| | 32 | This case is closest to the Matched case. Here we see the effects of the Poisson boundary conditions in a similar way that we did above in the Matched case but not as exaggerated. That is, the velocity increases near the spherical boundary, but not as drastically. Near the end of the simulation, when the speeds have approached vrad/cs~4 nearer the BE sphere boundary, do we very quickly see a build up of density in the corresponding region. I wonder if this time corresponds to the time we see a 'turn-over' in the solution from compression wave to classic collapse? The free-fall time of ambient in this case is |
