Bhabha scattering at NNLO with next-to-soft stabilisation
arXiv:2106.07469 · doi:10.1016/j.physletb.2021.136547
Abstract
A critical subject in fully differential QED calculations originates from numerical instabilities due to small fermion masses that act as regulators of collinear singularities. At next-to-next-to-leading order (NNLO) a major challenge is therefore to find a stable implementation of numerically delicate real-virtual matrix elements. In the case of Bhabha scattering this has so far prevented the development of a fixed-order Monte Carlo at NNLO accuracy. In this paper we present a new method for stabilising the real-virtual matrix element. It is based on the expansion for soft photon energies including the non-universal subleading term calculated with the method of regions. We have applied this method to Bhabha scattering to obtain a stable and efficient implementation within the McMule framework. We therefore present for the first time fully differential results for the photonic NNLO corrections to Bhabha scattering.
6 pages, 3 figures
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- Towards testing in : radiative corrections and projections for Belle II
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- Analytic results for two-loop planar master integrals for Bhabha scattering