SKA-Phase 1 sensitivity to synchrotron radio emission from multi-TeV Dark Matter candidates

@article{Cembranos2019SKAPhase1S,
  title={SKA-Phase 1 sensitivity to synchrotron radio emission from multi-TeV Dark Matter candidates},
  author={Jos{\'e} Alberto Ruiz Cembranos and Alvaro de la Cruz-Dombriz and V. Gammaldi and Miguel Mendez-Isla},
  journal={arXiv: High Energy Physics - Phenomenology},
  year={2019}
}
In the era of radio astronomy, the high sensitivity of the Square Kilometre Array (SKA) could play a decisive role in the detection of new radio sources. In this work, we study the SKA sensitivity to the synchrotron radio emission expected by the annihilation of TeV DM candidate in the Draco dwarf spheroidal galaxy. On the one hand, we consider model-independent DM candidates: we find out that with 1000 hours of data-taking, SKA1-MID will be able to exclude up to 10 TeV thermal DM candidates… 
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