Numerical simulations of simultaneous pair-drop impacts and their energetics
Ziyao Zhang, Alfonso A. Castrejon-Pita, Wouter Mostert
TL;DR
This work tackles the dynamics of simultaneous pair-drop impacts on a hydrophobic substrate using high-resolution 3D direct numerical simulations to resolve the central rising sheet formed by colliding lamellae. By validating against experiments and developing an energetic framework, it connects the maximum central-sheet height $H_{s,max}$ to the initial inertial–capillary balance through two geometric approximations—the cylindrical disk and the lollipop—while incorporating viscous dissipation. The study finds robust scaling trends, notably $H_{s,max} \sim We^{0.68} Re^{0.2}$ in the large-$Re$ regime (with geometry-dependent variations) and demonstrates near collapse of height dynamics under appropriate $We$ and $Re$ rescalings, providing a practical route to predict central-sheet evolution in multi-drop impacts. These results enhance understanding of inter-drop interactions in sprays and coatings and offer a framework applicable to more complex fluids and surface conditions.
Abstract
We present three-dimensional direct numerical simulations of the simultaneous impact of two identical drops on an hydrophobic substrate, varying the relative strength of capillary and viscous effects respectively through Weber and Reynolds numbers of impact. The interaction between the two drops is characterized by the appearance of a lamella arising from the collision of the two droplets' spreading rims. We examine the width, the height, and the general morphological evolution of the central sheet; the numerical data is validated against prior experiments and used to guide the development of an energetic model for the maximum elevation of the central sheet. In particular, the rise of the central sheet resembles the spreading behaviour single-drop impacts, especially at high Weber and Reynolds numbers. This fact can be used to estimate scalings in the capillary- and viscous-dominated regimes, which can be used to collapse the trajectories. These insights provide a route for a more complete understanding of the dynamics for the central rising sheet, and anticipate the detailed study of its fragmentation characteristics
