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@PHDTHESIS{Rathmann:1013584,
      author       = {Rathmann, Lena Maria},
      othercontributors = {Krämer, Michael and Kahlhöfer, Felix Karl David},
      title        = {{D}ark matter indirect detection and phenomenology of
                      flavored dark matter models},
      school       = {RWTH Aachen University},
      type         = {Dissertation},
      address      = {Aachen},
      publisher    = {RWTH Aachen University},
      reportid     = {RWTH-2025-05621},
      pages        = {1 Online-Ressource : Illustrationen},
      year         = {2025},
      note         = {Veröffentlicht auf dem Publikationsserver der RWTH Aachen
                      University; Dissertation, RWTH Aachen University, 2025},
      abstract     = {Dark matter remains one of the most fascinating puzzles in
                      modern physics, with its existence being well established
                      through a variety of astrophysical observations. However,
                      despite extensive experimental and theoretical efforts, the
                      properties of dark matter remain largely unknown. In this
                      thesis, we contribute to the search for dark matter by
                      studying two different strategies: First, we study indirect
                      detection with cosmic ray antideuterons which can provide
                      insights into the interactions of dark matter with Standard
                      Model particles. Second, we develop dark matter models to
                      help explain the observational evidence and study
                      specifically the phenomenology of flavored dark matter
                      models. In the first part, we investigate the indirect
                      detection of dark matter with cosmic ray antideuterons which
                      are expected to have a much lower background compared to
                      other antiparticles, making them a promising target for dark
                      matter searches. We compute their injection spectrum using
                      Monte Carlo simulations, taking into account the
                      uncertainties that arise from the modeling of the production
                      of antideuterons. We simulate the propagation of
                      antideuterons through the Galaxy using two different
                      propagation models and include the uncertainties of the
                      propagation parameters. The computed antideuteron fluxes are
                      used to develop and train a neural network emulator to
                      predict the antideuteron flux with a significant speed-up
                      compared to simulations. Using the emulator, we investigate
                      the sensitivity of current and future experiments to
                      antideuterons produced in dark matter annihilations. We find
                      that our tool is accurate and efficient and can be used for
                      the interpretation of future antideuteron data in the
                      context of dark matter. In the second part of the thesis we
                      focus on the phenomenology of flavored dark matter models.
                      These models offer a rich phenomenology that can evade
                      current constraints and allow for a more dynamic freeze-out
                      phenomenology. First, we study a flavored Majorana dark
                      matter model with couplings to up-type quarks and focus on
                      more general freeze-out scenarios. We perform detailed scans
                      over the parameter space to obtain viable points that are
                      not excluded by current constraints and find that including
                      coannihilation and conversion processes significantly
                      increases the viable parameter space of the model. The
                      parameter space is then confronted with constraints from a
                      variety of LHC searches, and we discuss possible signatures
                      to distinguish the Majorana dark matter model from the Dirac
                      case. We find that the charge asymmetry in the production of
                      a top quark and a jet is a promising signature. Lastly, we
                      expand the study to include a variety of flavored dark
                      matter models and develop a framework to perform an
                      automated study of the phenomenology of these models. This
                      framework includes all relevant constraints from the relic
                      abundance, direct and indirect detection experiments as well
                      as flavor and collider constraints and allows for a
                      systematic study of the viable parameter space of flavored
                      dark matter models. To demonstrate the capabilities of the
                      framework, we perform a study of a model with couplings to
                      right-handed leptons. We conclude that the phenomenology of
                      the model can be studied very efficiently with this
                      framework and find that it is mostly constrained by the
                      relic abundance and flavor observables.},
      cin          = {136110 / 130000},
      ddc          = {530},
      cid          = {$I:(DE-82)136110_20140620$ / $I:(DE-82)130000_20140620$},
      pnm          = {DFG project G:(GEPRIS)418642100 - Neue flavour-verletzende
                      Wechselwirkungen bei hohen Transversalimpulsen (C3a)
                      (418642100) / TRR 257: Phänomenologische
                      Elementarteilchenphysik nach der Higgs-Entdeckung},
      pid          = {G:(GEPRIS)418642100 / G:(GEPRIS)396021762},
      typ          = {PUB:(DE-HGF)11},
      doi          = {10.18154/RWTH-2025-05621},
      url          = {https://publications.rwth-aachen.de/record/1013584},
}