http://arxiv.org/abs/2104.13787
Dust plays a central role in several astrophysical processes. Hence the need of dust/gas numerical solutions, and analytical problems to benchmark them. In the seminal dustywave problem, we discover a regime where sound waves can not propagate through the mixture above a large critical dust fraction. We characterise this regime analytically, making it of use for testing accuracy of numerical solvers at large dust fractions.
T. David–Cléris and G. Laibe
Thu, 29 Apr 21
48/50
Comments: Accepted for publication in MNRAS