eng URI http://hdl.handle.net/10795/3021 φυσικές και εφαρμοσμένες επιστήμες πυρηνική φυσική στοιχειώδη σωματίδια ραδιενέργεια αστρονομία We present some results on the radiative signatures of the one zone hadronic model. For this we have solved five spatially averaged, time-dependent coupled kinetic equations which describe the evolution of relativistic protons, electrons, photons, neutrons and neutrinos in a spherical volume containing a magnetic field. Protons are injected and lose energy by synchrotron, photopair and photopion production. We model photopair and photopion using the results of relevant MC codes, like the SOPHIA code in the case of photopion, which give accurate description for the injection of secondaries which then become source functions in their respective equations. This approach allows us to calculate the expected photon and neutrino spectra simultaneously in addition to examining questions like the efficiency and the temporal behaviour of the hadronic models. 6 pp. LOMv1.0 creator LOMv1.0 publisher LOMv1.0 Scientific Coordinator LOMv1.0 Project Executing Organisation 2011-12-14 Digital Library of the Operational Programme "Education and Lifelong Learning" abstract types Text Radiation mechanisms: non-thermal Radiative transfer Galaxies: active 109564 application/pdf http://repository.edulll.gr/edulll/bitstream/10795/3021/2/3021_1.41_%ce%94%ce%97%ce%9c_20_12_12.pdf arXiv:1112.3029v1 [astro-ph.HE] URI http://hdl.handle.net/10795/3021 LOMv1.0creator 2016-05-05T10:50:19Z LOMv1.0validator 2016-05-05T10:50:19Z LOMv1.0 gre no no Copyright EYD-EPEDBM (Operational Programme "Education and Lifelong Learning")