Figure 14: Convective instabilities inside the proto-neutron star in the 2D simulation of Müller and
Janka [176]. The evolutions of the temperature (left panels) and logarithmic density (right panels)
distributions are shown for the radial region . The upper and lower panels correspond to
times and , respectively, after the start of the simulation. The temperature values range
from to . The values of the logarithm of the density range from to
. The temperature and density both increase as the colors change from blue to green,
yellow, and red. (Figure 7 of [176]; used with permission.)
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