NNLO QCD corrections to associated $WH$ production and $H \to b \bar b$ decay
Fabrizio Caola, Gionata Luisoni, Kirill Melnikov, Raoul Röntsch
TL;DR
The paper delivers fully differential NNLO QCD corrections to Higgs production in association with a W boson and the subsequent H → bb decay in the massless b-quark limit, using a nested soft-collinear subtraction framework. It includes top-quark-loop Higgs emission contributions and a previously neglected NNLO decay term, and examines the impact of experimental cuts on kinematic distributions. The study demonstrates substantial corrections in certain observables and validates fixed-order results against parton-shower simulations, emphasizing the importance of precise NNLO predictions for WH(b b) phenomenology. It also highlights the need for fully massive-bottom calculations to address interference effects that arise at NNLO in the decay stage.
Abstract
We present a computation of the next-to-next-to-leading order (NNLO) QCD corrections to the production of a Higgs boson in association with a W boson at the LHC and the subsequent decay of the Higgs boson into a b-bbar pair, treating the b-quarks as massless. We consider various kinematic distributions and find significant corrections to observables that resolve the Higgs decay products. We also find that a cut on the transverse momentum of the W boson, important for experimental analyses, may have a significant impact on kinematic distributions and radiative corrections. We show that some of these effects can be adequately described by simulating QCD radiation in Higgs boson decays to b-quarks using parton showers. We also describe contributions to Higgs decay to a b-bbar pair that first appear at NNLO and that were not considered in previous fully-differential computations. The calculation of NNLO QCD corrections to production and decay sub-processes is carried out within the nested soft-collinear subtraction scheme presented by some of us earlier this year. We demonstrate that this subtraction scheme performs very well, allowing a computation of the coefficient of the second order QCD corrections at the level of a few per mill.
