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most citedComparison of the measured atmospheric muon rate with Monte Carlo simulations and sensitivity study for detection of prompt atmospheric muons with KM3NeT

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astro-ph.HE2025

Ultraviolet radiation and neutrinos: two messengers from CCSNe in the CSM scenario

Silvia Gagliardini, Simone Dall'Osso, Dafne Guetta +4

Massive stars (>8 ) often undergo intense mass loss through winds or eruptive events in the final stages of their evolution, leading to the formation of a dense circumst…