  The radio galaxy IC310 located in the Perseus Cluster is one of the brightest
objects in the radio and X-ray bands, and one of the closest active galactic
nuclei observed in very-high energies. In GeV - TeV $\gamma$-rays, IC310 was
detected in low and high flux states by the MAGIC telescopes from October 2009
to February 2010. Taking into account that the spectral energy distribution
(SED) up to a few GeV seems to exhibit a double-peak feature and that a
single-zone synchrotron self-Compton (SSC) model can explain all of the
multiwavelength emission except for the non-simultaneous MAGIC emission, we
interpret, in this work, the multifrequency data set of the radio galaxy IC310
in the context of homogeneous hadronic and leptonic models. In the leptonic
framework, we present a multi-zone SSC model with two electron populations to
explain the whole SED whereas for the hadronic model, we propose that a
single-zone SSC model describes the SED up to a few GeVs and neutral pion decay
products resulting from p$\gamma$ interactions could describe the TeV - GeV
$\gamma$-ray spectra. These interactions occur when Fermi-accelerated protons
interact with the seed photons around the SSC peaks. We show that, in the
leptonic model the minimum Lorentz factor of second electron population is
exceedingly high $\gamma_e\sim10^5$ disfavoring this model, and in the hadronic
model the required proton luminosity is not extremely high $\sim 10^{44}$
erg/s, provided that charge neutrality between the number of electrons and
protons is given. Correlating the TeV $\gamma$-ray and neutrino spectra through
photo-hadronic interactions, we find that the contribution of the emitting
region of IC310 to the observed neutrino and ultra-high-energy cosmic ray
fluxes are negligible.
