Supernovae and gamma-ray bursts in the induced gravitational collapse paradigm

I review recent progress in the understanding of long, energetic (10⁵²–10⁵⁴ erg) gamma-ray bursts (GRBs) associated to supernovae (SN) Ib/c. This occurrence is explained within the Induced Gravitational Collapse (IGC) paradigm, following the sequence: 1) an initial binary system consists in a compact Iron-Carbon-Oxygen (FeCO) core and a neutron star (NS); 2) the FeCO core explodes, giving origin to a SN, and part of the SN ejecta accretes onto the NS which reaches its criticalmass and collapses to a black hole (BH) giving rise to a long GRB; 3) a new NS (ν-NS) is generated by the SN as a remnant. Observational consequences of this scenario are outlined.