Fechas: 31 de marzo - 1 de abril, 2022.
Lugar: Sala de Claustros, Facultad de Ciencias (Universidad de Granada).
Contacto: Sergio Navas (Dpto. Física Teórica y del Cosmos, UGR).
The goal of the workshop is to bring together experts on indirect detection of dark matter with neutrinos from different experiments: IceCube, KM3NeT, ANTARES, GVD... as well as phenomenologists and theoreticians to discuss the latest advances and future avenues on the indirect detection of dark matter with neutrinos. The following topics will be covered:
- Where do we stand? Summary of recent dark matter searches by different experiments
- Detector parameters: effective volumes/areas, how we calculate them, etc.
- Signal Monte Carlos: what simulation framework and parameters are we using
- Where to look for dark matter (pros/cons): Earth, dwarf galaxies, galaxy clusters...
- New backgrounds, solar atmospheric neutrinos
- Planned low energy extensions
