Production of high-energy neutrinos in binary-neutron-star merger events
High-energy neutral astrophysical messengers, such as neutrinos and photons, can be produced by the interaction of ultra-high-energy cosmic rays (UHECRs) with radiation fields, either during extragalactic propagation or within source environments.Neutrinos and gamma-rays can play a crucial role in the study of acceleration mechanisms of cosmic rays