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A Study of Diffractive Scattering with the ATLAS and ALFA Experiment

This thesis presents a study of diffractive scattering of high-energy protons. Hadronic diffraction is not well-understood and many alternative approaches exist. The Monte Carlo event generator Pythia 8 follows a Pomeron-based approach, where the invariant mass of the diffractive system and the squa...

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Detalles Bibliográficos
Autor principal: Lind, Alexander Pedersen
Lenguaje:eng
Publicado: 2017
Materias:
Acceso en línea:http://cds.cern.ch/record/2275644
Descripción
Sumario:This thesis presents a study of diffractive scattering of high-energy protons. Hadronic diffraction is not well-understood and many alternative approaches exist. The Monte Carlo event generator Pythia 8 follows a Pomeron-based approach, where the invariant mass of the diffractive system and the squared momentum transfer $t$ of the system is set up according to a phenomenological Pomeron flux parameterization, which is parameterized by the super-critical Pomeron trajectory, $\alpha(t) = 1 + \varepsilon + \alpha' t$, where the intercept parameter $\varepsilon$ and the slope parameter $\alpha'$ can be tuned by the user. A fast detector response simulation of the ALFA and ATLAS detectors has been developed in the Rivet toolkit for the purposes of this thesis. The developed simulation framework is able to handle the beam transport of diffractively scattered protons as well as impose the kinematic acceptance of the ALFA detector which was found to be approximately $\xi \lesssim 0.22$, with a pseudorapidity coverage of $9 \lesssim |\eta| \lesssim 13$. The simulation framework has been used in a phenomenological study of single diffraction, in order to study observables most sensitive to the Pomeron flux parameters. Using this information, a statistical fit procedure to determine the Pomeron flux parameters $\varepsilon$ and $\alpha'$ has been developed and tested on several generated test samples. Data recorded at $\sqrt{s} = 13$ TeV, $\beta^{*} = 90$ m, and $\theta_{C} = 2\times50 \text{ }\mu\text{rad}$ at the ATLAS experiment in the Run 2 period has been analysed. Several structures in the measured single diffractive distributions are observed in data which are not present in the simulation. An investigation into the possible background sources of these structures is presented.