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@ARTICLE{Cirelli:426970,
      author       = {Cirelli, Marco and Gouttenoire, Yann and Petraki, Kalliopi
                      and Sala, Filippo},
      title        = {{H}omeopathic {D}ark {M}atter, or how diluted heavy
                      substances produce high energy cosmic rays},
      journal      = {Journal of cosmology and astroparticle physics},
      volume       = {02},
      number       = {2},
      issn         = {1475-7516},
      address      = {London},
      publisher    = {IOP},
      reportid     = {PUBDB-2019-03958, arXiv:1811.03608},
      pages        = {014},
      year         = {2019},
      note         = {PIF-2017-72},
      abstract     = {We point out that current and planned telescopes have the
                      potential of probing annihilating Dark Matter (DM) with a
                      mass of O(100) TeV and beyond. As a target for such
                      searches, we propose models where DM annihilates into
                      lighter mediators, themselves decaying into Standard Model
                      (SM) particles. These models allow to reliably compute the
                      energy spectra of the SM final states, and to naturally
                      evade the unitarity bound on the DM mass. Indeed, long-lived
                      mediators may cause an early matter-dominated phase in the
                      evolution of the Universe and, upon decaying, dilute the
                      density of preexisting relics thus allowing for very large
                      DM masses. We compute this dilution in detail and provide
                      results in a ready-to-use form. Considering for concreteness
                      a model of dark U(1) DM, we then study both dilution and the
                      signals at various high energy telescopes observing γ rays,
                      neutrinos and charged cosmic rays. This study enriches the
                      physics case of these experiments, and opens a new
                      observational window on heavy new physics sectors.},
      cin          = {T},
      ddc          = {530},
      cid          = {I:(DE-H253)T-20120731},
      pnm          = {611 - Fundamental Particles and Forces (POF3-611) /
                      PIF-2017-72 - PIER Seed Project: Dark Matter at 10 TeV and
                      beyond, a new goal for cosmic-ray experiments
                      $(2017_IVF-PIF-2017-72)$},
      pid          = {G:(DE-HGF)POF3-611 / $G:(DE-HGF)2017_IVF-PIF-2017-72$},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000458377000003},
      eprint       = {1811.03608},
      howpublished = {arXiv:1811.03608},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:1811.03608;\%\%$},
      doi          = {10.1088/1475-7516/2019/02/014},
      url          = {https://bib-pubdb1.desy.de/record/426970},
}