\relax \providecommand\hyper@newdestlabel[2]{} \providecommand\BKM@entry[2]{} \providecommand\HyperFirstAtBeginDocument{\AtBeginDocument} \HyperFirstAtBeginDocument{\ifx\hyper@anchor\@undefined \global\let\oldcontentsline\contentsline \gdef\contentsline#1#2#3#4{\oldcontentsline{#1}{#2}{#3}} \global\let\oldnewlabel\newlabel \gdef\newlabel#1#2{\newlabelxx{#1}#2} \gdef\newlabelxx#1#2#3#4#5#6{\oldnewlabel{#1}{{#2}{#3}}} \AtEndDocument{\ifx\hyper@anchor\@undefined \let\contentsline\oldcontentsline \let\newlabel\oldnewlabel \fi} \fi} \global\let\hyper@last\relax \gdef\HyperFirstAtBeginDocument#1{#1} \providecommand\HyField@AuxAddToFields[1]{} \providecommand\HyField@AuxAddToCoFields[2]{} \bibstyle{lucas_unsrt} \abx@aux@refcontext{nty/global//global/global} \abx@aux@cite{PREV_RESEARCH} \abx@aux@segm{0}{0}{PREV_RESEARCH} \abx@aux@cite{DEEP_BOOSTED} \abx@aux@segm{0}{0}{DEEP_BOOSTED} \abx@aux@cite{TAU21} \abx@aux@segm{0}{0}{TAU21} \@writefile{toc}{\boolfalse {citerequest}\boolfalse {citetracker}\boolfalse {pagetracker}\boolfalse {backtracker}\relax } \@writefile{lof}{\boolfalse {citerequest}\boolfalse {citetracker}\boolfalse {pagetracker}\boolfalse {backtracker}\relax } \@writefile{lot}{\boolfalse {citerequest}\boolfalse {citetracker}\boolfalse {pagetracker}\boolfalse {backtracker}\relax } \babel@aux{british}{} \BKM@entry{id=1,dest={73656374696F6E2E31},srcline={143},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030495C3030306E5C303030745C303030725C3030306F5C303030645C303030755C303030635C303030745C303030695C3030306F5C3030306E} \abx@aux@segm{0}{0}{PREV_RESEARCH} \@writefile{toc}{\contentsline {section}{\numberline {1}Introduction}{1}{section.1}\protected@file@percent } \newlabel{introduction}{{1}{1}{Introduction}{section.1}{}} \BKM@entry{id=2,dest={73656374696F6E2E32},srcline={192},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030545C303030685C303030655C3030306F5C303030725C303030655C303030745C303030695C303030635C303030615C3030306C5C3030305C3034305C3030306D5C3030306F5C303030745C303030695C303030765C303030615C303030745C303030695C3030306F5C3030306E} \BKM@entry{id=3,dest={73756273656374696F6E2E322E31},srcline={201},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030535C303030745C303030615C3030306E5C303030645C303030615C303030725C303030645C3030305C3034305C3030306D5C3030306F5C303030645C303030655C3030306C} \@writefile{toc}{\contentsline {section}{\numberline {2}Theoretical motivation}{2}{section.2}\protected@file@percent } \newlabel{theoretical-motivation}{{2}{2}{Theoretical motivation}{section.2}{}} \@writefile{toc}{\contentsline {subsection}{\numberline {2.1}Standard model}{2}{subsection.2.1}\protected@file@percent } \newlabel{sec:sm}{{2.1}{2}{Standard model}{subsection.2.1}{}} \@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces Elementary particles of the Standard Model and their mass charge and spin.\relax }}{2}{figure.caption.2}\protected@file@percent } \providecommand*\caption@xref[2]{\@setref\relax\@undefined{#1}} \newlabel{fig:sm}{{1}{2}{Elementary particles of the Standard Model and their mass charge and spin.\relax }{figure.caption.2}{}} \BKM@entry{id=4,dest={73756273756273656374696F6E2E322E312E31},srcline={300},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030535C303030685C3030306F5C303030725C303030745C303030635C3030306F5C3030306D5C303030695C3030306E5C303030675C303030735C3030305C3034305C3030306F5C303030665C3030305C3034305C303030745C303030685C303030655C3030305C3034305C303030535C303030745C303030615C3030306E5C303030645C303030615C303030725C303030645C3030305C3034305C3030304D5C3030306F5C303030645C303030655C3030306C} \BKM@entry{id=5,dest={73756273656374696F6E2E322E32},srcline={333},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030455C303030785C303030635C303030695C303030745C303030655C303030645C3030305C3034305C303030715C303030755C303030615C303030725C3030306B5C3030305C3034305C303030735C303030745C303030615C303030745C303030655C30303073} \@writefile{toc}{\contentsline {subsubsection}{\numberline {2.1.1}Shortcomings of the Standard Model}{4}{subsubsection.2.1.1}\protected@file@percent } \newlabel{shortcomings-of-the-standard-model}{{2.1.1}{4}{Shortcomings of the Standard Model}{subsubsection.2.1.1}{}} \@writefile{toc}{\contentsline {subsection}{\numberline {2.2}Excited quark states}{4}{subsection.2.2}\protected@file@percent } \newlabel{sec:qs}{{2.2}{4}{Excited quark states}{subsection.2.2}{}} \@writefile{lof}{\contentsline {figure}{\numberline {2}{\ignorespaces Feynman diagram showing a possible decay of a q* particle to a W boson and a quark with the W boson also decaying to two quarks.