2021
DOI: 10.1016/j.ijmultiphaseflow.2021.103837
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Alignment of slender fibers and thin disks induced by coherent structures of wall turbulence

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Cited by 12 publications
(5 citation statements)
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“…where u(x, t) and p(x, t) are the velocity and pressure fields, ρ is the fluid density, τ is the stress tensor, and f fib is the feedback forcing from the fibre. Here, f turb is the external forcing term used to sustain turbulence, chosen to be the Arnold-Beltrami-Childress forcing (Dombre et al 1986) given by…”
Section: Methodsmentioning
confidence: 99%
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“…where u(x, t) and p(x, t) are the velocity and pressure fields, ρ is the fluid density, τ is the stress tensor, and f fib is the feedback forcing from the fibre. Here, f turb is the external forcing term used to sustain turbulence, chosen to be the Arnold-Beltrami-Childress forcing (Dombre et al 1986) given by…”
Section: Methodsmentioning
confidence: 99%
“…This property is also highly dependent on the configuration: e.g. in homogeneous isotropic turbulence flows, fibres are known to usually align with the intermediate eigenvector of the strain rate tensor, whereas for channels, they are a function of the channel height, largely influenced by the coherent structures (Cui et al 2021). Clearly, the alignment can also be influenced by viscoelastic stresses; experiments with low Reynolds number simple shear flows have shown that orientation of semi-dilute fibre suspensions in weakly (Iso, Koch & Cohen 1996b) and highly (Iso et al 1996a) elastic fluids change in comparison to their aligned directions in Newtonian flows (Stover, Koch & Cohen 1992).…”
Section: Alignmentmentioning
confidence: 99%
“…For Re p 1, the models include the Stokes resistance (Brenner 1963(Brenner , 1964Brenner & Cox 1963) and Jeffery torque (Jeffery 1922) for non-spherical particles. In the PP-DNSs without considering the effect of gravity, the weak inertial or inertialess prolate spheroids near the wall tend to align their symmetry axes with the streamwise direction, while the weak inertial or inertialess oblate spheroids preferentially align their symmetry axes with the wall-normal direction (Marchioli et al 2010;Challabotla, Zhao & Andersson 2015b;Zhao et al 2015;Jie et al 2019b;Cui et al 2020bCui et al , 2021. As the particle inertia increases, prolate spheroids have a tendency to tumble, while oblate spheroids preferentially spin in the streamwise-wall-normal plane near the wall (Marchioli et al 2010;Marchioli & Soldati 2013;Challabotla et al 2015a;Zhao et al 2015Zhao et al , 2019.…”
Section: Angular Dynamics Of Spheroidal Particles In Turbulent Channe...mentioning
confidence: 99%
“…Note that only the wall-normal particle velocity is reversed and the particle orientation remains the same after a collision. The same computational method has been widely employed in our previous studies (Challabotla et al 2015a;Cui et al 2020bCui et al , 2021Jie et al 2022). In this study, we tracked swarms of 300 000 spheroids of each case with the aspect ratio ranging from 0.02 to 50, and Stokes number ranging from 1 to 100.…”
Section: Direct Numerical Simulations Of Fluid and Particlesmentioning
confidence: 99%
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