Radiative corrections to pair production of unstable particles: results for e^+e^- --> 4 fermions
W. Beenakker, F. A. Berends, A. P. Chapovsky
TL;DR
This work develops and applies a gauge-invariant double-pole approximation (DPA) within a pole-scheme framework to compute the complete ${\cal O}(\alpha)$ electroweak radiative corrections to $e^{+}e^{-} \to W^{+}W^{-} \to 4f$ with unstable $W$ bosons. It cleanly separates factorizable corrections (production and decay of on-shell $W$'s) from non-factorizable, soft/semisoft photon exchanges that couple different stages, and treats real-photon radiation across hard, semi-soft, and soft regimes with carefully defined phase-space mappings. The results show sizable corrections near the $W$-pair threshold driven predominantly by initial-state radiation, along with observable distortions in invariant-mass and angular distributions; non-factorizable corrections are generally small, while the formalism remains gauge-invariant and implementable for LEP2-era phenomenology and beyond. The study provides a practical, quantitative framework for incorporating RC into four-fermion final states via a DPA-based event-generation-compatible approach, enabling precise tests of the Standard Model and robust comparisons to anomalous triple gauge-boson couplings.
Abstract
Radiative corrections to processes that involve the production and subsequent decay of unstable particles are complex due to various theoretical and practical problems. The so-called double-pole approximation offers a way out of these problems. This method is applied to the reaction $e^{+}e^{-} \to W^{+}W^{-} \to 4 $fermions, which allows us to address all the key issues of dealing with unstable particles, like gauge invariance, interactions between different stages of the reaction, and overlapping resonances. Within the double-pole approximation the complete $\OO(α)$ electroweak corrections are evaluated for this off-shell $W$-pair production process. Examples of the effect of these corrections on a number of distributions are presented. These comprise mass and angular distributions as well as the photon-energy spectrum.