\relax }}{4}{figure.caption.3}\protected@file@percent } \newlabel{fig:qsfeynman}{{2}{4}{Feynman diagram showing a possible decay of a q* particle to a W boson and a quark with the W boson also decaying to two quarks.\relax }{figure.caption.3}{}} \abx@aux@cite{QSTAR_THEORY} \abx@aux@segm{0}{0}{QSTAR_THEORY} \gdef \LT@i {\LT@entry {1}{63.63869pt}\LT@entry {1}{71.97462pt}\LT@entry {1}{69.63869pt}\LT@entry {1}{65.97462pt}} \abx@aux@segm{0}{0}{PREV_RESEARCH} \BKM@entry{id=6,dest={73756273756273656374696F6E2E322E322E31},srcline={421},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030515C303030755C303030615C3030306E5C303030745C303030755C3030306D5C3030305C3034305C303030435C303030685C303030725C3030306F5C3030306D5C3030306F5C303030645C303030795C3030306E5C303030615C3030306D5C303030695C303030635C3030305C3034305C303030625C303030615C303030635C3030306B5C303030675C303030725C3030306F5C303030755C3030306E5C30303064} \@writefile{lot}{\contentsline {table}{\numberline {1}{\ignorespaces Branching ratios of the decaying q* particle.\relax }}{5}{table.1}\protected@file@percent } \@writefile{toc}{\contentsline {subsubsection}{\numberline {2.2.1}Quantum Chromodynamic background}{5}{subsubsection.2.2.1}\protected@file@percent } \newlabel{sec:qcdbg}{{2.2.1}{5}{Quantum Chromodynamic background}{subsubsection.2.2.1}{}} \@writefile{lof}{\contentsline {figure}{\numberline {3}{\ignorespaces Two examples of QCD processes resulting in two jets.\relax }}{6}{figure.caption.4}\protected@file@percent } \newlabel{fig:qcdfeynman}{{3}{6}{Two examples of QCD processes resulting in two jets.\relax }{figure.caption.4}{}} \BKM@entry{id=7,dest={73656374696F6E2E33},srcline={453},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030455C303030785C303030705C303030655C303030725C303030695C3030306D5C303030655C3030306E5C303030745C303030615C3030306C5C3030305C3034305C303030535C303030655C303030745C303030755C30303070} \BKM@entry{id=8,dest={73756273656374696F6E2E332E31},srcline={459},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C3030304C5C303030615C303030725C303030675C303030655C3030305C3034305C303030485C303030615C303030645C303030725C3030306F5C3030306E5C3030305C3034305C303030435C3030306F5C3030306C5C3030306C5C303030695C303030645C303030655C30303072} \abx@aux@cite{website} \abx@aux@segm{0}{0}{website} \BKM@entry{id=9,dest={73756273656374696F6E2E332E32},srcline={494},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030435C3030306F5C3030306D5C303030705C303030615C303030635C303030745C3030305C3034305C3030304D5C303030755C3030306F5C3030306E5C3030305C3034305C303030535C3030306F5C3030306C5C303030655C3030306E5C3030306F5C303030695C30303064} \@writefile{toc}{\contentsline {section}{\numberline {3}Experimental Setup}{7}{section.3}\protected@file@percent } \newlabel{experimental-setup}{{3}{7}{Experimental Setup}{section.3}{}} \@writefile{toc}{\contentsline {subsection}{\numberline {3.1}Large Hadron Collider}{7}{subsection.3.1}\protected@file@percent } \newlabel{large-hadron-collider}{{3.1}{7}{Large Hadron Collider}{subsection.3.1}{}} \@writefile{toc}{\contentsline {subsection}{\numberline {3.2}Compact Muon Solenoid}{7}{subsection.3.2}\protected@file@percent } \newlabel{compact-muon-solenoid}{{3.2}{7}{Compact Muon Solenoid}{subsection.3.2}{}} \abx@aux@cite{CMS_PLOT} \abx@aux@segm{0}{0}{CMS_PLOT} \abx@aux@segm{0}{0}{CMS_PLOT} \BKM@entry{id=10,dest={73756273756273656374696F6E2E332E322E31},srcline={524},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030435C3030306F5C3030306F5C303030725C303030645C303030695C3030306E5C303030615C303030745C303030655C3030305C3034305C303030635C3030306F5C3030306E5C303030765C303030655C3030306E5C303030745C303030695C3030306F5C3030306E5C30303073} \BKM@entry{id=11,dest={73756273756273656374696F6E2E332E322E32},srcline={553},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030545C303030685C303030655C3030305C3034305C303030745C303030725C303030615C303030635C3030306B5C303030695C3030306E5C303030675C3030305C3034305C303030735C303030795C303030735C303030745C303030655C3030306D} \@writefile{lof}{\contentsline {figure}{\numberline {4}{\ignorespaces The setup of the Compact Muon Solenoid showing its onion like structure, the different detector parts and where different particles are detected \autocite {CMS_PLOT}.