
SciPost Physics Submission
2 Theory uncertainties from scale variations
The description of proton-proton collisions in the collinear approximation is based on the
separation of hard scattering at the parton level convolved with universal parton densities
encapsulating non-perturbative inputs [7,8],
σ(θ)≈X
a,bZd xaxbfa(xa;µF)fb(xb;µF)ˆ
σab(θ;µF,µR), (1)
where the sum runs over partons inside the protons, fa/bare parton distribution functions
(PDFs), ˆ
σis the partonic hard-scattering cross-section, and θrepresents parameter(s) of in-
terest. A typical LHC analysis infers information on the parameter of interest θthrough com-
parison with data measuring the observable σ(θ). We will be concerned primarily with inclu-
sive cross sections, which are under better theoretical control than differential cross-sections,
including QCD radiation of jets, or fully exclusive event generation.
The partonic cross-section ˆ
σis computed as a perturbative expansion in the QCD coupling
αs[6], but estimating the precision of a given truncation is challenging. Estimates based on
the size of the expansion parameter αs, or αs/π, are fraught because the perturbative series
formally has a zero radius of convergence, implying that at a high enough order one does
not expect subsequent terms in the expansion to be smaller than the preceding ones. While
most predictions for inclusive cross-sections at the LHC appear to be convergent at least up
to next-to-next-to-leading order (NNLO), naive estimates based on the size of the expansion
parameter are found to be insufficiently conservative [6].
The PDFs appearing in Eq.(1) are extracted from a large orthogonal dataset (keeping track
of the scale dependence) under the assumption that the relevant processes are described by
the SM [9], and include their own comprehensive uncertainty treatment [10–13].
At each perturbative order, ultraviolet (UV) divergences in cross-section predictions are
removed through renormalization, introducing a logarithmic dependence on an unphysical
renormalization scale µRin the prediction. Similarly, infrared (IR) and collinear divergences
are absorbed into the definition of the parton densities, introducing logarithms of an equally
unphysical factorization scale µF. Both scales can be related through the resummation of
large collinear logarithms, but generally are independent scales with different infrared and
ultraviolet origins and can be chosen independently [7].
The dependence of the theoretical prediction on the choice of scale introduces an arbi-
trariness into the prediction, and is an artifact arising from the truncation of the perturbative
series. Formally, at all orders, the scale dependence would vanish, and thus the degree to
which the prediction depends on the choice of scale at any finite order can be thought of as
a measure of how significant the contribution of the uncomputed remaining terms in the se-
ries is expected to be. Traditionally, the uncertainty on the predicted hadronic cross-section
in Eq.(1) is estimated by varying µRand µFaround a suitable central scale. The choice of the
central scale can vary depending on the physics process, it could be for example the scalar sum
of transverse mass of all final state particles,the invariant mass of the system being produced,
the average transverse energy of jets produced, or centre-of-mass energy of the collider. The
logarithmic dependence on the scale requires µ∼Ewhere Echaracterizes the physical en-
ergy scale appearing in the observable of interest. This choice insures that terms growing as
log E/µ do not spoil perturbation theory, but it cannot distinguish choices of scale differing by
order-one factors.
While the scale variation may provide a measure of the impact of missing higher orders,
it is not the ‘true’ uncertainty – which would quantify the likelihood distribution of the differ-
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