{"title":"Plasma kinetics: Discrete Boltzmann modelling and Richtmyer-Meshkov instability","authors":"Jiahui Song, Aiguo Xu, Long Miao, Feng Chen, Zhipeng Liu, Lifeng Wang, Ningfei Wang, Xiao Hou","doi":"arxiv-2303.12356","DOIUrl":null,"url":null,"abstract":"A discrete Boltzmann model (DBM) for plasma kinetics is proposed. The DBM\ncontains two physical functions. The first is to capture the main features\naiming to investigate and the second is to present schemes for checking\nthermodynamic non-equilibrium (TNE) state and describing TNE effects. For the\nfirst function, mathematically, the model is composed of a discrete Boltzmann\nequation coupled by a magnetic induction equation. Physically, the model is\nequivalent to a hydrodynamic model plus a coarse-grained model for the most\nrelevant TNE behaviors including the entropy production rate. The first\nfunction is verified by recovering hydrodynamic non-equilibrium (HNE) behaviors\nof a number of typical benchmark problems. Extracting and analyzing the most\nrelevant TNE effects in Orszag-Tang problem are practical applications of the\nsecond function. As a further application, the Richtmyer-Meshkov instability\nwith interface inverse and re-shock process is numerically studied. It is found\nthat, in the case without magnetic field, the non-organized momentum flux shows\nthe most pronounced effects near shock front, while the non-organized energy\nflux shows the most pronounced behaviors near perturbed interface. The\ninfluence of magnetic field on TNE effects shows stages: before the interface\ninverse, the TNE strength is enhanced by reducing the interface inverse speed;\nwhile after the interface inverse, the TNE strength is significantly reduced.\nBoth the global averaged TNE strength and entropy production rate contributed\nby non-organized energy flux can be used as physical criteria to identify\nwhether or not the magnetic field is sufficient to prevent the interface\ninverse.","PeriodicalId":501231,"journal":{"name":"arXiv - PHYS - Cellular Automata and Lattice Gases","volume":"56 41","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2023-03-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Cellular Automata and Lattice Gases","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2303.12356","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
A discrete Boltzmann model (DBM) for plasma kinetics is proposed. The DBM
contains two physical functions. The first is to capture the main features
aiming to investigate and the second is to present schemes for checking
thermodynamic non-equilibrium (TNE) state and describing TNE effects. For the
first function, mathematically, the model is composed of a discrete Boltzmann
equation coupled by a magnetic induction equation. Physically, the model is
equivalent to a hydrodynamic model plus a coarse-grained model for the most
relevant TNE behaviors including the entropy production rate. The first
function is verified by recovering hydrodynamic non-equilibrium (HNE) behaviors
of a number of typical benchmark problems. Extracting and analyzing the most
relevant TNE effects in Orszag-Tang problem are practical applications of the
second function. As a further application, the Richtmyer-Meshkov instability
with interface inverse and re-shock process is numerically studied. It is found
that, in the case without magnetic field, the non-organized momentum flux shows
the most pronounced effects near shock front, while the non-organized energy
flux shows the most pronounced behaviors near perturbed interface. The
influence of magnetic field on TNE effects shows stages: before the interface
inverse, the TNE strength is enhanced by reducing the interface inverse speed;
while after the interface inverse, the TNE strength is significantly reduced.
Both the global averaged TNE strength and entropy production rate contributed
by non-organized energy flux can be used as physical criteria to identify
whether or not the magnetic field is sufficient to prevent the interface
inverse.