Galaxy cluster mass halos ("clusters") in a dark matter simulation are matched to nodes several different cosmic webs found using the Disperse web finder. The have smoothings and parameter choices; for each, 4 methods considered matching clusters. For most of webs, outnumber clusters, but not every has node match (and sometimes $>1$ matches same node). clusters frequently lacking distribution l...

The dynamics of a three-phase gas–liquid–liquid multiphase system is examined by direct numerical simulations. consists continuous liquid phase, buoyant gas bubbles, and smaller heavy drops that fall relative to the liquid. computational domain fully periodic, force equal weight mixture added keep it in place. governing parameters are selected so terminal Reynolds numbers bubbles moderate; whil...