Figure 20
From: Entropy-limited hydrodynamics: a novel approach to relativistic hydrodynamics
Rotating star test: density on \(\pmb{(x, y)}\) plane. Two-dimensional rest-mass density distribution relative to the initial data maximum value on the equatorial \((x,y)\) plane at time \(t=4\text{,}300~M_{\odot}\) for the rotating star test. The behaviour of the star exterior is dynamic and chaotic with EL5 as compared with MP5.