Infrared divergences in scattering amplitudes from correlators of Wilson Lines
dc.contributor.advisor
Gardi, Einan
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dc.contributor.advisor
Smillie, Jennifer
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dc.contributor.author
Milloy, Calum William
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dc.contributor.sponsor
other
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dc.date.accessioned
2021-01-26T12:29:33Z
dc.date.available
2021-01-26T12:29:33Z
dc.date.issued
2020-11-30
dc.description.abstract
Scattering amplitudes in theories with massless particles feature infrared (IR)
divergences. In QCD, gluons are massless and when their momenta tends to zero
the amplitude diverges. We call this a soft divergence. For massless external
particles there are further divergences called collinear divergences, when the
invariant jet mass of the external and a radiated gluon tends to zero. Even
in a UV finite theory such as N = 4 super-Yang Mills there exists infrared
divergences. In fact, in the planar theory there exists an all-order ansatz for the
IR divergences called the BDS ansatz which amounts to the exponentiation of the
one loop result with anomalous dimensions that can be computed to all orders.
In this thesis we shall be considering the more complicated case of non-planar
QCD with both massless and massive scattering particles.
First, we shall review the IR factorisation formula for massive scattering
amplitudes. Here, soft divergences are described by the soft anomalous dimension
matrix. It is defined to be a vacuum expectation value of non-lightlike Wilson
lines. This object is calculable in perturbation theory. It exponentiates and
the exponent is a sum over webs. We will then focus on how to calculate the
individual integrals that appear in webs. The technique of differential equations
is explained and applied to integrals up to two loops for webs. We then discuss a
basis of functions for these specific integrals with the idea of creating an ansatz
for the soft anomalous dimension and other related quantities.
The second half of the thesis concerns massless scattering amplitudes. By
factorising not only the amplitude but also a parton distribution function we
find that they share the same hard collinear behaviour. They differ in their
pure soft poles which are governed by lightlike Wilson-line correlators that follow
different contours dictated by the kinematics. It allows us to explain an observed
relation between the subleading pole of the form factor, γG, and the coefficient
of δ(1 − x) in the DGLAP splitting kernels, Bδ. We then argue that divergences
of lightlike Wilson-line correlators take a general form that only depend on local
features, individual line lengths, and not on the global geometry.
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dc.identifier.uri
https://hdl.handle.net/1842/37487
dc.identifier.uri
http://dx.doi.org/10.7488/era/771
dc.language.iso
en
dc.publisher
The University of Edinburgh
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dc.relation.hasversion
G. Falcioni, E. Gardi and C. Milloy, Relating amplitude and PDF factorisation through Wilson-line geometries, JHEP 11 (2019) 100 [1909.00697].
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dc.subject
Large Hadron Collider
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dc.subject
LHC
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dc.subject
resummation
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dc.subject
resummation calculations
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dc.subject
non-planar QCD
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dc.subject
massless scattering amplitudes
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dc.subject
Wilson-line
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dc.title
Infrared divergences in scattering amplitudes from correlators of Wilson Lines
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dc.type
Thesis or Dissertation
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dc.type.qualificationlevel
Doctoral
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dc.type.qualificationname
PhD Doctor of Philosophy
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