Recipes to energize core-collapse supernova explosions

          @misc{ scivideos_PIRSA:11060021,
            doi = {10.48660/11060021},
            url = {https://pirsa.org/11060021},
            author = {},
            keywords = {Particle Physics},
            language = {en},
            title = {Recipes to energize core-collapse supernova explosions},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2011},
            month = {jun},
            note = {PIRSA:11060021 see, \url{https://scivideos.org/index.php/pirsa/11060021}}
          }
          

Abstract

Recent multidimensional supernova simulations seem to support an assumption that the neutrino-driven mechanism might work to blow up massive stars. However the explosion energies obtained in those simulations are usually not enough to account for the canonical explosion energy of 10^51 ergs. In this contribution we'd like to address whether some new physical elements so far ignored in the supernova simulations would or would not have an impact on the neutrino-heating mechanism such as the effects of neutrino self-interactions nuclear burning and the turbulent heatingdue to the magneto-rotational instability. These effects are included in our 2D simulations with the spectral neutrino transport (Suwa et al. (2010)).In addition we will report our 3D results based on the 3D version of the code and discuss their potential impacts on the explosion mechanism. Based on these results we will compute the gravitational radiation and neutrinoemission and then discuss some prospects towards multi-messenger astronomyof supernova explosions.