\relax }}{8}{figure.caption.5}\protected@file@percent } \newlabel{fig:cms_setup}{{4}{8}{The setup of the Compact Muon Solenoid showing its onion like structure, the different detector parts and where different particles are detected \autocite {CMS_PLOT}.\relax }{figure.caption.5}{}} \@writefile{toc}{\contentsline {subsubsection}{\numberline {3.2.1}Coordinate conventions}{8}{subsubsection.3.2.1}\protected@file@percent } \newlabel{coordinate-conventions}{{3.2.1}{8}{Coordinate conventions}{subsubsection.3.2.1}{}} \BKM@entry{id=12,dest={73756273756273656374696F6E2E332E322E33},srcline={563},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030545C303030685C303030655C3030305C3034305C303030655C3030306C5C303030655C303030635C303030745C303030725C3030306F5C3030306D5C303030615C303030675C3030306E5C303030655C303030745C303030695C303030635C3030305C3034305C303030635C303030615C3030306C5C3030306F5C303030725C303030695C3030306D5C303030655C303030745C303030655C30303072} \BKM@entry{id=13,dest={73756273756273656374696F6E2E332E322E34},srcline={577},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030545C303030685C303030655C3030305C3034305C303030685C303030615C303030645C303030725C3030306F5C3030306E5C303030695C303030635C3030305C3034305C303030635C303030615C3030306C5C3030306F5C303030725C303030695C3030306D5C303030655C303030745C303030655C30303072} \BKM@entry{id=14,dest={73756273756273656374696F6E2E332E322E35},srcline={586},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030545C303030685C303030655C3030305C3034305C303030735C3030306F5C3030306C5C303030655C3030306E5C3030306F5C303030695C30303064} \@writefile{lof}{\contentsline {figure}{\numberline {5}{\ignorespaces Coordinate conventions of the CMS illustrating the use of \(\miteta \) and \(\mitphi \). The Z axis is in beam direction. Taken from https://inspirehep.net/record/1236817/plots\relax }}{9}{figure.caption.6}\protected@file@percent } \newlabel{fig:cmscoords}{{5}{9}{Coordinate conventions of the CMS illustrating the use of \(\eta \) and \(\phi \). The Z axis is in beam direction. Taken from https://inspirehep.net/record/1236817/plots\relax }{figure.caption.6}{}} \@writefile{toc}{\contentsline {subsubsection}{\numberline {3.2.2}The tracking system}{9}{subsubsection.3.2.2}\protected@file@percent } \newlabel{the-tracking-system}{{3.2.2}{9}{The tracking system}{subsubsection.3.2.2}{}} \@writefile{toc}{\contentsline {subsubsection}{\numberline {3.2.3}The electromagnetic calorimeter}{9}{subsubsection.3.2.3}\protected@file@percent } \newlabel{the-electromagnetic-calorimeter}{{3.2.3}{9}{The electromagnetic calorimeter}{subsubsection.3.2.3}{}} \@writefile{toc}{\contentsline {subsubsection}{\numberline {3.2.4}The hadronic calorimeter}{9}{subsubsection.3.2.4}\protected@file@percent } \newlabel{the-hadronic-calorimeter}{{3.2.4}{9}{The hadronic calorimeter}{subsubsection.3.2.4}{}} \BKM@entry{id=15,dest={73756273756273656374696F6E2E332E322E36},srcline={594},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030545C303030685C303030655C3030305C3034305C3030306D5C303030755C3030306F5C3030306E5C3030305C3034305C303030735C303030795C303030735C303030745C303030655C3030306D} \BKM@entry{id=16,dest={73756273756273656374696F6E2E332E322E37},srcline={603},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030545C303030685C303030655C3030305C3034305C303030545C303030725C303030695C303030675C303030675C303030655C303030725C3030305C3034305C303030735C303030795C303030735C303030745C303030655C3030306D} \BKM@entry{id=17,dest={73756273756273656374696F6E2E332E322E38},srcline={617},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030545C303030685C303030655C3030305C3034305C303030505C303030615C303030725C303030745C303030695C303030635C3030306C5C303030655C3030305C3034305C303030465C3030306C5C3030306F5C303030775C3030305C3034305C303030615C3030306C5C303030675C3030306F5C303030725C303030695C303030745C303030685C3030306D} \BKM@entry{id=18,dest={73756273656374696F6E2E332E33},srcline={637},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C3030304A5C303030655C303030745C3030305C3034305C303030635C3030306C5C303030755C303030735C303030745C303030655C303030725C303030695C3030306E5C30303067} \@writefile{toc}{\contentsline {subsubsection}{\numberline {3.2.5}The solenoid}{10}{subsubsection.3.2.5}\protected@file@percent } \newlabel{the-solenoid}{{3.2.5}{10}{The solenoid}{subsubsection.3.2.5}{}} \@writefile{toc}{\contentsline {subsubsection}{\numberline {3.2.6}The muon system}{10}{subsubsection.3.2.6}\protected@file@percent } \newlabel{the-muon-system}{{3.2.6}{10}{The muon system}{subsubsection.3.2.6}{}} \@writefile{toc}{\contentsline {subsubsection}{\numberline {3.2.7}The Trigger system}{10}{subsubsection.3.2.7}\protected@file@percent } \newlabel{the-trigger-system}{{3.2.7}{10}{The Trigger system}{subsubsection.3.2.7}{}} \@writefile{toc}{\contentsline {subsubsection}{\numberline {3.2.8}The Particle Flow algorithm}{10}{subsubsection.3.2.8}\protected@file@percent } \newlabel{the-particle-flow-algorithm}{{3.2.8}{10}{The Particle Flow algorithm}{subsubsection.3.2.8}{}} \@writefile{toc}{\contentsline {subsection}{\numberline {3.3}Jet clustering}{10}{subsection.3.3}\protected@file@percent } \newlabel{jet-clustering}{{3.3}{10}{Jet clustering}{subsection.3.3}{}} \abx@aux@cite{ANTIKT} \abx@aux@segm{0}{0}{ANTIKT} \abx@aux@segm{0}{0}{ANTIKT} \@writefile{lof}{\contentsline {figure}{\numberline {6}{\ignorespaces Comparison of the \(k_t\), Cambridge/Aachen, SISCone and anti-\(k_t\) algorithms clustering a sample parton-level event with many random soft \enquote {ghosts}. Taken from \autocite {ANTIKT}\relax }}{11}{figure.caption.7}\protected@file@percent } \newlabel{fig:antiktcomparison}{{6}{11}{Comparison of the \(k_t\), Cambridge/Aachen, SISCone and anti-\(k_t\) algorithms clustering a sample parton-level event with many random soft \enquote {ghosts}. Taken from \autocite {ANTIKT}\relax }{figure.caption.7}{}} \BKM@entry{id=19,dest={73656374696F6E2E34},srcline={682},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C3030304D5C303030655C303030745C303030685C3030306F5C303030645C3030305C3034305C3030306F5C303030665C3030305C3034305C303030615C3030306E5C303030615C3030306C5C303030795C303030735C303030695C30303073} \abx@aux@segm{0}{0}{PREV_RESEARCH} \abx@aux@segm{0}{0}{PREV_RESEARCH} \BKM@entry{id=20,dest={73756273656374696F6E2E342E31},srcline={724},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030535C303030695C303030675C3030306E5C303030615C3030306C5C3030305C3034305C303030615C3030306E5C303030645C3030305C3034305C303030425C303030615C303030635C3030306B5C303030675C303030725C3030306F5C303030755C3030306E5C303030645C3030305C3034305C3030306D5C3030306F5C303030645C303030655C3030306C5C3030306C5C303030695C3030306E5C30303067} \abx@aux@segm{0}{0}{QSTAR_THEORY} \@writefile{toc}{\contentsline {section}{\numberline {4}Method of analysis}{12}{section.4}\protected@file@percent } \newlabel{sec:moa}{{4}{12}{Method of analysis}{section.4}{}} \@writefile{toc}{\contentsline {subsection}{\numberline {4.1}Signal and Background modelling}{12}{subsection.4.1}\protected@file@percent } \newlabel{signal-and-background-modelling}{{4.1}{12}{Signal and Background modelling}{subsection.4.1}{}} \@writefile{lof}{\contentsline {figure}{\numberline {7}{\ignorespaces Combined fit of signal and background on a toy dataset with gaussian errors and a simulated resonance mass of 3 TeV.\relax }}{13}{figure.caption.8}\protected@file@percent } \newlabel{fig:cb_fit}{{7}{13}{Combined fit of signal and background on a toy dataset with gaussian errors and a simulated resonance mass of 3 TeV.\relax }{figure.caption.8}{}} \BKM@entry{id=21,dest={73656374696F6E2E35},srcline={792},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030505C303030725C303030655C303030735C303030655C3030306C5C303030655C303030635C303030745C303030695C3030306F5C3030306E5C3030305C3034305C303030615C3030306E5C303030645C3030305C3034305C303030645C303030615C303030745C303030615C3030305C3034305C303030715C303030755C303030615C3030306C5C303030695C303030745C30303079} \BKM@entry{id=22,dest={73756273656374696F6E2E352E31},srcline={806},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030505C303030725C303030655C303030735C303030655C3030306C5C303030655C303030635C303030745C303030695C3030306F5C3030306E} \@writefile{toc}{\contentsline {section}{\numberline {5}Preselection and data quality}{14}{section.5}\protected@file@percent } \newlabel{preselection-and-data-quality}{{5}{14}{Preselection and data quality}{section.5}{}} \@writefile{toc}{\contentsline {subsection}{\numberline {5.1}Preselection}{14}{subsection.5.1}\protected@file@percent } \newlabel{preselection}{{5.1}{14}{Preselection}{subsection.5.1}{}} \@writefile{lof}{\contentsline {figure}{\numberline {8}{\ignorespaces Number of jet distribution showing the cut at number of jets $\ge $ 2. Left: distribution before the cut. Right: distribution after the cut. 1st row: data from 2016. 