Deformation and stability of a gas bubble in a biaxial straining flow
Aliénor Rivière, David Fabre, Jacques Magnaudet, François Gallaire
TL;DR
This work uses the L-ALE framework to map the full bifurcation structure and linear stability of a gas bubble at the stagnation point of a biaxial straining flow across a range of $We$ and $Oh$. It uncovers a saddle-node bifurcation with strongly $Oh$-dependent equilibrium shapes, including both oblate and prolate morphologies and two sets of disconnected branches. The linear stability analysis reveals symmetry-preserving and drift modes, plus a novel azimuthal $m=2$ instability on oblate shapes, suggesting possible breakup scenarios in turbulence. The findings offer insights into bubble deformation and breakup in isotropic turbulence and extend prior uniaxial results to biaxial configurations, with potential implications for modeling bubble transport and fragmentation in practical flows.
Abstract
Taking advantage of the recently developed L-ALE framework [Sierra-Ausin \textit{et al.}, Phys. Rev. Fluids {\bf{7}}, 113603 (2022)], we characterize the linear dynamics of an incompressible gas bubble immersed in a biaxial straining flow. We show that the system undergoes a saddle-node bifurcation with strongly different equilibrium shapes when varying the Ohnesorge number, $\Oh$, which compares viscous and capillary effects. Equilibrium shapes are found to be oblate for sufficiently large $\Oh$ while, counter-intuitively, they are prolate for low-enough $\Oh$. The bifurcation diagram is found to contain also two sets of disconnected branches that cannot be obtained by continuation starting from a spherical shape. One set corresponds to bubble shapes expected to be unstable, while the second set comprises a wide region exhibiting stable shapes that might be observed in practice. We then characterize the linear stability of the various branches. In addition to the unstable axisymmetric mode arising at the saddle-node bifurcation, two non-oscillating drift modes are also identified, together with a new unstable non-oscillating mode with azimuthal wave number $m=2$. This mode might be responsible for some type of bubble breakup observed in experiments.
