  We have performed our data analysis of the observations by Swift and Fermi
satellites in order to probe the induced gravitational collapse (IGC) paradigm
for GRBs associated with supernovae (SNe), in the "terra incognita" of GRB
130427A. We compare and contrast our data analysis with those in the
literature. We have verified that the GRB 130427A conforms to the IGC paradigm
by examining the power law behavior of the luminosity in the early $10^4$ s of
the Swift-XRT observations. This has led to the successful prediction of the
occurrence of SN 2013cq and to the identification of the four different
episodes of the "binary driven hypernovae" (BdHNe). The exceptional quality of
the data has allowed the identification of novel features in Episode 3
including: a) the confirmation and the extension of the existence of the
recently discovered "nested structure" in the late X-ray luminosity in GRB
130427A, as well as the identification of a spiky structure at $10^2$ s in the
cosmological rest-frame of the source; b) a power law emission of the GeV
luminosity light curve and its onset at the end of Episode 2 c) different
Lorentz $\Gamma$ factors for the emitting regions of the X-ray and GeV
emissions in this Episode 3. These results make it possible to test the details
of the physical and astrophysical regimes at work in the BdHNe: 1) a newly born
neutron star and the supernova ejecta, originating in Episode 1, 2) a newly
formed black hole originating in Episode 2, and 3) the possible interaction
among these components, observable in the standard features of Episode 3.
