΠ̂₂/dq² at q² = 0 for a lepton of mass m, and compare it with topic 13.02. Then find what fraction of the slope comes from pairs with √s/m below 3 and below 10, and compare with the share of Π̂₂(−Q²) at Q/m = 100 that comes from √s/m below 10.
  1. For |q²| well below 4m², 1/(s − q²) = 1/s + q²/s² + …, so Π̂₂(q²) = (q²/π)∫ ds Im Π̂₂(s)/s² + O(q⁴). The slope is (1/π)∫ ds Im Π̂₂(s)/s² = −(α/3π)∫ ds β(1 + 2m²/s)/s², s from 4m² to ∞.
  2. Put u = 4m²/s, so ds/s² = −du/(4m²), β = √(1 − u) and 1 + 2m²/s = 1 + u/2. The integral becomes (1/4m²)∫₀¹ √(1 − u)(1 + u/2) du = (1/4m²)(2/3 + 2/15) = 1/(5m²), using ∫₀¹ u√(1 − u) du = 4/15.
  3. So the slope is −α/(15πm²) and Π̂₂ ≈ −αq²/(15πm²), exactly topic 13.02's result from expanding the Feynman-parameter logarithm. Checks: it has dimension GeV⁻², and it vanishes as m → ∞, a heavy loop decoupling. For the electron it is −5.93 × 10⁻⁴ MeV⁻².
  4. Cutting the u integral at u = 4/9 (√s/m = 3) and at u = 0.04 (√s/m = 10) and integrating numerically, the region below √s/m = 3 supplies 46.0% of the slope and the region below 10 supplies 95.0%.
  5. At Q/m = 100 the integrand per unit ln s is (α/3π)β(1 + 2m²/s)Q²/(s + Q²). The whole integral is 7.544 in units of α/3π, so Π̂₂ = 5.841 × 10⁻³; √s/m below 10 supplies 2.929 of it, 38.8%, and √s/m below 3 only 7.6%.
  6. The 1/s² weight of the slope favours the threshold, while at large Q² every e-fold of s up to Q² counts about equally: low-q² quantities are set by low-energy pairs, large-Q² ones by the whole spectrum.

AnswerSlope −α/(15πm²), topic 13.02's result. 46% of it comes from √s/m below 3 and 95% from below 10, against 7.6% and 38.8% of Π̂₂(−Q²) = 5.84 × 10⁻³ at Q/m = 100.

HardA narrow vector meson V of mass M and electronic width Γₑₑ adds ∫σ(e⁺e⁻ → V → anything) ds = 12π²Γₑₑ/M, quoted from the spin-1 Breit-Wigner formula. Find its Im Π̂ and, by the dispersion relation, its Π̂(q²). For the J/ψ (M = 3.0969 GeV, Γₑₑ = 5.53 keV), find the shift of 1/α at spacelike Q = MZ = 91.19 GeV, and Π̂V at timelike √q² = 3.000 GeV and 3.200 GeV.
  1. R(s) = 3sσ/(4πα²). Away from its peak a resonance this narrow acts as a δ-function: R(s) = (3M²/4πα²)(12π²Γₑₑ/M)δ(s − M²) = (9πMΓₑₑ/α²)δ(s − M²), so Im Π̂V(s) = −(α/3)R(s) = −(3πMΓₑₑ/α)δ(s − M²).
  2. The dispersion relation does the integral at once: Π̂V(q²) = (q²/π)(−3πMΓₑₑ/α)/[M²(M² − q²)] = −(3Γₑₑ/αM) q²/(M² − q²), derived. Checks: Γₑₑ/M is dimensionless, Π̂V(0) = 0 as the definition of α requires, and for |q²| ≪ M² it falls as q²/M², a heavy state decoupling.
  3. Numerically 3Γₑₑ/(αM) = 3 × 5.53 × 10⁻⁶ GeV × 137.036/3.0969 GeV = 7.341 × 10⁻⁴.
  4. At q² = −MZ² = −8315.6 GeV², Π̂V = 7.341 × 10⁻⁴ × 8315.6/(9.591 + 8315.6) = 7.333 × 10⁻⁴. Since 1/αeff = (1 − Π̂)/α, the J/ψ lowers 1/α(MZ²) by 7.333 × 10⁻⁴ × 137.036 = 0.100, about 2.7% of the 3.78 by which hadrons must take the three-lepton 132.73 to the measured 128.95 (topic 13.05).
  5. At √q² = 3.000 GeV, 97 MeV below the peak and about a thousand total widths (Γ = 92.6 keV) away: Π̂V = −7.341 × 10⁻⁴ × 9.000/0.591 = −0.0112. At 3.200 GeV: Π̂V = +7.341 × 10⁻⁴ × 10.240/0.649 = +0.0116.
  6. The real part changes sign through the resonance and near it is fifteen times its value at MZ: the absorptive peak in R has a dispersive partner that lowers αeff just below the J/ψ and raises it just above. Within a few widths of the peak the δ-function must give way to the full Breit-Wigner shape.

AnswerIm Π̂V = −(3πMΓₑₑ/α)δ(s − M²) and Π̂V(q²) = −(3Γₑₑ/αM)q²/(M² − q²), with 3Γₑₑ/αM = 7.34 × 10⁻⁴. The J/ψ lowers 1/α(MZ²) by 0.100; Π̂V = −0.0112 at 3.000 GeV and +0.0116 at 3.200 GeV.

Extra challenging questions

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