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Lecture 17: Local Balance Laws

Steven M. Wise · 1:04:39 · Watch on YouTube

Part of University of Tennessee, Knoxville MATH 537. See all 21 lectures and search them

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Lecture 17: Local Balance Laws Watch on YouTube →

Overview

Steven M. Wise converts integral balance laws into local Eulerian equations using the transport theorem, the divergence theorem, and localization. The derivations yield the linear momentum equation, show that angular momentum balance requires a symmetric Cauchy stress, and produce local first- and second-law equations, including the assumptions that reduce the energy balance to the heat equation.

Key takeaways

Chapters

0:00 From Integral Balance Laws to Local Eulerian Equations
2:50 Deriving Local Linear Momentum Balance
9:47 Angular Momentum Balance and the Stress Symmetry Goal
12:12 Material Derivative of the Angular Momentum Integrand
24:23 Using Linear Momentum to Prove Cauchy Stress Symmetry
30:06 Rate of Strain and the Energy-Balance Setup
34:30 Converting Stress Power into Boundary Work
40:00 Kinetic Energy and the Net-Working Identity
44:30 Local First Law: Internal Energy, Heat Flux, and Sources
50:00 Localizing the First-Law Integral
52:30 Modeling Assumptions That Recover the Heat Equation
57:17 Local Second Law and Nonnegative Entropy Production

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Transcript excerpt

0:04 Welcome back to continuum mechanics. This is uh class number 17. It's our second lecture in chapter 5 talking about balance laws. All of the balance laws that we worked with were given in integral form to begin with and now we're engaging in the task of converting these into what are called local laws. These are essentially differential equations that we can work with and try to solve at some point. Uh if you use the finite element method, the interesting thing is that ultimately you integrate these equations and then solve them by in their what's called the weak form. And so you bring the the integrations back in order to solve the equations at least approximately. uh but to make the equations uh and the

0:54 the way people are most used to building and working with uh models is to uh convert all of our balance laws into what are called local laws. And so we started that process last time with a conservation of mass equation and um and a result related to that. Now we want to talk about the conservation of linear momentum and write these equations write this idea in a local version a local what's called oilarian version or a spatial version. Here's the result that we want to prove. Let fi be a motion with spatial velocity v and mass density row. Axiom 5.2 2 that is the balance of

1:43 linear momentum is equivalent to this equation. Row times the total time derivative of the velocity field V is equal to the divergence of the stress tensor field plus row * V. Let's make sure everything in sight makes sense. So the total time derivative of V is a vector field again. So row * V is a vector field. Row * B is

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