Lepto-Hadronic Scenarios for TeV Extensions of Gamma-Ray Burst Afterglow Spectra
Authors: Marc Klinger (Deutsches Elektronen-Synchrotron DESY, Zeuthen, Germany), Chengchao Yuan (Deutsches Elektronen-Synchrotron DESY, Zeuthen, Germany), Andrew M. Taylor (Deutsches Elektronen-Synchrotron DESY, Zeuthen, Germany), Walter Winter (Deutsches Elektronen-Synchrotron DESY, Zeuthen, Germany)
Abstract: Recent multi-wavelength observations of gamma-ray burst afterglows observed in the TeV energy range challenge the simplest Synchrotron Self-Compton (SSC) interpretation of this emission, and are consistent with a single power-law component spanning over eight orders of magnitude in energy. To interpret this generic behaviour in the single-zone approximation without adding further free parameters, we perform an exhaustive parameter space study using the public, time-dependent, multi-messenger transport software AM3. This description accounts for the radiation from non-thermal protons and the lepto-hadronic cascade induced by pp- and p{\gamma}-interactions. We summarise the main scenarios which we have found (SSC, Extended-syn, Proton-syn, pp-cascade, and p{\gamma}-cascade), and discuss their advantages and limitations. We find that possible high-density environments, as may be typical for surrounding molecular cloud material, offer an alternative explanation for producing flat hard (source) spectra up to and beyond energies of 10 TeV.
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