11–15 Jul 2022
Niels Bohr Institute
Europe/Copenhagen timezone
Zoom room: https://ucph-ku.zoom.us/j/61850277164?pwd=bW9yN3ltTkFXOXRacjNBSUYvWHZYZz09

Dark Matter decay to neutrinos

12 Jul 2022, 14:36
12m
Auditorium A (NBI)

Auditorium A

NBI

Speaker

Diyaselis Delgado (Harvard University)

Description

Dark matter (DM) particles are predicted to decay into Standard Model particles which would produce signals of neutrinos, gamma-rays, and other secondary particles. Neutrinos provide an avenue to probe astrophysical sources of DM particles. We review the decay of dark matter into neutrinos over a range of dark matter masses from MeV/c2 to ZeV/c2. We examine the expected contributions to the neutrino flux at current and upcoming neutrino and gamma-ray experiments, such as Hyper-Kamiokande, DUNE, CTA, TAMBO, and IceCube Gen-2. We consider galactic and extragalactic signals of decay processes into neutrino pairs, yielding constraints on the dark matter decay lifetime that ranges from tau ∼ 1.2×10^21 s at 10 MeV/c2 to 1.5x10^29 s at 1 PeV/c2.

Primary author

Diyaselis Delgado (Harvard University)

Presentation materials