Solutions to Homework Set 3

Similar documents
Space Curves. Recall the parametric equations of a curve in xy-plane and compare them with parametric equations of a curve in space.

Physics 116C Solution of inhomogeneous ordinary differential equations using Green s functions

Math 115 ( ) Yum-Tong Siu 1. Lagrange Multipliers and Variational Problems with Constraints. F (x,y,y )dx

The Basic Functional 2 1

4. Calculus of Variations

Calculus of Variations

STURM-LIOUVILLE BOUNDARY VALUE PROBLEMS

Edexcel GCE Core Mathematics (C2) Required Knowledge Information Sheet. Daniel Hammocks

The Form of Hanging Slinky

ES 111 Mathematical Methods in the Earth Sciences Lecture Outline 1 - Thurs 28th Sept 17 Review of trigonometry and basic calculus

The Wave Equation I. MA 436 Kurt Bryan

Math 8 Winter 2015 Applications of Integration

Calculus of Variations: The Direct Approach

MATH34032: Green s Functions, Integral Equations and the Calculus of Variations 1. 1 [(y ) 2 + yy + y 2 ] dx,

Centre of Mass, Moments, Torque

Chapter 2. Constraints, Lagrange s equations

Plates on elastic foundation

A REVIEW OF CALCULUS CONCEPTS FOR JDEP 384H. Thomas Shores Department of Mathematics University of Nebraska Spring 2007

Section 5.1 #7, 10, 16, 21, 25; Section 5.2 #8, 9, 15, 20, 27, 30; Section 5.3 #4, 6, 9, 13, 16, 28, 31; Section 5.4 #7, 18, 21, 23, 25, 29, 40

1.9 C 2 inner variations

n f(x i ) x. i=1 In section 4.2, we defined the definite integral of f from x = a to x = b as n f(x i ) x; f(x) dx = lim i=1

Math 100 Review Sheet

MORE FUNCTION GRAPHING; OPTIMIZATION. (Last edited October 28, 2013 at 11:09pm.)

Math 61CM - Solutions to homework 9

Summary: Method of Separation of Variables

Polynomials and Division Theory

Line Integrals. Partitioning the Curve. Estimating the Mass

PHYSICS 116C Homework 4 Solutions

4181H Problem Set 11 Selected Solutions. Chapter 19. n(log x) n 1 1 x x dx,

Main topics for the First Midterm

MA Handout 2: Notation and Background Concepts from Analysis

Math 1102: Calculus I (Math/Sci majors) MWF 3pm, Fulton Hall 230 Homework 2 solutions

JUST THE MATHS UNIT NUMBER INTEGRATION APPLICATIONS 6 (First moments of an arc) A.J.Hobson

f(x) dx, If one of these two conditions is not met, we call the integral improper. Our usual definition for the value for the definite integral

US01CMTH02 UNIT Curvature

Improper Integrals. Type I Improper Integrals How do we evaluate an integral such as

Partial Derivatives. Limits. For a single variable function f (x), the limit lim

Question 1: Figure 1: Schematic

Electromagnetism Answers to Problem Set 10 Spring 2006

Name Solutions to Test 3 November 8, 2017

Higher Checklist (Unit 3) Higher Checklist (Unit 3) Vectors

Math 5440 Problem Set 3 Solutions

Physics 9 Fall 2011 Homework 2 - Solutions Friday September 2, 2011

Quantum Physics II (8.05) Fall 2013 Assignment 2

. Double-angle formulas. Your answer should involve trig functions of θ, and not of 2θ. cos(2θ) = sin(2θ) =.

1.3 The Lemma of DuBois-Reymond

Exam 2, Mathematics 4701, Section ETY6 6:05 pm 7:40 pm, March 31, 2016, IH-1105 Instructor: Attila Máté 1

63. Representation of functions as power series Consider a power series. ( 1) n x 2n for all 1 < x < 1

Math 5440 Problem Set 3 Solutions

MASTER CLASS PROGRAM UNIT 4 SPECIALIST MATHEMATICS WEEK 11 WRITTEN EXAMINATION 2 SOLUTIONS SECTION 1 MULTIPLE CHOICE QUESTIONS

Integration Techniques

We partition C into n small arcs by forming a partition of [a, b] by picking s i as follows: a = s 0 < s 1 < < s n = b.

10 Vector Integral Calculus

Problem Set 3 Solutions

PH12b 2010 Solutions HW#3

6.5 Numerical Approximations of Definite Integrals

PHYS 601 HW3 Solution

Math 473: Practice Problems for the Material after Test 2, Fall 2011

HIGHER SCHOOL CERTIFICATE EXAMINATION MATHEMATICS 4 UNIT (ADDITIONAL) Time allowed Three hours (Plus 5 minutes reading time)

Chapter 5. , r = r 1 r 2 (1) µ = m 1 m 2. r, r 2 = R µ m 2. R(m 1 + m 2 ) + m 2 r = r 1. m 2. r = r 1. R + µ m 1

Math 426: Probability Final Exam Practice

Introduction to the Calculus of Variations

Chapter 4 Contravariance, Covariance, and Spacetime Diagrams

. Double-angle formulas. Your answer should involve trig functions of θ, and not of 2θ. sin 2 (θ) =

Problem Set 3

MATH34032: Green s Functions, Integral Equations and the Calculus of Variations 1

MATH 253 WORKSHEET 24 MORE INTEGRATION IN POLAR COORDINATES. r dr = = 4 = Here we used: (1) The half-angle formula cos 2 θ = 1 2

THE EXISTENCE-UNIQUENESS THEOREM FOR FIRST-ORDER DIFFERENTIAL EQUATIONS.

