Multimessengers from Core-Collapse Supernovae: Multidimensionality as a Key to Bridge Theory and Observation
Figure 14
Panel (a) shows explosion energies (red line) versus input neutrino luminosities (), where green and blue lines show contributions from kinetic and thermal energy, respectively. Panel (b) shows the mass of protoneutron star () and the explosion timescales () as a function of . is estimated as the enclosed mass exceeding and as the time scale when the mass ejection rate at 100 km drops down to in our 2D simulations (from [248]).
