Speaker
Dr
Luis Salvador Miranda
(The Chinese University of Hong Kong)
Description
We discuss the potential sensitivities of next-gen neutrino telescopes in the northern hemisphere, such as KM3NeT ORCA and ARCA on dark matter annihilation in the Galactic halo.
With its energy and angular resolutions, as well as advantages sky coverage taken into account, we show that KM3Net is expected to yield very competitive limits for dark matter annihilations. We also discuss the implications for WIMP and simplified models.
Primary author
Dr
Luis Salvador Miranda
(The Chinese University of Hong Kong)
Co-authors
Dr
Kenny C. Y. Ng
(The Chinese University of Hong Kong)
Dr
Suzan Basegmez du Pree
(Nikhef, National Institute for Subatomic Physics)
Dr
Andrew Cheek
(Astrocent, Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences)
Dr
Chiara Arina
(Institute for Mathematics and Physics, Université catholique de Louvain)
