2025MNRAS.544.2897P

The blazar 3C 454.3 experienced a major flare in 2010 November, making it the brightest $\gamma$-ray source in the sky of the Fermi-Large Area Telescope (LAT). We obtain seven daily consecutive spectral energy distributions (SEDs) of the flare in the infrared, optical, ultraviolet, X-ray, and $\gamma$-ray bands with publicly available data. We simulate the physical conditions in the blazar and show that the observed SEDs are well reproduced in the framework of a 'standing feature' where the position of the emitting region is almost stationary, located beyond the outer radius of the broad-line region and into which fresh blobs of relativistically moving magnetized plasma are continuously injected. Meanwhile, a model with a single 'moving blob' does not describe the data well. We obtain a robust upper limit to the amount of high-energy protons in the jet of 3C 454.3 from the electromagnetic SED. We construct a neutrino light curve of 3C 454.3 and estimate the expected neutrino yield at energies $\ge 100$ TeV for 3C 454.3 to be up to $6 \times 10^{-3}$ $\nu _{\mu }$ per year. Finally, we extrapolate our model findings to the light curves of all Fermi-LAT flat-spectrum radio quasars. We find that next-generation neutrino telescopes are expected to detect approximately one multimessenger ($\gamma + \nu _{\mu }$) flare per year from bright blazars with neutrino peak energy in the hundreds TeV-hundreds PeV energy range and show that the electromagnetic flare peak can precede the neutrino arrival by months to years.