2nd row: combined data from 2016, 2017 and 2018. The signal curves are amplified by a factor of 10,000, to be visible.\relax }}{15}{figure.caption.9}\protected@file@percent } \newlabel{fig:njets}{{8}{15}{Number of jet distribution showing the cut at number of jets $\ge $ 2. Left: distribution before the cut. Right: distribution after the cut. 1st row: data from 2016. 2nd row: combined data from 2016, 2017 and 2018. The signal curves are amplified by a factor of 10,000, to be visible.\relax }{figure.caption.9}{}} \@writefile{lof}{\contentsline {figure}{\numberline {9}{\ignorespaces $\mitDelta \miteta $ distribution showing the cut at $\mitDelta \miteta \le 1.3$. Left: distribution before the cut. Right: distribution after the cut. 1st row: data from 2016. 2nd row: combined data from 2016, 2017 and 2018. The signal curves are amplified by a factor of 10,000, to be visible.\relax }}{16}{figure.caption.10}\protected@file@percent } \newlabel{fig:deta}{{9}{16}{$\Delta \eta $ distribution showing the cut at $\Delta \eta \le 1.3$. Left: distribution before the cut. Right: distribution after the cut. 1st row: data from 2016. 2nd row: combined data from 2016, 2017 and 2018. The signal curves are amplified by a factor of 10,000, to be visible.\relax }{figure.caption.10}{}} \@writefile{lof}{\contentsline {figure}{\numberline {10}{\ignorespaces Invariant mass distribution showing the cut at $m_{jj} \ge \SI {1050}{\giga \eV }$. It shows the expected smooth falling functions of the background whereas the signal peaks at the simulated resonance mass. Left: distribution before the cut. Right: distribution after the cut. 1st row: data from 2016. 2nd row: combined data from 2016, 2017 and 2018.\relax }}{17}{figure.caption.11}\protected@file@percent } \newlabel{fig:invmass}{{10}{17}{Invariant mass distribution showing the cut at $m_{jj} \ge \SI {1050}{\giga \eV }$. It shows the expected smooth falling functions of the background whereas the signal peaks at the simulated resonance mass. Left: distribution before the cut. Right: distribution after the cut. 1st row: data from 2016. 2nd row: combined data from 2016, 2017 and 2018.\relax }{figure.caption.11}{}} \BKM@entry{id=23,dest={73756273656374696F6E2E352E32},srcline={922},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030445C303030615C303030745C303030615C3030305C3034305C3030302D5C3030305C3034305C3030304D5C3030306F5C3030306E5C303030745C303030655C3030305C3034305C303030435C303030615C303030725C3030306C5C3030306F5C3030305C3034305C303030435C3030306F5C3030306D5C303030705C303030615C303030725C303030695C303030735C3030306F5C3030306E} \BKM@entry{id=24,dest={73756273756273656374696F6E2E352E322E31},srcline={968},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030535C303030695C303030645C303030655C303030625C303030615C3030306E5C30303064} \@writefile{toc}{\contentsline {subsection}{\numberline {5.2}Data - Monte Carlo Comparison}{18}{subsection.5.2}\protected@file@percent } \newlabel{data---monte-carlo-comparison}{{5.2}{18}{Data - Monte Carlo Comparison}{subsection.5.2}{}} \@writefile{lof}{\contentsline {figure}{\numberline {11}{\ignorespaces Comparision of data with the Monte Carlo simulation. 1st row: data from 2016. 2nd row: combined data from 2016, 2017 and 2018.\relax }}{18}{figure.caption.12}\protected@file@percent } \newlabel{fig:data-mc}{{11}{18}{Comparision of data with the Monte Carlo simulation. 1st row: data from 2016. 2nd row: combined data from 2016, 2017 and 2018.\relax }{figure.caption.12}{}} \@writefile{toc}{\contentsline {subsubsection}{\numberline {5.2.1}Sideband}{19}{subsubsection.5.2.1}\protected@file@percent } \newlabel{sideband}{{5.2.1}{19}{Sideband}{subsubsection.5.2.1}{}} \@writefile{lof}{\contentsline {figure}{\numberline {12}{\ignorespaces Comparison of data with the Monte Carlo simulation in the sideband region. 1st row: data from 2016. 2nd row: combined data from 2016, 2017 and 2018.\relax }}{19}{figure.caption.13}\protected@file@percent } \newlabel{fig:sideband}{{12}{19}{Comparison of data with the Monte Carlo simulation in the sideband region. 1st row: data from 2016. 2nd row: combined data from 2016, 2017 and 2018.