2015
DOI: 10.1080/14685248.2015.1093638
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Large eddy simulation of orientation and rotation of ellipsoidal particles in isotropic turbulent flows

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Cited by 10 publications
(9 citation statements)
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“…(30) is the contribution parallel to p needed to keep the strain from changing the magnitude of p. It is natural to expect significant errors in the calculation of p over time when the exact velocity gradients (available in DNS) are replaced with those computed from the resolved velocity fielded yielded by LES. In addition, SGS effects are expected also on the rotational dispersion coefficient of the particles: This coefficient depends on the turbulent energy dissipation rate, which is reduced when SGS velocity fluctuations are not accounted for [22]. Indeed, results from a priori tests demonstrate that SGS fluctuations mostly affect particle rotation, resulting in weaker particle alignment with the vorticity field and reduced particle rotational energy if neglected.…”
Section: Elongated Particles In Homogeneous Isotropic Turbulencementioning
confidence: 99%
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“…(30) is the contribution parallel to p needed to keep the strain from changing the magnitude of p. It is natural to expect significant errors in the calculation of p over time when the exact velocity gradients (available in DNS) are replaced with those computed from the resolved velocity fielded yielded by LES. In addition, SGS effects are expected also on the rotational dispersion coefficient of the particles: This coefficient depends on the turbulent energy dissipation rate, which is reduced when SGS velocity fluctuations are not accounted for [22]. Indeed, results from a priori tests demonstrate that SGS fluctuations mostly affect particle rotation, resulting in weaker particle alignment with the vorticity field and reduced particle rotational energy if neglected.…”
Section: Elongated Particles In Homogeneous Isotropic Turbulencementioning
confidence: 99%
“…Direct comparison against DNS results shows that the stochastic model (LES-SDE) provides poor prediction of particle alignment and over-prediction (under-prediction) of the reconstructed rotational energy at large (small) aspect ratios. This is probably due to the fact that the stochastic part of the model used by [22] is Gaussian and uncorrelated in time: Therefore, the model cannot take into account any effect due to the anisotropy of particle rotation dynamics, which are correlated with preferential alignment phenomena, and any effect on particle rotational diffusivity due to the different correlation timescales characterizing the particle angular velocities [75]. The ADM-based model has little influence on particle alignment compared to a priori (FDNS) and a posteriori (LES) results, but improves prediction of the rotational energy for aspect ratios larger than unity: This is ascribed to the capability of ADM to recover fluid enstrophy near the cut-off scale [22].…”
Section: Elongated Particles In Homogeneous Isotropic Turbulencementioning
confidence: 99%
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