Ducci L, Perinati E, Romano P, Vercellone S, Nikołajuk M, Santangelo A, Sasaki M (2025)
Publication Type: Journal article
Publication year: 2025
Book Volume: 701
Article Number: A98
DOI: 10.1051/0004-6361/202555242
We explored the expected properties of the neutrino emission from accreting neutron stars in X-ray binaries using numerical simulations. The simulations are based on a model in which neutrinos are produced by the decay of charged pions and kaons, generated in inelastic collisions between protons accelerated up to TeV energies in the magnetosphere of a magnetized (B ∼ 1012 G) neutron star and protons of the accretion disc. Our results show that this process can produce strong neutrino emission up to a few tens of TeV when the X-ray luminosity is above ∼1039 erg s-1, as in ultra-luminous X-ray (ULX) pulsars. We show that neutrinos from a transient Galactic ULX pulsar with Lx ≈ 5 × 1039 erg s-1 can be detected with kilometre-scale detectors such as IceCube if the source is within about 3-4 kpc. We also derived an upper limit on the neutrino flux from the Galactic ULX pulsar Swift J0243.6+6124 using IceCube data, a result that has not been previously reported. Our findings establish a new benchmark for future astrophysical neutrino observations, critical for interpreting data from current and upcoming instruments with significantly improved sensitivity.
APA:
Ducci, L., Perinati, E., Romano, P., Vercellone, S., Nikołajuk, M., Santangelo, A., & Sasaki, M. (2025). Ultra-luminous X-ray pulsars as sources of TeV neutrinos. Astronomy & Astrophysics, 701. https://doi.org/10.1051/0004-6361/202555242
MLA:
Ducci, L., et al. "Ultra-luminous X-ray pulsars as sources of TeV neutrinos." Astronomy & Astrophysics 701 (2025).
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