General Lagrangian solution (review) Curvilinear coordinate systems

Slides:



Advertisements
Similar presentations
Fourier’s Law and the Heat Equation
Advertisements

Fourier’s Law and the Heat Equation
The Asymptotic Ray Theory
EE3321 ELECTROMAGENTIC FIELD THEORY
EE3321 ELECTROMAGENTIC FIELD THEORY
Chapter 24 Gauss’s Law.
Chapter 23 Gauss’ Law.
DIFFUSION OF NEUTRONS OVERVIEW Basic Physical Assumptions
Chapter 24 Gauss’s Law.
Fundamentals of Applied Electromagnetics
Kinetics of Rigid Bodies in Three Dimensions
Basic Governing Differential Equations
1 MECH 221 FLUID MECHANICS (Fall 06/07) Tutorial 6 FLUID KINETMATICS.
Chapter 24 Gauss’s Law.
Method to Use Conservations Laws in Fluid Flows…… P M V Subbarao Professor Mechanical Engineering Department I I T Delhi Mathematics of Reynolds Transport.
Vectors and the Geometry of Space 9. 2 Announcement Wednesday September 24, Test Chapter 9 (mostly )
X y z Point can be viewed as intersection of surfaces called coordinate surfaces. Coordinate surfaces are selected from 3 different sets.
Lecture 4: Boundary Value Problems
UNIVERSITI MALAYSIA PERLIS
The Hydrogen Atom Quantum Physics 2002 Recommended Reading: Harris Chapter 6, Sections 3,4 Spherical coordinate system The Coulomb Potential Angular Momentum.
Geometric Transformation. So far…. We have been discussing the basic elements of geometric programming. We have discussed points, vectors and their operations.
3-1 Lesson 3 Objectives Boundary conditions Boundary conditions General Lagrangian solution (review) General Lagrangian solution (review) Curvilinear coordinate.
Section 17.5 Parameterized Surfaces
1 Gauss’s Law For r > a Reading: Chapter Gauss’s Law Chapter 28.
Chapter 24 Gauss’s Law. Let’s return to the field lines and consider the flux through a surface. The number of lines per unit area is proportional to.
Sect. 1.3: Constraints Discussion up to now  All mechanics is reduced to solving a set of simultaneous, coupled, 2 nd order differential eqtns which.
Chapter 11 Angular Momentum. Angular momentum plays a key role in rotational dynamics. There is a principle of conservation of angular momentum.  In.
Vectors n v What is the projection of the vector (1, 3, 2) onto the plane described by ? Louisiana Tech University Ruston, LA
13-1 Lesson 13 Objectives Begin Chapter 5: Integral Transport Begin Chapter 5: Integral Transport Derivation of I.T. form of equation Derivation of I.T.
Gauss’ Law Chapter 23 Copyright © 2014 John Wiley & Sons, Inc. All rights reserved.
Chapter 4: Solutions of Electrostatic Problems 4-1 Introduction 4-2 Poisson’s and Laplace’s Equations 4-3 Uniqueness of Electrostatic Solutions 4-4 Methods.
10-1 Lesson 10 Objectives Chapter 4 [1,2,3,6]: Multidimensional discrete ordinates Chapter 4 [1,2,3,6]: Multidimensional discrete ordinates Multidimensional.
Wave Dispersion EM radiation Maxwell’s Equations 1.
Wave Equations: EM Waves. Electromagnetic waves for E field for B field.
Review on Coulomb’s Law and the electric field definition Coulomb’s Law: the force between two point charges The electric field is defined as The force.
MODULE 6 ANGULAR MOTION AND ANGULAR MOMENTUM In Module 3 we solved the Schrödinger equation for motion in a circular trajectory about a central, fixed.
COORDINATE SYSTEMS & TRANSFORMATION
ENE 325 Electromagnetic Fields and Waves Lecture 2 Static Electric Fields and Electric Flux density.
LINE,SURFACE & VOLUME CHARGES
Prof. Dr. Faisel Ghazi Mohammed
Soh Ping Jack, Azremi Abdullah Al-Hadi, Ruzelita Ngadiran
CE 3305 Engineering FLUID MECHANICS
CE 3305 Engineering FLUID MECHANICS
Fourier’s Law and the Heat Equation
Part IV: Detailed Flow Structure Chap. 7: Microscopic Balances
The Transport Equation (cont’d)
Fourier’s Law and the Heat Equation
Cylindrical and Spherical Coordinates
Distributed Forces: Moments of Inertia
11 Vectors and the Geometry of Space
Chapter 4 [1,2,3,6]: Multidimensional discrete ordinates
Kinetics of Rigid Bodies in Three Dimensions
ENE 325 Electromagnetic Fields and Waves
ENE/EIE 325 Electromagnetic Fields and Waves
Reading: Chapter 28 For r > a Gauss’s Law.
ENE/EIE 325 Electromagnetic Fields and Waves
ENE 325 Electromagnetic Fields and Waves
Kinematics of Rigid Bodies in Three Dimensions
Section 17.1 Parameterized Curves
Vectors for Calculus-Based Physics
G L Pollack and D R Stump Electromagnetism
Chapter 12 Vectors and Geometry of Space
11 Vectors and the Geometry of Space
Thermodynamics of a Type I superconductor
Cylindrical and Spherical Coordinates
CHAPTER 3 MAGNETOSTATICS.
Notes 6 ECE 3318 Applied Electricity and Magnetism Coordinate Systems
Fundamentals of Applied Electromagnetics
Review Chapter 1-8 in Jackson
Lesson 4: Application to transport distributions
Presentation transcript:

