A dominant dimensionless number and theoretical model for the evolution of multiphase Richtmyer-Meshkov instability

被引:6
|
作者
Si, Yingming [1 ,2 ]
Li, Shuai [3 ,4 ]
Meng, Baoqing [1 ,2 ]
Wang, Chun [1 ,2 ]
Tian, Baolin [4 ]
机构
[1] Chinese Acad Sci, Inst Mech, State Key Lab High Temp Gas Dynam, Beijing 100190, Peoples R China
[2] Univ Chinese Acad Sci, Sch Engn Sci, Beijing 100049, Peoples R China
[3] China Acad Engn Phys, Grad Sch, Beijing 100088, Peoples R China
[4] Inst Appl Phys & Computat Math, Mech Teaching & Res Off, Beijing 100094, Peoples R China
基金
中国国家自然科学基金;
关键词
SHOCK; TAYLOR; FLOW;
D O I
10.1063/5.0180793
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
Multiphase Richtmyer-Meshkov instability (RMI) is often accompanied by a dispersed phase of particles, where the evolution of the mix zone width (MZW) is a significant issue. The Stokes number ( S t) is a key dimensionless parameter for particle-containing multiphase flows because it represents the ability of particles to follow the fluid. However, our theoretical analysis and numerical simulation indicate that the Stokes number is not the only dominant parameter for the evolution of multiphase RMI. This study uses the derivation of particle and fluid momentum equations to demonstrate the inability of the Stokes number to predict MZW evolution, that is, even at the same Stokes number, increasing the particle density or the radius leads to completely different MZW evolution trends. This study proposes a novel dimensionless number, S d, to measure the effect of drag on the fluid owing to the particles. S d is the ratio of the relaxation time of the fluid velocity affected by the particle force to the characteristic time of the shock wave. We developed theoretical models of MZW at different S d values. Subsequently, a set of multiphase RMI numerical simulations on uniformly distributed particles with different S t and S d values was conducted. The numerical results verify the theoretical predictions and effectiveness of the proposed dimensionless number. The phase diagram containing different simulation cases demonstrates that the Stokes number cannot be used to predict MZW and must be combined with S d to determine its evolution.
引用
收藏
页数:9
相关论文
共 50 条
  • [1] A dominant dimensionless number and theoretical model for the evolution of multiphase Richtmyer-Meshkov instability (vol 36, 013314, 2024)
    Si, Yingming
    Li, Shuai
    Meng, Baoqing
    Wang, Chun
    Tian, Baolin
    PHYSICS OF FLUIDS, 2024, 36 (02)
  • [2] Model for the Richtmyer-Meshkov instability
    Wouchuk, JG
    Nishihara, K
    ICPP 96 CONTRIBUTED PAPERS - PROCEEDINGS OF THE 1996 INTERNATIONAL CONFERENCE ON PLASMA PHYSICS, VOLS 1 AND 2, 1997, : 22 - 25
  • [3] Nonlinear evolution of the Richtmyer-Meshkov instability
    Herrmann, Marcus
    Moin, Parviz
    Abarzhi, Snezhana I.
    JOURNAL OF FLUID MECHANICS, 2008, 612 (311-338) : 311 - 338
  • [4] The Richtmyer-Meshkov instability
    Brouillette, M
    ANNUAL REVIEW OF FLUID MECHANICS, 2002, 34 : 445 - 468
  • [5] Impulsive model for the Richtmyer-Meshkov instability
    Vandenboomgaerde, M
    Mugler, C
    Gauthier, S
    PHYSICAL REVIEW E, 1998, 58 (02): : 1874 - 1882
  • [6] Richtmyer-Meshkov instability evolution in layered system
    Aleshin, AN
    Lazareva, EV
    Sergeev, SV
    Zaytsev, SG
    LASER AND PARTICLE BEAMS, 1999, 17 (04) : 649 - 652
  • [7] Richtmyer-Meshkov instability evolution in layered system
    Aleshin, A.N.
    Lazareva, E.V.
    Sergeev, S.V.
    Zaytsev, S.G.
    Laser and Particle Beams, 17 (04): : 649 - 652
  • [8] Studies on the nonlinear evolution of the Richtmyer-Meshkov instability
    Sadot, O
    Erez, L
    Oron, D
    Erez, G
    Ben-Dor, G
    Alon, U
    Levin, LA
    Shvarts, D
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2000, 127 (02): : 469 - 473
  • [9] Nonlinear evolution of an interface in the Richtmyer-Meshkov instability
    Matsuoka, C
    Nishihara, K
    Fukuda, Y
    PHYSICAL REVIEW E, 2003, 67 (03):
  • [10] Alfven Number for the Richtmyer-Meshkov Instability in Magnetized Plasmas
    Sano, Takayoshi
    ASTROPHYSICAL JOURNAL, 2021, 920 (01):