Speaker
Description
Following IceCube’s recent detection of Galactic plane emission, resolving individual Galactic neutrino sources has become an important objective. In this talk, I will present an overview of the current status of Galactic neutrino source searches with IceCube, focusing on the transition from source detection to source identification in the multi-messenger era. I will discuss how observations across different messengers, together with advances in search methodologies and source morphology modelling, can improve our ability to identify the astrophysical origins of Galactic neutrinos.
The presentation will highlight the key challenges in Galactic neutrino source identification, including source confusion, extended emission, and detector limitations, before outlining our group's ongoing work toward morphology-informed searches for neutrino emission from molecular clouds near cosmic-ray accelerators.
| Research Area | Neutrino Physics |
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