Rayleigh–Taylor instability in strongly coupled plasma

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 o...

Descripción completa

Detalles Bibliográficos
Autores principales: Wani, Rauoof, Mir, Ajaz, Batool, Farida, Tiwari, Sanat
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2022
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9262965/
https://www.ncbi.nlm.nih.gov/pubmed/35798786
http://dx.doi.org/10.1038/s41598-022-15725-2

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9262965/
https://www.ncbi.nlm.nih.gov/pubmed/35798786
http://dx.doi.org/10.1038/s41598-022-15725-2

Ejemplares similares