Figure 11

Figure 8: An equatorial 2D slice from the Ott et al. [305] 3D simulation of their collapse model E20A that has a post-core-bounce β = T∕|W | of ∼ 9%. The snapshot displayed corresponds to t = 71.02 ms after core bounce. Shown is a colormap encoding specific entropy per baryon s in units of the Boltzmann constant kB. The colormap is cut at s = 3 kB/baryon to emphasize the dynamics in the unshocked (hence low-entropy) inner proto-neutron star regions. Visualization by Christian Ott.