Investigating binary-neutron-star mergers as production sites of high-energy neutrinos
Year: 2025
Type: article
Abstract: The end state of binary-neutron-star (BNS) mergers can manifest conditions to produce high-energy neutrinos. Inspired by the event GW170817, detected in gravitational waves and in optical/infrared emission, we investigate a scenario in which cosmic-ray (CR) particles are accelerated, in a population of BNS mergers, in the energy range that might contribute from the knee to the ankle of the CR measured spectrum. By taking into account the measured thermal and non-thermal energy density of the photon fields in the source environment as a function of the time after the merger, we model the CR interactions and the consequent neutrino production. We propagate the escaped CR and neutrino fluxes through the extragalactic space and compare the expected diffuse fluxes to the experimental data and current limits. Depending on the CR spectral and composition parameters at acceleration, and on the possible contribution to the sub-ankle CR flux, we discuss the predicted diffuse neutrino flux associated to this class of astrophysical objects, as a function of the details of the photon field characterizing the merger stage, including its evolution in time. We constrain the fraction of accelerated baryons in the source site given the BNS merger rate per volume, taking into account at the same time the constraints from the measured CR and neutrino fluxes.
Authors: S. Rossoni, D. Boncioli, G. Sigl
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
Estimated APC paid: $3,290
Awards: Verbundprojekt 05A2023 - AUGER: Das Pierre-Auger-Projekt: Erdgebundene Messung der kosmischen Strahlung höchster Energien bis über 10^20 eV. Teilprojekt 2., Verbundprojekt 05A2020 - AUGER: Das Pierre-Auger-Projekt:Messungen der kosmischen Energien von über 10^(20) eV. Teilprojekt 4, G7463224461
OpenAlex ID: W4406170193