2022
DOI: 10.1103/physreve.105.065205
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Effect of collisions with a second fluid on the temporal development of nonlinear, single-mode, Rayleigh-Taylor instability

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“…Noticeably, the potential model equations can recover the linear evolution of the interface or be used to construct buoyancy drag and bubble merger models accounting for the turbulence regime (Ramaprabhu et al 2006). These approaches were also successfully extended to ablative RTI configurations (Betti & Sanz 2006), to two-dimensional RTI with a horizontal magnetic field perpendicular to the single-mode perturbation (Gupta et al 2010), and more recently to the context of a partially ionized plasma (Cauvet et al 2022). The potential models have some limitations (Mikaelian 2008), and in particular they cannot account for the bubble/spike reacceleration when the secondary shear instabilities develop (Ramaprabhu et al 2006;Wei & Livescu 2012;Bian et al 2020).…”
Section: Introductionmentioning
confidence: 99%
“…Noticeably, the potential model equations can recover the linear evolution of the interface or be used to construct buoyancy drag and bubble merger models accounting for the turbulence regime (Ramaprabhu et al 2006). These approaches were also successfully extended to ablative RTI configurations (Betti & Sanz 2006), to two-dimensional RTI with a horizontal magnetic field perpendicular to the single-mode perturbation (Gupta et al 2010), and more recently to the context of a partially ionized plasma (Cauvet et al 2022). The potential models have some limitations (Mikaelian 2008), and in particular they cannot account for the bubble/spike reacceleration when the secondary shear instabilities develop (Ramaprabhu et al 2006;Wei & Livescu 2012;Bian et al 2020).…”
Section: Introductionmentioning
confidence: 99%