\relax }{figure.caption.13}{}} \BKM@entry{id=25,dest={73656374696F6E2E36},srcline={1006},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C3030304A5C303030655C303030745C3030305C3034305C303030735C303030755C303030625C303030735C303030745C303030725C303030755C303030635C303030745C303030755C303030725C303030655C3030305C3034305C303030735C303030655C3030306C5C303030655C303030635C303030745C303030695C3030306F5C3030306E} \BKM@entry{id=26,dest={73756273656374696F6E2E362E31},srcline={1031},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C3030304E5C3030302D5C303030535C303030755C303030625C3030306A5C303030655C303030745C303030745C303030695C3030306E5C303030655C303030735C30303073} \abx@aux@segm{0}{0}{TAU21} \BKM@entry{id=27,dest={73756273656374696F6E2E362E32},srcline={1064},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030445C303030655C303030655C303030705C303030415C3030304B5C30303038} \abx@aux@segm{0}{0}{DEEP_BOOSTED} \@writefile{toc}{\contentsline {section}{\numberline {6}Jet substructure selection}{20}{section.6}\protected@file@percent } \newlabel{jet-substructure-selection}{{6}{20}{Jet substructure selection}{section.6}{}} \@writefile{toc}{\contentsline {subsection}{\numberline {6.1}N-Subjettiness}{20}{subsection.6.1}\protected@file@percent } \newlabel{n-subjettiness}{{6.1}{20}{N-Subjettiness}{subsection.6.1}{}} \abx@aux@segm{0}{0}{DEEP_BOOSTED} \abx@aux@segm{0}{0}{DEEP_BOOSTED} \@writefile{toc}{\contentsline {subsection}{\numberline {6.2}DeepAK8}{21}{subsection.6.2}\protected@file@percent } \newlabel{deepak8}{{6.2}{21}{DeepAK8}{subsection.6.2}{}} \@writefile{lof}{\contentsline {figure}{\numberline {13}{\ignorespaces Comparison of tagger efficiencies, showing, between others, the DeepAK8 and \(\mittau _{21}\) tagger used in this analysis. Taken from \autocite {DEEP_BOOSTED}\relax }}{21}{figure.caption.14}\protected@file@percent } \newlabel{fig:ak8_eff}{{13}{21}{Comparison of tagger efficiencies, showing, between others, the DeepAK8 and \(\tau _{21}\) tagger used in this analysis. Taken from \autocite {DEEP_BOOSTED}\relax }{figure.caption.14}{}} \BKM@entry{id=28,dest={73756273656374696F6E2E362E33},srcline={1117},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C3030304F5C303030705C303030745C303030695C3030306D5C303030695C3030307A5C303030615C303030745C303030695C3030306F5C3030306E} \@writefile{toc}{\contentsline {subsection}{\numberline {6.3}Optimization}{22}{subsection.6.3}\protected@file@percent } \newlabel{sec:opt}{{6.3}{22}{Optimization}{subsection.6.3}{}} \@writefile{lof}{\contentsline {figure}{\numberline {14}{\ignorespaces Significance plots for the deep boosted (left) and N-subjettiness (right) tagger at the 2 TeV masspoint.\relax }}{22}{figure.caption.15}\protected@file@percent } \newlabel{fig:sig}{{14}{22}{Significance plots for the deep boosted (left) and N-subjettiness (right) tagger at the 2 TeV masspoint.\relax }{figure.caption.15}{}} \BKM@entry{id=29,dest={73656374696F6E2E37},srcline={1171},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030535C303030695C303030675C3030306E5C303030615C3030306C5C3030305C3034305C303030655C303030785C303030745C303030725C303030615C303030635C303030745C303030695C3030306F5C3030306E} \BKM@entry{id=30,dest={73756273656374696F6E2E372E31},srcline={1194},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030555C3030306E5C303030635C303030655C303030725C303030745C303030615C303030695C3030306E5C303030745C303030695C303030655C30303073} \@writefile{toc}{\contentsline {section}{\numberline {7}Signal extraction}{23}{section.7}\protected@file@percent } \newlabel{sec:extr}{{7}{23}{Signal extraction}{section.7}{}} \@writefile{toc}{\contentsline {subsection}{\numberline {7.1}Uncertainties}{23}{subsection.7.1}\protected@file@percent } \newlabel{uncertainties}{{7.1}{23}{Uncertainties}{subsection.7.1}{}} \BKM@entry{id=31,dest={73656374696F6E2E38},srcline={1222},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030525C303030655C303030735C303030755C3030306C5C303030745C30303073} \abx@aux@segm{0}{0}{PREV_RESEARCH} \BKM@entry{id=32,dest={73756273656374696F6E2E382E31},srcline={1230},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030325C303030305C303030315C30303036} \gdef \LT@ii {\LT@entry {1}{36.64455pt}\LT@entry {3}{74.98244pt}\LT@entry {1}{70.98048pt}\LT@entry {1}{103.96877pt}\LT@entry {1}{99.29884pt}} \BKM@entry{id=33,dest={73756273756273656374696F6E2E382E312E31},srcline={1291},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030505C303030725C303030655C303030765C303030695C3030306F5C303030755C303030735C3030305C3034305C303030725C303030655C303030735C303030655C303030615C303030725C303030635C30303068} \@writefile{toc}{\contentsline {section}{\numberline {8}Results}{24}{section.8}\protected@file@percent } \newlabel{results}{{8}{24}{Results}{section.8}{}} \@writefile{toc}{\contentsline {subsection}{\numberline {8.1}2016}{24}{subsection.8.1}\protected@file@percent } \newlabel{section}{{8.1}{24}{2016}{subsection.8.1}{}} \newlabel{tbl:res2016}{{2}{24}{2016}{table.2}{}} \@writefile{lot}{\contentsline {table}{\numberline {2}{\ignorespaces Mass limits found using the data collected in 2016\relax }}{24}{table.2}\protected@file@percent } \@writefile{toc}{\contentsline {subsubsection}{\numberline {8.1.1}Previous research}{24}{subsubsection.8.1.1}\protected@file@percent } \newlabel{previous-research}{{8.1.1}{24}{Previous research}{subsubsection.8.1.1}{}} \@writefile{lof}{\contentsline {figure}{\numberline {15}{\ignorespaces Results of the cross section limits for 2016 using the $\mittau _{21}$ tagger (left) and the deep boosted tagger (right).\relax }}{25}{figure.caption.16}\protected@file@percent } \newlabel{fig:res2016}{{15}{25}{Results of the cross section limits for 2016 using the $\tau _{21}$ tagger (left) and the deep boosted tagger (right).\relax }{figure.caption.16}{}} \abx@aux@segm{0}{0}{PREV_RESEARCH} \abx@aux@segm{0}{0}{PREV_RESEARCH} \BKM@entry{id=34,dest={73756273656374696F6E2E382E32},srcline={1322},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030435C3030306F5C3030306D5C303030625C303030695C3030306E5C303030655C303030645C3030305C3034305C303030645C303030615C303030745C303030615C303030735C303030655C30303074} \gdef \LT@iii {\LT@entry {1}{36.64455pt}\LT@entry {3}{74.98244pt}\LT@entry {1}{70.98048pt}\LT@entry {1}{103.96877pt}\LT@entry {1}{99.29884pt}} \abx@aux@segm{0}{0}{PREV_RESEARCH} \BKM@entry{id=35,dest={73756273656374696F6E2E382E33},srcline={1377},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030435C3030306F5C3030306D5C303030705C303030615C303030725C303030695C303030735C3030306F5C3030306E5C3030305C3034305C3030306F5C303030665C3030305C3034305C303030745C303030615C303030675C303030675C303030655C303030725C30303073} \@writefile{lof}{\contentsline {figure}{\numberline {16}{\ignorespaces Previous results of the cross section limits for q\discretionary {\tmspace +\thinmuskip {.1667em}\TU/latinmodern-math.otf(2)/m/n/12 \char 2}{}{} decaying to qW (left) and q\discretionary {\tmspace +\thinmuskip {.1667em}\TU/latinmodern-math.otf(2)/m/n/12 \char 2}{}{} decaying to qZ (right). Taken from \cite {PREV_RESEARCH}.\relax }}{26}{figure.caption.17}\protected@file@percent } \newlabel{fig:prev}{{16}{26}{Previous results of the cross section limits for q\* decaying to qW (left) and q\* decaying to qZ (right). Taken from \cite {PREV_RESEARCH}.\relax }{figure.caption.17}{}} \@writefile{toc}{\contentsline {subsection}{\numberline {8.2}Combined dataset}{26}{subsection.8.2}\protected@file@percent } \newlabel{combined-dataset}{{8.2}{26}{Combined dataset}{subsection.8.2}{}} \@writefile{lot}{\contentsline {table}{\numberline {3}{\ignorespaces Mass limits found using the data collected in 2016 - 2018\relax }}{26}{table.3}\protected@file@percent } \@writefile{lof}{\contentsline {figure}{\numberline {17}{\ignorespaces Results of the cross section limits for the three combined years using the $\mittau _{21}$ tagger (left) and the deep boosted tagger (right).\relax }}{27}{figure.caption.18}\protected@file@percent } \newlabel{fig:resCombined}{{17}{27}{Results of the cross section limits for the three combined years using the $\tau _{21}$ tagger (left) and the deep boosted tagger (right).\relax }{figure.caption.18}{}} \@writefile{toc}{\contentsline {subsection}{\numberline {8.3}Comparison of taggers}{28}{subsection.8.3}\protected@file@percent } \newlabel{comparison-of-taggers}{{8.3}{28}{Comparison of taggers}{subsection.8.3}{}} \@writefile{lof}{\contentsline {figure}{\numberline {18}{\ignorespaces Comparison of expected limits of the different taggers using different datasets. Left: decay to qW. Right: decay to qZ\relax }}{28}{figure.caption.19}\protected@file@percent } \newlabel{fig:limit_comp}{{18}{28}{Comparison of expected limits of the different taggers using different datasets. Left: decay to qW. Right: decay to qZ\relax }{figure.caption.19}{}} \@writefile{lof}{\contentsline {figure}{\numberline {19}{\ignorespaces Comparision of deep boosted and N-subjettiness tagger in the high purity category using the data from year 2018.