Eddy Viscosity And Kinetic Energy (2.6) - Computational fluid dynamics (Contd.)
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Eddy Viscosity and Kinetic Energy

Eddy Viscosity and Kinetic Energy

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Interactive Audio Lesson

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Introduction to Reynolds Shear Stress

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Teacher
Teacher Instructor

Today, we're going to start with Reynolds shear stress, denoted as $ ho au_{ij}$. Can anyone tell me what Reynolds shear stress signifies in fluid dynamics?

Student 1
Student 1

Isn’t it related to how turbulent flows transfer momentum?

Teacher
Teacher Instructor

Exactly! It's essentially a measure of the momentum transfer due to turbulence. It represents how fluctuations impact the mean flow velocity.

Student 2
Student 2

So, does this mean we need to solve for it when modeling flows?

Teacher
Teacher Instructor

Yes, we face what's called the closure problem, where we need to express this in terms of known average quantities. This sets the stage for using models like the k-epsilon.

Understanding Turbulent Kinetic Energy

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Teacher
Teacher Instructor

Now, let’s explore turbulent kinetic energy, often just called 'k'. What do you think it consists of?

Student 3
Student 3

I think it includes the energy due to the fluctuations in velocity?

Teacher
Teacher Instructor

Right! It’s the sum of the mean kinetic energy and the fluctuations, represented mathematically. The overall kinetic energy can be represented as $K + k$, where $K$ is the mean and $k$ is the turbulent kinetic energy.

Student 4
Student 4

How do we calculate these terms to find turbulent kinetic energy?

Teacher
Teacher Instructor

Great question! We use specific equations that relate it to other variables, particularly within the k-epsilon model.

The Role of Eddy Viscosity ($ u_T$)

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Teacher Instructor

"Next, let's talk about eddy viscosity, denoted as $

Reynolds Number and Its Implications

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Teacher
Teacher Instructor

Finally, let’s analyze Reynolds number and its implications on our modeling efforts. What does Reynolds number indicate?

Student 3
Student 3

It compares inertial and viscous forces in the fluid flow.

Teacher
Teacher Instructor

Exactly! A high Reynolds number means inertial forces dominate, indicating turbulent flow conditions, while a low number signifies laminar flow.

Student 4
Student 4

Why is this important for computational simulations?

Teacher
Teacher Instructor

Because it impacts our computational resources greatly! High Reynolds numbers lead to significant grid resolutions during simulations.

Introduction & Overview

Read summaries of the section's main ideas at different levels of detail.

Quick Overview

This section explores the concepts of eddy viscosity and kinetic energy in the context of turbulent flow modeling, particularly through the k-epsilon model.

Standard

The section details how eddy viscosity relates to turbulent kinetic energy and its dissipation, introducing the k-epsilon model as a crucial technique in computational fluid dynamics. It covers key equations, the significance of turbulence models, and the implications of Reynolds numbers in simulating turbulent flows.

Detailed

In this section, we delve into the interplay between eddy viscosity and kinetic energy in turbulent flows, emphasizing how these concepts are fundamental in closure problems within computational fluid dynamics (CFD). The Reynolds shear stress, represented as $
ho au_{ij}$, plays a vital role in understanding mean flows, while the k-epsilon model serves as a standard methodology for modeling turbulent kinetic energy (k) and its dissipation rate (epsilon). The section provides essential equations connecting eddy viscosity ($
u_T$) to various parameters, further noting the importance of the Reynolds number in computational simulations. Additionally, it contextualizes the turbulence models and emphasizes their relevance in accurately predicting fluid behaviors in real-world scenarios, along with the implications on computational resources required for direct numerical simulations.

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Introduction to Eddy Viscosity

Chapter 1 of 4

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Chapter Content

So, if you see there is a term called nu T. So, this nu t is the eddy viscosity. So, this actually is not should better be called as turbulent eddy viscosity, nu T, it can be actually dimensionally related to kinetic energy k kinetic energy dissipation rate epsilon through nu T is written as c mu into k square by epsilon.

Detailed Explanation

Eddy viscosity (nu T) is a measure of how momentum is transferred in turbulent flow. It's derived from the kinetic energy (k) of the turbulent flow and the rate at which this energy dissipates (epsilon). Essentially, nu T relates to how much turbulence influences the flow, allowing us to understand how fast particles move in a fluid. It's expressed mathematically as nu T = c_mu × (k^2 / epsilon), where c_mu is a constant obtained from experiments.

Examples & Analogies

Think of a crowded room where people are moving around in a random manner. The 'eddy viscosity' is like the invisible forces that help the individuals bump into each other and change direction, reflecting how momentum is transferred throughout the crowd.

The Role of Turbulent Kinetic Energy

Chapter 2 of 4

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Chapter Content

The turbulent kinetic energy and the energy dissipation can be determined from the following equation. So, now, we said that this is the equation which we are going to use for determining tau i j and that we can use in our average equation Reynolds average Navier stokes equation.

Detailed Explanation

Turbulent kinetic energy (k) represents the chaotic, random motion of fluid particles in turbulent flows. It is crucial because it allows for understanding the energy dynamics in turbulence, including how energy changes and dissipates in the flow. The turbulent kinetic energy relates to the Reynolds-averaged Navier-Stokes equations, which describe how fluid moves under various conditions, accounting for averages over turbulent fluctuations.

Examples & Analogies

Imagine a river with varying depth and speed. The turbulent kinetic energy in the river reflects how fast and chaotically the water flows. When there’s a blockage (like a rock), the energy changes, illustrating how turbulence behaves in different flow situations.

Modeling Turbulence: K-Epsilon Equations

Chapter 3 of 4

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Chapter Content

So, what we do is we solve the k and epsilon equations to find out turbulent kinetic turbulent eddy viscosity nu T put it into the Reynolds shear stress equation and use that in the average equation of Reynolds Navier Stokes equation.

Detailed Explanation

In turbulence modeling, particularly using the k-epsilon model, we solve equations for both turbulent kinetic energy (k) and energy dissipation rate (epsilon). By determining these two variables, we can establish the eddy viscosity (nu T). This, in turn, helps predict turbulent shear stress (tau ij) and integrates these findings into the Reynolds-averaged Navier-Stokes equations, essential for understanding fluid dynamics.

Examples & Analogies

Think of a mechanic tuning an engine. They need to understand how much fuel (energy) goes into the engine and how it’s released (dissipation) for the car to run efficiently. Similarly, the k-epsilon model fine-tunes our understanding of turbulence in fluid flows.

Importance of Dimensional Analysis

Chapter 4 of 4

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Chapter Content

C mu is a non-dimensional constant. Which values we know from experiments for uniform and isotropic turbulence there is no production or diffusion of turbulent kinetic energy, therefore, del k delta t will be equal to - epsilon E.

Detailed Explanation

The constant C_mu provides essential context in dimensional analysis for turbulence modeling. It indicates relationships between the physical variables involved in the k-epsilon model. This helps researchers predict how turbulent kinetic energy behaves under varying conditions. Essentially, knowing C_mu allows us to make accurate predictions without needing direct experimental data every time.

Examples & Analogies

Like how a chef uses a recipe as a reference for cooking. The recipe helps balance flavors (constants) so the dish doesn’t turn out too salty or bland. Similarly, C_mu acts as a reference in fluid dynamics, ensuring accuracy in modeling turbulent flows.

Key Concepts

  • Reynolds shear stress: It helps quantifying momentum transfer in turbulent flows.

  • Turbulent kinetic energy (k): It serves as a measure of energy in turbulence.

  • Eddy viscosity ($ν_T$): A key parameter in modeling turbulence in fluid flows.

  • Closure problem: A challenge in expressing turbulent properties in terms of averaged quantities.

  • k-epsilon Model: A widely used turbulence model for predicting properties in turbulent flows.

Examples & Applications

When modeling flow around a bridge, the k-epsilon model can help predict how turbulence affects structure stability.

Using a numerical simulation of airflow over a car, the role of eddy viscosity can provide insights on fuel efficiency by reducing drag.

Memory Aids

Interactive tools to help you remember key concepts

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Rhymes

In turbulence, we see with glee, Reynolds shear stress sets momentum free.

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Stories

Imagine a turbulent river with lots of rocks. The water flows faster in some places (mean flow) and swirls in others (turbulent flow). The energy from the swirls keeps the river moving smoothly.

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Memory Tools

Kinetic energy = K + k: Mean + fluctuations make it not lack!

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Acronyms

Eddy Viscosity = E.V. = Energy Vortex!

Flash Cards

Glossary

Reynolds Shear Stress

A measure of the momentum transfer in turbulent flow, related to fluctuations impacting mean velocity.

Turbulent Kinetic Energy (k)

The energy in a turbulent flow due to velocity fluctuations, consisting of a mean and a turbulent component.

Closure Problem

The challenge of expressing complex turbulent quantities in terms of known average values during modeling.

kepsilon Model

A widely used turbulence model that relates turbulent kinetic energy and its dissipation rate.

Reference links

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