Lecture 19. The Method of Zs When problems get complicated numerical complexity makes computation SLOW The method of Zs speeds the computation up We will.

Slides:



Advertisements
Similar presentations
Eric Prebys, FNAL.  We have focused largely on a kinematics based approach to beam dynamics.  Most people find it more intuitive, at least when first.
Advertisements

Lecture 6: Constraints II
Quantum One: Lecture 6. The Initial Value Problem for Free Particles, and the Emergence of Fourier Transforms.
Lecture 5: Constraints I
1 MA 1128: Lecture 19 – 4/19/11 Quadratic Formula Solving Equations with Graphs.
Lecture 7 Rolling Constraints The most common, and most important nonholonomic constraints They cannot be written in terms of the variables alone you must.
Lecture 2. A Day of Principles The principle of virtual work d’Alembert’s principle Hamilton’s principle 1 (with an example that applies ‘em all at the.
Mr Barton’s Maths Notes
Physics 430: Lecture 16 Lagrange’s Equations with Constraints
Lecture 9 Hamilton’s Equations conjugate momentum cyclic coordinates Informal derivation Applications/examples 1.
Please open your laptops, log in to the MyMathLab course web site, and open Quiz 3.1 IMPORTANT NOTE: If you have time left on your quiz clock after you.
3.6 Systems with Three Variables
Lecture 20: Putting it all together An actual mechanism A physical abstraction: links, springs, wheels, motors, etc. A mathematical model of the physical.
Module 5Relativity of Velocity and Acceleration1 Module 5 Relativity of Velocity and Acceleration The velocity transforms follow directly from the Lorentz.
DERIVING LINEAR REGRESSION COEFFICIENTS
Solving Systems of Equations
Section 11.2 Systems of Linear Equations
ME 407 Advanced Dynamics We will learn to model systems that can be viewed as collections of rigid bodies Common mechanical systems Robots Various wheeled.
The Node Voltage Method
1 Lecture 27. Two Big Examples The eleven link diver The Stanford Arm (Kane & Levinson)
ME451 Kinematics and Dynamics of Machine Systems
ME451 Kinematics and Dynamics of Machine Systems Numerical Solution of DAE IVP Newmark Method November 1, 2013 Radu Serban University of Wisconsin-Madison.
1 Lecture 25: Modeling Diving I. 2 What do we need to do? Figure out what and how to simplify Build a physical model that we can work with Once that is.
Lecture 13: Stability and Control I We are learning how to analyze mechanisms but what we’d like to do is make them do our bidding We want to be able to.
University Prep Math Patricia van Donkelaar Course Outcomes By the end of the course,
Lecture 12: The Constraint Null Space The matrix C has M rows and N columns, M < N If we have set this up correctly, the rows of C are independent Nonholonomic.
Lecture 8: Rolling Constraints II
Lecture 14: Stability and Control II Reprise of stability from last time The idea of feedback control Remember that our analysis is limited to linear systems.
Lecture 23 The Spherical Bicycle II 1 The story so far: We found the constraint matrix and the null space matrix We “cheated” a little bit in assessing.
Lecture 26. Control of the Diver In order for a diver to do what he or she does the diver applies effective torques at the joints We want to find a recipe.
Differential Equations MTH 242 Lecture # 13 Dr. Manshoor Ahmed.
Lesson 4-2: Solving Systems – Substitution & Linear Combinations
First, a little review: Consider: then: or It doesn’t matter whether the constant was 3 or -5, since when we take the derivative the constant disappears.
Ch. 8: Hamilton Equations of Motion Sect. 8.1: Legendre Transformations Lagrange Eqtns of motion: n degrees of freedom (d/dt)[(∂L/∂q i )] - (∂L/∂q i )
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.
Integration by Substitution Antidifferentiation of a Composite Function.
Lagrange’s Equations with Undetermined Multipliers Marion, Section 7.5 Holonomic Constraints are defined as those which can be expressed as algebraic.
Solution of. Linear Differential Equations The first special case of first order differential equations that we will look is the linear first order differential.
Do Now (3x + y) – (2x + y) 4(2x + 3y) – (8x – y)
Chapter 4 Section 4.1 Solving Systems of Equations in Two Variables.
Phy 303: Classical Mechanics (2) Chapter 3 Lagrangian and Hamiltonian Mechanics.
ME 440 Intermediate Vibrations Th, April 16, 2009 Chapter 6: Multi-degree of Freedom (MDOF) Systems © Dan Negrut, 2009 ME440, UW-Madison Quote of the Day:
Ch : Solving Systems of Equations Algebraically.
Advanced Engineering Mathematics, 7 th Edition Peter V. O’Neil © 2012 Cengage Learning Engineering. All Rights Reserved. CHAPTER 4 Series Solutions.
Solving Systems of Equations By Elimination. Warm – up!! *As you walk in, please pick up your calculator!!* Use substitution to solve the following systems.
1 Lecture 15: Stability and Control III — Control Philosophy of control: closed loop with feedback Ad hoc control thoughts Controllability Three link robot.
Section 3.5 Solving Systems of Linear Equations in Two Variables by the Addition Method.
Finding Definite Integrals by Substitution and Solving Separable Differential Equations.
Canonical Equations of Motion -- Hamiltonian Dynamics
Lecture 10 Reprise and generalized forces The Lagrangian Holonomic constraints Generalized coordinates Nonholonomic constraints Euler-Lagrange equations.
3-2 Solving Systems Algebraically. In addition to graphing, which we looked at earlier, we will explore two other methods of solving systems of equations.
1 Lecture 24: Controlling the Uncontrollable Building the Unbuildable How do we deal with this uncontrollable system? Can we extend the method of Zs to.
SOLVING SYSTEMS OF EQUATIONS BY SUBSTITUTION. #1. SOLVE one equation for the easiest variable a. Isolated variable b. Leading Coefficient of One #2. SUBSTITUTE.
Notes 6.5, Date__________ (Substitution). To solve using Substitution: 1.Solve one equation for one variable (choose the variable with a coefficient of.
Lecture 22 The Spherical Bicycle 1. 2 Some relative dimensions with the wheel radius and mass as unity sphere radius 2, mass 50 fork length 4, radius.
Section 10.3 The Elimination Method Section 10.4 Systems of Linear Equations in 3 Variables.
Objective The student will be able to: solve systems of equations using elimination with addition and subtraction.
Advanced Higher Notes. Inverse Trigonometric Functions Integration By Partial Fractions 1 Integration By Partial Fractions 2 Integration By Partial.
Please CLOSE YOUR LAPTOPS, and turn off and put away your cell phones, and get out your note- taking materials.
6) x + 2y = 2 x – 4y = 14.
CLOSE Please YOUR LAPTOPS, and get out your note-taking materials.
MTH1170 Integration by Partial Fractions
5.2 Solving Systems Using Substitution
THE SUBSTITUTION METHOD
Quantum One.
Solving Systems of Equations
© Sharif University of Technology - CEDRA By: Professor Ali Meghdari
The Substitution Method
Linear Functions and Slope-Intercept Form Lesson 2-3
Presentation transcript:

