Description
The IceCube neutrino observatory has a diverse program of dark matter studies searching for neutrinos from self-annihilating and decaying dark matter particles gravitationally clustered in nearby galaxies, the Milky Way, the Sun and the Earth. The future IceCube Upgrade is expected to enhance IceCube's sensitivity for DM studies in the 1-100 GeV mass range. In this contribution we will present updated sensitivities of the IceCube Upgrade for dark matter annihilation and decay in the Galactic dark matter halo.
| Collaboration | The IceCube experiment |
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Primary author
Rikke Stougaard Klausen
(University of Copenhagen)
Co-author
Prof.
Markus Tobias Ahlers
(University of Copenhagen)