General Lagrangian solution (review) Curvilinear coordinate systems Lesson 3 Objectives Boundary conditions General Lagrangian solution (review) Curvilinear coordinate systems Cylindrical Sphere Curvilinear Boltzmann Equation Conservative form of curvilinear equations

Initial and boundary conditions In order to solve for the flux y in a volume V of space (with its external surfaces denoted as G) at time t>0, we need to specify two types of external conditions: Initial conditions, Boundary conditions, for all for incoming angles (i.e., directions for which , where we have followed the usual convention of having be outward-pointing normal vectors on the surface.

where is the solution to: Initial conditions The usual situation for specifying initial conditions is to use the solution to the steady-state (i.e., time-independent) solution Boltzmann at time = 0, that is: where is the solution to:

The most common boundary conditions are: Void: Specified: (coupled problems) Reflected: Periodic: where the points map White:

Void boundary condition Vacuum: No particles going INTO volume V

Specified boundary condition V Entering particles from another problem or external source

Reflected boundary condition V V Like particle “mirrors” on each boundary

Periodic boundary condition V V Exiting particle re-enters on another boundary

White boundary condition No matter what direction it exits, re-enters isotropically.

General Lagrangian solution As you will remember, in the previous lesson we used an Lagrangian frame of reference. This gave us a solution in the form: where we defined s as the distance of travel of the particle.

General Lagrangian solution (2) This frame of reference is “moving along with” an unperturbed” pack of particles, and the equation “is completely parameterized” in terms of s: By “completely parameterized,” we mean that ALL the variables of y are defined as functions of s.

General Lagrangian solution (3) That is, beginning at some initial u=0, where a particle has some position (x0,y0,z0), direction cosines (m0 ,h0 ,x0), energy E0, and age t0, all of the variable changes can be associated with s. z y x

General Lagrangian solution (4) We evaluate the pieces of the total derivative that are appropriate to the coordinate system:

Cartesian coordinate system (static) z Notes: Same coordinate system for position and direction Direction coordinate system not dependent on particle position y x

Cartesian coordinate system static (2)

Corresponds to an arrangement of homogenous rectangular blocks: 2D Cartesian static Cartesian geometry can be simplified to 2D if one dimension can be assumed to be infinite simplifying the flux dependence: Corresponds to an arrangement of homogenous rectangular blocks: y Note: Infinite in z direction. x

2D Cartesian static (2)

Corresponds to an arrangement of homogenous parallel slabs: 1D Cartesian static Cartesian geometry can be simplified to 1D if two dimensions can be assumed to be infinite: Corresponds to an arrangement of homogenous parallel slabs: Note: Infinite in y and z directions. x

1D Cartesian static

Curvilinear coordinate systems We have worked out the equation for only ONE of the THREE orthogonal coordinate systems in common use (out of the 13 that have been identified) The other two are cylindrical and spherical

Curvilinear equations The Boltzmann Equation assumes a different form for the curvilinear (cylindrical and spherical) geometries. This is because the r vector follows the particle (like a skeet shooter’s rifle). The result of this is that the direction cosines change as the particle moves, which means that the angular derivatives of the Eulerian solution are no longer 0:

Spherical coordinate system z Notes: is parallel to position vector. is in same plane as the vertical axis and , perpendicular to . Third axis is perpendicular to the other two. r y x

Spherical coordinate system

1D spherical Spherical geometry is usually applied in its 1D radial form: Corresponds to a concentric arrangement of spherical shells:

1D spherical (Losing the azumuthal direction components is actually a little trickier than this)

Spherical 1D curvilinear equations In spherical 1D, a close up on the particle is:

Spherical 1D curvilinear equations (2) Final form of spherical 1D streaming term:

Cylindrical coordinate system z Notes: is parallel to projection of position vector. is in the (x,y) plane. Third axis is vertical. z y r x

Cylindrical coordinate system (2)

2D Cylindrical Cylindrical geometry can be simplified to 2D if there is rotational symmetry about the z axis: Corresponds to an arrangement of homogenous finite-height cylindrical rings: z Note: Homogeneous in q direction. All three direction cosines needed. y x

1D Cylindrical Cylindrical geometry can be simplified to 1D if there is rotational symmetry about the z axis and homogeneous in z direction: Corresponds to an arrangement of homogenous infinite-height cylindrical rings: Note: Homogeneous in q and z directions. Two direction variables needed.

1D Cylindrical (2)

Cylindrical 1D curvilinear equations In cylindrical 1D, a close up on the particle is:

Cylindrical 1D curvilinear equations Final form of cylindrical 1D streaming term:

Resulting curvilinear 1D B.E.’s The resulting B.E. for the 1D geometries are: Cartesian: Spherical Cylindrical

Conservative form Having spent all this trouble getting the curvilinear equations, we are NOT going to use them! Instead we are going to convert them into so-called conservative form, which will be better for us later when we finite difference in space. For now, I want you to be able to do two things: State why we are doing this: “So that when we finite difference the streaming operator, the resulting terms will conserve particles.” Show that the two are equivalent. This just involves simple differential calculus.

Conservative form for 1D B.E.’s The resulting conservative B.E.’s for the 1D curvilinear geometries are: Spherical Cylindrical

Homework Problems (3-1) Use the product differentiation rule to show that the conservative and non-conservative forms of the 1D spherial equation are identical. (3-2) Use the product differentiation rule to show that the conservative and non-conservative forms of the 1D cylindrical equation are identical.

Homework Problems (2) (3-3) Show that the white boundary condition is given by: