5 papers
Optimizing the potential of KM3NeT in detecting core-collapse supernovae
KM3NeT Collaboration, O. Adriani, A. Albert +285
Core-collapse supernovae mark the end of life of massive stars. However, despite their importance in astrophysics, their underlying mechanisms remain unclear. Neutrinos that emerge…
Evidence for particle acceleration approaching PeV energies in the W51 complex
The LHAASO Collaboration, Zhen Cao, F. Aharonian +284
The -ray emission from the W51 complex is widely acknowledged to be attributed to the interaction between the cosmic rays (CRs) accelerated by the shock of supernova remnant (S…
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…
Choked jets in BSG/RSG as possible sources of high-energy neutrinos
Matteo Pais, Angela Zegarelli, Silvia Celli +1
The death of massive stars is accompanied by the formation of central and accreting compact objects and the subsequent launch of relativistic jets. However, not all jets successful…
Towards multi-messenger observations of core-collapse supernovae harbouring choked jets
A. Zegarelli, D Guetta, S. Celli +3
Choked jets (CJ) have attracted particular attention as potential sources of high-energy cosmic neutrinos. Testing this hypothesis is challenging because of the missing gamma-ray c…