We present new results on the Jets Driven Feedback Mechanism for powering the explosion of Core-Collapse supernovae (CCSN). We will present new post-bounce simulations using the FLASH hydrodynamic numerical code, which show the effects of jets driven feedback on the supernova explosions.
We show that the Jets Driven Feedback Mechanism can generate enough energy to explode the star.
We investigate the parameters by which the Jets Driven Feedback Mechanism can deposit energy inside the star forming hot bubbles that lead to the explosion.