The Regulated and Riemann Integrals

Jim Lambers MAT 280 Spring Semester Lecture 17 Notes. These notes correspond to Section 13.2 in Stewart and Section 7.2 in Marsden and Tromba.

Math 231E, Lecture 33. Parametric Calculus

Chapter 4. Additional Variational Concepts

Jackson 2.26 Homework Problem Solution Dr. Christopher S. Baird University of Massachusetts Lowell

f(a+h) f(a) x a h 0. This is the rate at which

Line Integrals. Chapter Definition

(uv) = u v + uv, (1) u vdx + b [uv] b a = u vdx + u v dx. (8) u vds =

Section 17.2 Line Integrals

7.1 Integral as Net Change and 7.2 Areas in the Plane Calculus

ACM 105: Applied Real and Functional Analysis. Solutions to Homework # 2.

ntegration (p3) Integration by Inspection When differentiating using function of a function or the chain rule: If y = f(u), where in turn u = f(x)

Jackson 2.7 Homework Problem Solution Dr. Christopher S. Baird University of Massachusetts Lowell

Phys 7221, Fall 2006: Homework # 6

Reversing the Chain Rule. As we have seen from the Second Fundamental Theorem ( 4.3), the easiest way to evaluate an integral b

TABLE OF CONTENTS 3 CHAPTER 1

Problem set 1: Solutions Math 207B, Winter 2016

SOLUTIONS FOR ADMISSIONS TEST IN MATHEMATICS, COMPUTER SCIENCE AND JOINT SCHOOLS WEDNESDAY 5 NOVEMBER 2014

14.4. Lengths of curves and surfaces of revolution. Introduction. Prerequisites. Learning Outcomes

Further integration. x n nx n 1 sinh x cosh x log x 1/x cosh x sinh x e x e x tan x sec 2 x sin x cos x tan 1 x 1/(1 + x 2 ) cos x sin x

ES.181A Topic 8 Notes Jeremy Orloff

Jack Simons, Henry Eyring Scientist and Professor Chemistry Department University of Utah

7.2 The Definite Integral

Mathematics Extension 2

df dt f () b f () a dt

NUMERICAL INTEGRATION. The inverse process to differentiation in calculus is integration. Mathematically, integration is represented by.

Chapter 5 Bending Moments and Shear Force Diagrams for Beams

APPLICATIONS OF THE DEFINITE INTEGRAL

First midterm topics Second midterm topics End of quarter topics. Math 3B Review. Steve. 18 March 2009

Definition of Continuity: The function f(x) is continuous at x = a if f(a) exists and lim

Improper Integrals, and Differential Equations

Data Provided: A formula sheet and table of physical constants is attached to this paper. DEPARTMENT OF PHYSICS & Autumn Semester ASTRONOMY

Transcription:

Solutions to Homework Set 3 1 Bent brs: First recll some elementry clculus results: the curvture κ, nd the rdius R of the osculting circle, t point (x, y on curve y(x re given by κ = 1 R = dψ = 1 d tn 1 y 1 + y 2 dx = y (1 + y 2 3/2 Here the rc length s nd the ngle ψ between the curve nd the x xis constitute the intrinisic coordintes of the curve y R ψ x Osculting circle nd intrinsic coordintes For ll prts of the present problem y is ssumed smll enough tht we cn get wy with the pproximtion R 1 = y Euler s problem: We observe tht if rod of fixed length L is bent into curve y(z, we hve 2 = dz 2 + dy 2, dz = ( 1 ẏ 2 = 1 2ẏ2 1 + Here the overdot indictes differentition with respect to the rc-length s For curves with smll y, we my pproximte y = ẏ nd dz in the lst expression The length of the projection of the rod on the z xis is therefore L 1 2 y 2 dz Combining the resulting expresion for the potentil energy of the lod with the bending energy gives the functionl U[y] Inserting the mode expnsion for y(z nd doing the integrl gives U[y] = L { ( Y I n 2 4 π 4 n Mg ( } n 2 π 2 2 2 L 4 2 L 2 n=1 The coefficient of 2 n is negtive when Mg > n2 π 2 Y I/L 2 We thus see tht the coefficient of 2 1 is the first to go negtive, mking n = 1 mode unstble, nd this occurs t when Mg = π 2 Y I/L 2 1

