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@PHDTHESIS{Saragnese:481508,
author = {Saragnese, Marco},
othercontributors = {Blümlein, Johannes and Moch, Sven-Olaf},
title = {{M}assive 2- and 3-loop corrections to hard scattering
processes in {QCD}},
school = {Universität Hamburg},
type = {Dissertation},
address = {Hamburg},
publisher = {Verlag Deutsches Elektronen-Synchrotron DESY},
reportid = {PUBDB-2022-04411, DESY-THESIS-2022-016},
series = {DESY-THESIS},
pages = {258},
year = {2022},
note = {Dissertation, Universität Hamburg, 2022},
abstract = {This thesis deals with calculations of higher-order
corrections in perturbative quantum chromodynamics(QCD). The
two-mass contributions to the 3-loop, polarized twist-two
operator matrixelements (OMEs) A(3),PSQq and A(3)gg,Q are
calculated. The N-space result for A(3)gg,Q is obtained
analyticallyas a function of the quark mass ratio, which for
A(3),PSQq is not yet possible. In thez-space representation,
one obtains for both matrix elements semi-analytical
representations interms of iterated integrals, whereby for
reasons of efficiency an additional integral is necessaryfor
some terms.These universal (process-independent) massive
OMEs govern the asymptotic behaviour ofthe Wilson
coefficients in deep-inelastic scattering at large
virtualities Q2 ≫ m2c,b, with mc,bthe charm and bottom
quark masses. These corrections are also required to define
the variableflavour number scheme. This scheme describes the
transition from massive quark corrections tothe massless
ones for very high momentum scales, which is relevant to the
description of colliderdata.In the single-mass, polarized
case, we derive the logarithmic corrections for the Wilson
coefficientsof the structure function g1 in the asymptotic
region Q2 ≫ m2c,b. This is done using theknown OMEs and
massless Wilson coefficients, using the renormalization
group equations.For the non-singlet structure functions FNS2
and gNS1 we revisit the scheme-invariant evolutionoperator
known for massless quarks and extend it to the massive case
with single- and two-masscorrections. In this case, the
evolution can effectively be described up to O(a3s) in the
Wilsoncoefficients, where as = αs/(4π) denotes the strong
coupling constant. The influence of thehitherto not fully
known 4-loop non-singlet anomalous dimension can be
described effectively.It turns out that the effect of the
theory error in question can be completely controlled.
Arepresentation by a Pad´e approximant proves to be
sufficient.We consider the class of functions of
multivariate hypergeometric series and study systemsof
differential equations obeyed by them. We describe an
algorithmic method to solve someclasses of such differential
systems which delivers a hypergeometric series solution
having nestedhypergeometric products as summand; we discuss
the relationship between these products andPochhammer
symbols. For a number of classical hypergeometric series we
derive differentialsystems and their associated difference
equations. We present some examples of series expansionsof
such functions and of the mathematical objects which arise
therein. We also present aMathematica package which
implements algorithms related to the solution of partial
linear differenceequations, focusing in particular on
bounding the degree of the denominator of solutionswhich are
rational functions. These methods are of particular
importance when solving multi-legcalculations for Feynman
diagrams, but also come into play when hypergeometric
methods formulti-loop integrals are used.We describe a
numerical implementation of an N-space library for the
calculation of scalingviolations for structure functions,
which can perform the evolution of parton
distributionfunctions up to NNLO from a parametrization
chosen by the user, and encodes massless andmassive Wilson
coefficients for the structure functions F2 and g1 in the
case of photon exchange,and for the structure functions
FW+±W−3 in the case of charged-current exchange. The
librarycontains analytic continuation of the relevant
harmonic sums in Mellin-space up to weight 5 andmany
weight-6 harmonic sums. The numerical representation in x
space is performed by contourintegration around the
singularities of the solution of the evolution equations in
N space.},
cin = {$Z_ZPPT$},
cid = {$I:(DE-H253)Z_ZPPT-20210408$},
pnm = {611 - Fundamental Particles and Forces (POF4-611) / SAGEX -
Scattering Amplitudes: from Geometry to Experiment (764850)},
pid = {G:(DE-HGF)POF4-611 / G:(EU-Grant)764850},
experiment = {EXP:(DE-MLZ)NOSPEC-20140101},
typ = {PUB:(DE-HGF)3 / PUB:(DE-HGF)11},
doi = {10.3204/PUBDB-2022-04411},
url = {https://bib-pubdb1.desy.de/record/481508},
}