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@PHDTHESIS{Brinckmann:766448,
      author       = {Brinckmann, Thejs},
      othercontributors = {Lesgourgues, Julien and Mertsch, Philipp},
      title        = {{I}nsight on the dark universe from cosmological
                      perturbations},
      school       = {RWTH Aachen University},
      type         = {Dissertation},
      address      = {Aachen},
      reportid     = {RWTH-2019-08078},
      pages        = {1 Online-Ressource (vi, 196 Seiten) : Illustrationen,
                      Diagramme},
      year         = {2018},
      note         = {Veröffentlicht auf dem Publikationsserver der RWTH Aachen
                      University 2019; Dissertation, RWTH Aachen University, 2018},
      abstract     = {Cosmology presents the best hope of measuring the sum of
                      neutrino masses in the future. The Cosmic Microwave
                      Background (CMB) has already been a treasure trove of
                      information; from Planck, BICEP/KECK, and their
                      predecessors; and will continue to provide ever more precise
                      information with upcoming or proposed CMB experiments, such
                      as LiteBird, CMB-S4, CORE and PICO. These missions will have
                      great synergy with other branches of cosmology. In
                      particular, massive neutrinos leave a distinct imprint on
                      the matter distribution of the universe, which upcoming
                      large-scale structure experiments such as Euclid and the
                      Square Kilometre Array will observe with unprecedented
                      levels of precision. The uncertainty in modelling of
                      non-linear structure formation is often neglected in other
                      forecasts, or scales corresponding to this regime are
                      entirely removed. In this work, we take into account that
                      our understanding of non-linear modelling is imperfect. We
                      show that a neutrino mass sum measurement is all but
                      guaranteed from cosmology in the next decade and that this
                      statement is robust to choice of cosmological model or
                      modelling of non-linear effects.},
      cin          = {139610 / 130000},
      ddc          = {530},
      cid          = {$I:(DE-82)139610_20160614$ / $I:(DE-82)130000_20140620$},
      typ          = {PUB:(DE-HGF)11},
      doi          = {10.18154/RWTH-2019-08078},
      url          = {https://publications.rwth-aachen.de/record/766448},
}