{ "id": "1502.03950", "version": "v1", "published": "2015-02-13T11:39:28.000Z", "updated": "2015-02-13T11:39:28.000Z", "title": "Time Dependent Hadronic Modeling of Flat Spectrum Radio Quasars", "authors": [ "Christopher Diltz", "Markus Boettcher", "Giovanni Fossati" ], "comment": "Accepted for publication in The Astrophysical Journal", "categories": [ "astro-ph.HE" ], "abstract": "We introduce a new time-dependent lepto-hadronic model for blazar emission that takes into account the radiation emitted by secondary particles, such as pions and muons, from photo hadronic interactions. Starting from a baseline parameter set guided by a fit to the spectral energy distribution of the blazar 3C 279, we perform a parameter study to investigate the effects of perturbations of the input parameters to mimic different flaring events to study the resulting lightcurves in the optical, X-ray, high energy (HE: E > 100 MeV) and very-high-energy (VHE: E > 100 GeV) gamma-rays as well as the neutrino emission associated with charged-pion and muon decay. We find that flaring events from an increase in the efficiency of Fermi II acceleration will produce a positive correlation between all bandpasses and a marked plateau in the HE gamma-ray lightcurve. We also predict a distinctive dip in the HE lightcurve for perturbations caused by a change in the proton injection spectral index. These plateaus / dips could be a tell tale signature of hadronic models for perturbations that lead to more efficient acceleration of high energy protons in parameter regimes where pion and muon synchrotron emission is non-negligible.", "revisions": [ { "version": "v1", "updated": "2015-02-13T11:39:28.000Z" } ], "analyses": { "keywords": [ "flat spectrum radio quasars", "time dependent hadronic modeling", "proton injection spectral index", "high energy", "photo hadronic interactions" ], "publication": { "doi": "10.1088/0004-637X/802/2/133" }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1344756 } } }