\relax }}{29}{figure.caption.20}\protected@file@percent } \newlabel{fig:comp_2018}{{19}{29}{Comparision of deep boosted and N-subjettiness tagger in the high purity category using the data from year 2018.\relax }{figure.caption.20}{}} \BKM@entry{id=36,dest={73656374696F6E2E39},srcline={1428},srcfile={2E2F7468657369732E746578}}{5C3337365C3337375C303030535C303030755C3030306D5C3030306D5C303030615C303030725C30303079} \@writefile{toc}{\contentsline {section}{\numberline {9}Summary}{30}{section.9}\protected@file@percent } \newlabel{summary}{{9}{30}{Summary}{section.9}{}} \gdef \LT@iv {\LT@entry {1}{63.6504pt}\LT@entry {1}{83.9922pt}\LT@entry {1}{90.6504pt}\LT@entry {1}{91.98048pt}\LT@entry {1}{77.99806pt}} \gdef \LT@v {\LT@entry {1}{63.6504pt}\LT@entry {1}{83.9922pt}\LT@entry {1}{90.6504pt}\LT@entry {1}{91.98048pt}\LT@entry {1}{77.99806pt}} \gdef \LT@vi {\LT@entry {1}{63.6504pt}\LT@entry {1}{83.9922pt}\LT@entry {1}{90.6504pt}\LT@entry {1}{91.98048pt}\LT@entry {1}{77.99806pt}} \newlabel{appendix}{{9}{33}{Appendix}{section*.22}{}} \@writefile{lot}{\contentsline {table}{\numberline {4}{\ignorespaces Cross Section limits using 2016 data and the N-subjettiness tagger for the decay to qW\relax }}{33}{table.4}\protected@file@percent } \@writefile{lot}{\contentsline {table}{\numberline {5}{\ignorespaces Cross Section limits using 2016 data and the deep boosted tagger for the decay to qW\relax }}{33}{table.5}\protected@file@percent } \@writefile{lot}{\contentsline {table}{\numberline {6}{\ignorespaces Cross Section limits using 2016 data and the N-subjettiness tagger for the decay to qZ\relax }}{33}{table.6}\protected@file@percent } \gdef \LT@vii {\LT@entry {1}{63.6504pt}\LT@entry {1}{83.9922pt}\LT@entry {1}{90.6504pt}\LT@entry {1}{91.98048pt}\LT@entry {1}{77.99806pt}} \gdef \LT@viii {\LT@entry {1}{63.6504pt}\LT@entry {1}{83.9922pt}\LT@entry {1}{90.6504pt}\LT@entry {1}{91.98048pt}\LT@entry {1}{77.99806pt}} \@writefile{lot}{\contentsline {table}{\numberline {7}{\ignorespaces Cross Section limits using 2016 data and deep boosted tagger for the decay to qZ\relax }}{34}{table.7}\protected@file@percent } \@writefile{lot}{\contentsline {table}{\numberline {8}{\ignorespaces Cross Section limits using the combined data and the N-subjettiness tagger for the decay to qW\relax }}{34}{table.8}\protected@file@percent } \gdef \LT@ix {\LT@entry {1}{63.6504pt}\LT@entry {1}{83.9922pt}\LT@entry {1}{90.6504pt}\LT@entry {1}{91.98048pt}\LT@entry {1}{77.99806pt}} \gdef \LT@x {\LT@entry {1}{63.6504pt}\LT@entry {1}{83.9922pt}\LT@entry {1}{90.6504pt}\LT@entry {1}{91.98048pt}\LT@entry {1}{77.99806pt}} \@writefile{lot}{\contentsline {table}{\numberline {9}{\ignorespaces Cross Section limits using the combined data and the deep boosted tagger for the decay to qW\relax }}{35}{table.9}\protected@file@percent } \@writefile{lot}{\contentsline {table}{\numberline {10}{\ignorespaces Cross Section limits using the combined data and the N-subjettiness tagger for the decay to qZ\relax }}{35}{table.10}\protected@file@percent } \gdef \LT@xi {\LT@entry {1}{63.6504pt}\LT@entry {1}{83.9922pt}\LT@entry {1}{90.6504pt}\LT@entry {1}{91.98048pt}\LT@entry {1}{77.99806pt}} \abx@aux@refcontextdefaultsdone \abx@aux@defaultrefcontext{0}{LHC}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{QSTAR_THEORY}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{CMS_REPORT}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{PARTICLE_FLOW}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{ANTIKT}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{PREV_RESEARCH}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{SUC_COMBINATION}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{LHC_MACHINE}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{SDM}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{DEEP_BOOSTED}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{MONTECARLO}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{CMS_PLOT}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{PARTICLE_PHYSICS}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{TAU21}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{CMS_TRIGGER}{nty/global//global/global} \abx@aux@defaultrefcontext{0}{HADRONIZATION}{nty/global//global/global} \@writefile{lot}{\contentsline {table}{\numberline {11}{\ignorespaces Cross Section limits using the combined data and deep boosted tagger for the decay to qZ\relax }}{36}{table.11}\protected@file@percent }