Lecture 19. The Method of Zs When problems get complicated numerical complexity makes computation SLOW The method of Zs speeds the computation up We will eventually look at the third problem of problem set 5 which is computationally impractical (at least in Mathematica) without Zs 1

We set this in the context of Hamilton’s equations with nonholonomic constraints I generally replace connectivity constraints with pseudononholonomic constraints When I do this we recall that we can write The momentum can be written in terms of u j. where I am borrowing Mathematica’s substitution operator 2

3 The game is to isolate the us, writing the derivatives as coefficients times us I will denote the coefficients in the momentum (Hamilton and reduced Hamilton) equations by Zs This is going to seem a wee bit weird Bear with me. It’ll make sense eventually

We note that p i is linear in u j, which we can write as 4 We can obtain the Zs from the usual momentum expression or The latter is often easier

5 It is clear from the expression that Z does not depend on u

6 We already have the equations for the evolution of q: Hamilton’s equations become where any explicit We need to replace

7 So that we have Hamilton’s equations in the form Remember that these are not actually correct because I have not written the Lagrange multipliers is the correct form

8 We have learned to multiply by S to obtain the correct form the reduced Hamilton’s equations We need to solve these simultaneously with the q equations

9 is, formally, a terribly complicated expression However, if we relegate the connectivity constraints to the pseudononholonomic world most of the derivatives of M are zero, and it is not at all bad We will see this in context

10 The full formal expression for the reduced Hamilton’s equations This is a set of nonlinear first order ordinary differential equations in u the coefficients of which are functions of q, often quite complicated functions This would be a snap to integrate numerically were the coefficients to be constant The method of Zs pretends that they are

11 I have adapted the method of Zs from Kane and Levinson’s 1983 paper, cited in the text Their work used Kane’s method, which I explore in the text, but not in class My method of Zs is not as complete as it might be, because I allow some of the coefficients to remain as explicit functions of q This relies onactually being pretty simple functions of q (and also the generalized forces)

12 Write Hamilton’s equations as follows We replace the Z variables by constants This choice of substitutions aligns with Hamilton’s equations, not the reduced equations

13 Of course, they are not constants, so we have to add algebraic equations to our system to allow us to calculate them as we go forward That has been a lot to digest, and we’ll go through an example shortly Let me try to summarize this first

14 the simple holonomic constraints generalized coordinates Lagrangian nonholonomic and pseudononholonomic constraints Hamilton’s equations Start from square one introduce the Zs reduced Hamilton’s equations with Zs generalized forces

15 Consider the little sphere on the big sphere — both free to roll

16 How do we set this up? Set the K axis of the big sphere horizontal as before for rolling I can choose the inertial axis such that the small sphere is on the i axis without loss of generality If all I care about is the ball rolling down starting from rest then the simplest thing to do is but its K axis horizontal as well

17

18 It might be fun to start the ball rolling on a line of latitude The easiest way to do that is to put the K axis on a line of longitude which we can do by the proper choice of  and . We want K to be Pick

19

20 Go to Mathematica to look at this