b Leonrdo d Vinci s problem: The strength of cntilever ws discussed by Glileo in his Dilogue Concerning Two New Sciences published 1654 His resoning ws not quite complete however Surprisingly, more correct nlysis of the problem hd been given by Leonrdo d Vinci more thn century erlier The energy is This is minimum when = δe = The drwing from Glileo s Dilogue E[y] = Y I 2 (y 2 dx + Mgy(L Y Iy (4 δy(x dx + Y I[y δy y δy] L + Mg δy(l for ny vrition δy(x At the wll end, x =, we re told tht y( = y ( = The displcement therefore stisfies y (4 =, with these boundry conditions Thus, we know tht the minimum energy configurtion will be of the form y(x = x 2 + bx 3, but do not yet know the constnts nd b Now consider the integrted-out terms t the weight end: Y Iy (Lδy (L (Y Iy (L Mgδy(L Even though we hve mde Y Iy(4 δy(x dx vnish, we cn still vry y(l nd y (L independently by vrying the s-yet-unknown constnts nd b: δy(l = L 2 δ + L 3 δb, δy (L = 2L δ + 3L 2 δb The vritions re independent becuse given ny desired δy(l nd δy (L, we cn solve for the necessry δ, δb s δ = 3L 2 δy(l 2L 3 δy (L, δb = L 1 δy(l + L 2 δy (L 2

Therefore, in the minimum-energy configurtion, the coefficients of δy(l nd δy (L must vnish seprtely, giving the boundry conditions The unique solution is y (L =, Y Iy (L = Mg y(x = Mg Y I Thus y(l = 1 3 MgL3 /Y I Note tht ( 1 6 x3 1 2 Lx2 Y Iy (x = Mg(x L The right-hnd-side of this lst eqution is the bending moment of the weight on the section of the rod t x The mximum bending moment occurs right where the rod enters the wll, nd this is where the cntilever would brek were the weight too lrge Lgrnge multipliers Recll tht finding the sttionry points of x Tx subject to the condition x x = 1 reduces to the problem of finding the normlized eigenvectors of the mtrix T The given qudrtic form is 13x 2 + 8xy + 7y 2 = ( x, y We therefore hve to digonlize the mtrix ( 13 4 T = 4 7 ( 13 4 4 7 ( x y It is possible to digonlize 2 2 mtrix lmost by inspection We begin by observing tht product of the eigenvlues is The sum of the eigenvlues is dett = 13 7 4 4 = 75 trt = 13 + 7 = 2 The eigenvlues re therefore λ = 5 nd λ = 15 The esiest wy to find the eigenvectors is to use Dirc s trick (see the ppendix in the notes to decompose the identity mtrix into opertors P λ tht project onto the eigenvectors corresponding to eigenvlue λ: The projection opertors re therefore (T 5I (T 15I I = + 15 5 (5 15 = P 15 + P 5 (1 P 5 = 1 1 (15I T, P 15 = 1 (T 5I 1 3

We cn project from lmost ny vector, so let s use v = (, 1 t The eigenvector corresponding to λ = 15 is proportionl to ( ( ( 8 4 4 (T 5Iv = = 4 2 1 2 After normlizing we find tht there re sttionry points t x = ±2/ 5, y = ±1/ 5, t which f(x, y = 15 Similrly, the eigenvector corresponding to λ = 5 is proportionl to ( ( ( 2 4 4 (15I Tv = =, 4 8 1 8 so the other sttionry points re t x = 1/ 5, y = ±2/ 5, t which f(x, y = 5 Ctenry gin: We seek to mke sttionry { F[x, y] = ρgy + 1 } 2 λ(s(ẋ2 + ẏ 2 1 Prt : Since the en of the chin re fixed, we cn discrd ny integrted out terms, nd so hve { δf = δx(s ( d (λ(sẋ + δy(s (ρg d } (λ(sẏ The potentil energy is therefore sttionry when = δf δx(s = δf δy(s d (λ(sẋ ρg d (λ(sẏ Tking into count the condition ẋ 2 + ẏ 2 = 1, which tells us tht s is the rc-length, we cn set ẋ = cos ψ nd ẏ = sin ψ, where ψ is the intrinsic coordinte Thus = d (λ(s cosψ ρg = d (λ(s sinψ The figure shows tht these re the conditions for the equilibrium of ech infinitesiml segment of the chin, with λ(s T(s being the tension t point s T(s+ ψ(s+ ψ(s ρ g T(s The free body digrm for the forces cting on segment of chin of length 4

The horizontl component of the force [T(s cosψ] s+ s must vnish, while the verticl component blnce is [T(s sin ψ] s+ s d (λ(s cosψ d (λ(s sinψ = ρg Prt b: The geometry tells us tht ψ = s/ We know tht T(s cosψ is constnt, C sy, nd so ρ(sg = d ( ( s C tn = C ( s sec2 (2 The constnt C is fixed by mking Mg = π/4 π/4 C ( s sec2 = C[tnψ] π/4 π/4 = 2C Thus ρ(s = M 2 sec2 ( s 5