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High Energy Physics - PhenomenologyEnglishPublished

Electron collisions use parton‑density functions to capture photon and lepton pair emissions

November 10, 2026arXiv: 2611.09408v1

In studies of electron‑positron collisions, physicists treat the incoming lepton as a composite object. The probability of finding an electron, a positron or a photon inside the incoming particle is encoded in parton‑density functions (PDFs). These PDFs obey evolution equations that were originally developed for strongly interacting quarks and gluons but have been adapted to the electromagnetic theory of QED.

Using this framework, researchers calculated how much the cross section for final‑state radiation changes when photons or lepton pairs are emitted from the initial state. At the mass of the Z boson (√s≈91.2 GeV) with no invariant‑mass cut, the leading photonic correction is –32.75 %. When a cut on the minimal invariant mass is applied (zmin=0.8) the correction reduces to –19.71 %. In both cases the leading pair correction remains essentially zero. A more detailed table shows the full set of coefficients for different cuts and energies.

Table of numerical values for leading photonic and pair corrections: h11 = –32.75 % (Z pole, no cut), 0 % (pair), –19.71 % (240 GeV, zmin = 0.8), 0 % (pair).
h11h10
h22
h21
h20
h33
h32
h44
h43
h55
s=MZ
zm​i​n=0.3
γ-32.746742.002104.88350-0.595130.01521-0.377570.071020.00345-0.001850.00315
Pairs00-0.306330.15852-0.021510.08757-0.04604-0.009090.00375-0.00008
Full-32.746742.002104.57747-0.43662-0.00630-0.290020.02499-0.005640.001900.00307
zm​i​n=0.8
γ-32.822412.005214.88622-0.595890.01524-0.376970.070940.00338-0.001840.00315
Pairs00-0.307190.15883-0.021500.08763-0.046040.009070.00374-0.00008
Full-32.822412.005214.57904-0.43706-0.00626-0.289840.02490-0.005680.001900.00307
s=240 GeV
zm​i​n=0.3
γ11.885970.19300-0.664630.16592-0.00779-0.036370.003670.00250-0.001202⋅10−7
Pairs000.23207-0.07145-0.00710-0.019580.00776-0.001260.000870.00009
Full11.885970.193000.432560.09446-0.01480-0.055950.011430.00124-0.000330.00009
zm​i​n=0.8
γ-19.710711.02535-0.641570.01773-0.000460.15716-0.02851-0.009600.002670.00002
Pairs00-0.097420.02401-0.00297-0.014800.009950.00455-0.00250-0.00028
Full-19.710711.02535-0.739890.04174-0.003430.14236-0.01856-0.005050.00018-0.00026
Table 1. Table 1 lists the leading photonic and pair corrections (h11) at the Z pole (no invariant‑mass cut) and at √s=240 GeV with zmin=0.8, showing the −32.75 % photonic and 0 % pair values at the Z pole and the −19.71 % photonic and 0 % pair values at 240 GeV.Arbuzov, Andrej, Romero, Cecilia, Voznaya, Uliana · arXiv:2611.09408v1 · Table 1: · CC BY 4.0

These numbers illustrate how resumming collinear emissions is essential for precision predictions. The perturbative expansion in powers of αⁿLⁿ converges slowly, especially near the soft‑photon limit where x→1. Consequently, explicit resummation or exponentiation is required to achieve the required accuracy.

The table also indicates that at a higher centre‑of‑mass energy (√s=240 GeV), photonic corrections become positive when the same invariant‑mass cut is applied, while pair corrections stay small. This energy dependence highlights the changing role of initial‑state radiation with collider energy.

These calculations underpin the theoretical accuracy needed for future electron‑positron colliders, ensuring that predictions for processes such as Higgs production or electroweak precision tests are reliable.

Source paper

Parton density functions for future electron-positron colliders

High Energy Physics - Phenomenology
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