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@INPROCEEDINGS{Cavasonza:316740,
      author       = {Cavasonza, Leila Ali and Krämer, Michael and Pellen,
                      Mathieu},
      title        = {{E}xploring {D}ark {M}atter with {AMS}-02 through
                      {E}lectroweak {C}orrections},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2017-00138},
      isbn         = {978-3-935702-43-0},
      series       = {DESY-PROC},
      pages        = {96-99},
      year         = {2015},
      comment      = {Cavasonza, Leila Ali "Exploring Dark Matter with AMS-02
                      through Electroweak Corrections" in Proceedings, 11th Patras
                      Workshop on Axions, WIMPs and WISPs (Axion-WIMP 2015) /
                      Irastorza, Igor G., Redondo, Javier, Carmona, José Manuel,
                      Cebrian, Susana, Dafni, Theopisti, Iguaz, Francisco J.,
                      Luzon, Gloria (eds.), Verlag Deutsches
                      Elektronen-Synchrotron : 2015 ; AXION-WIMP 2015 : 11th
                      Patras Workshop on Axions, WIMPs and WISPs, 2015-06-22 -
                      2015-06-26, Zaragoza},
      booktitle     = {Cavasonza, Leila Ali "Exploring Dark
                       Matter with AMS-02 through Electroweak
                       Corrections" in Proceedings, 11th
                       Patras Workshop on Axions, WIMPs and
                       WISPs (Axion-WIMP 2015) / Irastorza,
                       Igor G., Redondo, Javier, Carmona,
                       José Manuel, Cebrian, Susana, Dafni,
                       Theopisti, Iguaz, Francisco J., Luzon,
                       Gloria (eds.), Verlag Deutsches
                       Elektronen-Synchrotron : 2015 ;
                       AXION-WIMP 2015 : 11th Patras Workshop
                       on Axions, WIMPs and WISPs, 2015-06-22
                       - 2015-06-26, Zaragoza},
      abstract     = {The AMS-02 experiment is now measuring charged cosmic rays
                      fluxes with an unprecedented precision. It is thus necessary
                      to provide appropriate and complementary predictions for
                      dark matter signals. To that end, computing electroweak
                      corrections to the dark matter annihilation is an important
                      task. It is particularly relevant for leptophilic models
                      where anti-protons can be produced through the decay of
                      massive gauge bosons. From the lack of particular spectral
                      features in the AMS positron flux, we derive new model
                      independent upper limits on the annihilation cross section.
                      In particular we use a newly introduced background function
                      that allows to set limits using all the energy spectrum
                      probed by AMS-02. This is particularly interesting as
                      important phenomena such as solar modulation take place at
                      low energy. Using a new calculation of electroweak radiation
                      for vector dark matter annihilation, we can predict the
                      maximum flux of anti-protons in such leptophilic scenarios,
                      to be compared with future AMS measurments.},
      month         = {Jun},
      date          = {2015-06-22},
      organization  = {11th Patras Workshop on Axions, WIMPs
                       and WISPs, Zaragoza (Spain), 22 Jun
                       2015 - 26 Jun 2015},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.3204/DESY-PROC-2015-02/pellen_mathieu},
      url          = {https://bib-pubdb1.desy.de/record/316740},
}