Modelling turbulence induced by hydrodynamic instability in differentially-rotating flow

Project team

Dr Junho Park



Value of project to Coventry University


Total value of project


Duration of project

03/05/2022 – 02/05/2023

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Project overview

Rotating fluid flow is ubiquitous in many naturally occurring and engineering systems and plays a crucial role. For instance, the turbulence of geophysical vortices in the oceans is responsible for the mixing of fluid momentum and scalars such as salinity or planktons. Rotating flow is also important in industrial processes to produce homogenised products by efficient turbulent mixing (e.g. glass or polymer manufacturing processes). Rotation profiles of fluid flow are often differential, i.e. the angular speed varies with radius from the rotation axis. Such differentially-rotating flow can become centrifugally unstable when an imbalance exists between the pressure gradient and centrifugal force, a situation arising when the angular momentum decreases with the radius. This centrifugal instability is very destructive and thus an important source of turbulence. Most of the studies on centrifugal instability have considered linear analyses in which perturbations that drive the instability are assumed to be small enough to neglect nonlinear terms in the governing equations. On the other hand, nonlinear development processes of the instability such as saturation or laminar-turbulent transition have not been thoroughly investigated. In particular, the nonlinear centrifugal instability is not fully understood under the combined effects of thermal diffusion and stratification. Fluid flow with heat transfer is a very common configuration in various natural and engineering systems, thus revealing the role of such thermal effects on turbulence can significantly contribute to our knowledge of multi-physical flow systems in physical sciences and engineering. 

Project objectives

The current research programme aims to achieve two main objectives: (i) Investigate nonlinear development processes of the centrifugal instability under the effects of thermal diffusion and stratification, and; (ii) Develop a new turbulence model to apply to multi-physics simulations. In the first part of the programme, we will examine linear and nonlinear centrifugal instability of a famous rotating shear flow called Taylor-Couette (TC) flow, the flow between two concentric cylinders that rotate independently. We will first analyse linear centrifugal instability of the TC flow in thermally diffusive and stratified fluids using the Wentzel–Kramers–Brillouin-Jeffreys (WKBJ) method. The linear analysis will reveal how the thermal effects affect the initial growth of small-amplitude perturbations and the WKBJ method will allow us to derive explicit mathematical expressions of the instability growth. Nonlinear instability will then be investigated by both direct numerical simulations and a semi-linear model. Such nonlinear analyses can demonstrate how nonlinear interactions between perturbations and base flow lead to the saturation or laminar-turbulent transition processes. The second part of the programme will focus on developing a new turbulence model. Results from linear and nonlinear stability analyses will be used to construct a turbulent viscosity to apply to multi-physics simulations. More specifically, we will apply the new model to the state-of-the-art code for stellar physics simulations of the evolution of rotating stars. The updated code will simulate the stellar evolution and produce results such as radial distributions of mass, angular momentum or chemicals in the stellar interior. The outcomes will be compared with those from other stellar evolution simulations and observations. By achieving the main objectives of the proposed research, we will advance our understanding of instability-induced turbulence and its role in the multi-physics processes of the evolution of stars. Such turbulence modelling will also be beneficial for researchers in other fields of physical sciences and engineering.

Impact statement

The proposed research will have broad impacts in the fields of physical sciences and engineering. In fluid dynamics, our research will provide a better understanding of instability and its nonlinear development to turbulence under the complex effects of thermal diffusion and stratification. Apart from fluid dynamicists, the direct and immediate academic beneficiaries from the research project will be astrophysicists. The dynamics of differential rotation and centrifugal instability has not been considered in previous turbulence models in astrophysics simulations on, for instance, stellar evolution or accretion disks. Therefore, the proposed research will contribute to our knowledge of the evolution of rotating stars and the angular momentum transport in astrophysical disks. The turbulence modelling is also of great importance in oceanography due to the dynamical similarities of the Earth’s oceans with the interiors of stars. For instance, instability and turbulence of shear flow in stratified and rotating fluids are essentially linked to the dynamics of oceanic vortices such as mixing, inertia-gravity wave emission, lifetime, etc. The development of a new turbulence model will be highly appreciated by researchers who wish to improve large-scale geophysics simulations. Moreover, the proposed research will have an impact on multi-physics simulations in various engineering systems. For instance, glass or polymer manufacturing processes involve rotating mixers to create turbulence for efficient mixing, thus advanced turbulence models are crucial for simulations of fluid flow and heat transfer in these systems. In a broad sense, the proposed interdisciplinary research aligns with the UK Research and Development Roadmap (version 2020) that emphasises ‘Enable international collaboration of UK R&D and strengthen current collaboration mechanisms and Remove barriers to interdisciplinary research to realise the benefits of diverse perspectives and technologies’. The research programme will focus on not only new scientific findings but also beneficial impacts to both fluid dynamics and astrophysics communities by establishing an international collaboration between the UK and other countries.

 Queen’s Award for Enterprise Logo
University of the year shortlisted
QS Five Star Rating 2020