TAMBO and Cosmic-Ray Opportunities of the TAMBITO Demonstrator Array

Not scheduled
20m
Itaca Hall (Sorrento)

Itaca Hall

Sorrento

Ulisse Deluxe Hostel Via del Mare, 22 - 80067 Sorrento – Napoli – Italy
Oral Astrophysical Neutrinos

Speaker

Jeffrey Lazar (Université Catholique de Louvain)

Description

While IceCube has measured the flux of astrophysical neutrinos at energies up to several PeV, much remains to be discovered regarding their origin and nature. The Tau Air-Shower Mountain-Based Observatory (TAMBO), comprising 5000 particle detectors deployed in a steep valley, offers a cost-effective method for detecting supra-PeV neutrinos. TAMBO is specifically designed to detect tau neutrinos in the energy range from 1 PeV to 100 PeV, where tau neutrinos are a smoking gun signature of astrophysical neutrinos. As a stepping stone toward the full detector, the TAMBITO array is a 100-detector-scale demonstrator intended for deployment in the Peruvian Colca Valley. In this contribution, I will present the status of the TAMBO detector and explore potential cosmic ray studies that TAMBITO's unique geometry will enable.

Author

Jeffrey Lazar (Université Catholique de Louvain)

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