Probing photon-ALP oscillations from the MAGIC observations of FSRQ QSO B1420+326
arXiv:2310.16634 · doi:10.1103/PhysRevD.109.023011
Abstract
At the beginning of 2020, MAGIC reported a very-high-energy (VHE) flaring activity from the FSRQ QSO B1420+326. It is now the fourth known most distant blazar (z=0.682) with an observed VHE gamma-ray emission. In this work, we investigate the effect of photon-axionlike particle (ALP) oscillations in the gamma-ray spectra measured by Fermi-LAT and MAGIC around the flaring state. We set 95% C.L. upper limit on the ALP parameters and obtain a constraint on the photon-ALP coupling constant GeV for ALP masses eV. Assuming the hadronic origin of VHE photons, we also estimate the expected neutrino flux from this source and the contribution to diffuse neutrino flux from QSO B1420+326-like FSRQs at sub-PeV energies. Furthermore, we study the implications of photon-ALP oscillations on the counterpart -rays of the sub-PeV neutrinos. Finally, we investigate a viable scenario of invisible neutrino decay to ALPs on the gamma-ray spectra and diffuse -ray flux at sub-PeV energies. Interestingly, we find that for the choice of neutrino lifetime s eV, the -ray flux has a good observational sensitivity towards LHAASO-KM2A.
arXiv comment11 pages, 7 figures; Published version
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