Image Details
Caption: Figure 9.
Equilibrated-state values of σdyn, denoted by σdyn(∞), for all of our cases, plotted with respect to case number. We approximate ﹩{\sigma }_{{\rm{dyn}}}(\infty )\approx {[{\left\langle {\tau }_{{\rm{v}}}\right\rangle }_{{\rm{drz}},t}/{\left\langle {\tau }_{{\rm{mc}}}\right\rangle }_{{\rm{drz}},t}]}^{1/2}﹩, where the temporal average is over the equilibrated state.
© 2026. The Author(s). Published by the American Astronomical Society.