Rayleigh-Taylor instability in strongly coupled plasma.

ABSTRACT: Rayleigh-Taylor instability (RTI) is the prominent energy mixing mechanism when heavy fluid lies on top of light fluid under the gravity. In this work, the RTI is studied in strongly coupled plasmas using two-dimensional molecular dynamics simulations. The motivation is to understand the evolution of the instability with the increasing correlation (Coulomb coupling) that happens when the average Coulombic potential energy becomes comparable to the average thermal energy. We report the suppression of the RTI due to a decrease in growth rate with increasing coupling strength. The caging effect is expected a physical mechanism for the growth suppression observed in both the exponential and the quadratic growth regimes. We also report that the increase in shielding due to background charges in

SUBMITTER: Wani R 

PROVIDER: S-EPMC9262965 | biostudies-literature | 2022 Jul

REPOSITORIES: biostudies-literature