Speaker
Simon Sotirov
(MSU, INR RAS)
Description
We investigate and make theoretical estimates for the neutrino flux above 150 TeV in a scenario with a nearby source in the Cygnus region, the existence of which is motivated by the LHAASO gamma-ray bubble observations. By combining a state-of-the-art model of galactic cosmic rays with the contribution from a local source within the framework of a two-zone diffusion model, we investigate the neutrino signal for anisotropy.
Primary author
Simon Sotirov
(MSU, INR RAS)
