ENGI 4430 Parametric Vector Functions Page 2-01

Similar documents
ENGI 4430 Parametric Vector Functions Page dt dt dt

Chapter 9 Vector Differential Calculus, Grad, Div, Curl

MODULE 1. e x + c. [You can t separate a demominator, but you can divide a single denominator into each numerator term] a + b a(a + b)+1 = a + b

Figure 1a. A planar mechanism.

Phys101 Final Code: 1 Term: 132 Wednesday, May 21, 2014 Page: 1

Building to Transformations on Coordinate Axis Grade 5: Geometry Graph points on the coordinate plane to solve real-world and mathematical problems.

and the Doppler frequency rate f R , can be related to the coefficients of this polynomial. The relationships are:

Flipping Physics Lecture Notes: Simple Harmonic Motion Introduction via a Horizontal Mass-Spring System

ENGI Parametric Vector Functions Page 5-01

Work, Energy, and Power

Equilibrium of Stress

Phys101 First Major-131 Zero Version Coordinator: Dr. A. A. Naqvi Wednesday, September 25, 2013 Page: 1

Yeu-Sheng Paul Shiue, Ph.D 薛宇盛 Professor and Chair Mechanical Engineering Department Christian Brothers University 650 East Parkway South Memphis, TN

Flipping Physics Lecture Notes: Simple Harmonic Motion Introduction via a Horizontal Mass-Spring System

Chapter 3 Kinematics in Two Dimensions; Vectors

Q1. A string of length L is fixed at both ends. Which one of the following is NOT a possible wavelength for standing waves on this string?

CHAPTER 8b Static Equilibrium Units

Pre-Calculus Individual Test 2017 February Regional

Chapter 5: Force and Motion I-a

Rigid Body Dynamics (continued)

Physics 212. Lecture 12. Today's Concept: Magnetic Force on moving charges. Physics 212 Lecture 12, Slide 1

Chapter 2 GAUSS LAW Recommended Problems:

1 Course Notes in Introductory Physics Jeffrey Seguritan

GAUSS' LAW E. A. surface

PHYS 314 HOMEWORK #3

Review for the final exam (Math 127)

AP Physics Kinematic Wrap Up

Kinetics of Particles. Chapter 3

Phys102 Second Major-102 Zero Version Coordinator: Al-Shukri Thursday, May 05, 2011 Page: 1

MATHEMATICS SYLLABUS SECONDARY 5th YEAR

Example 1. A robot has a mass of 60 kg. How much does that robot weigh sitting on the earth at sea level? Given: m. Find: Relationships: W

Finding the Earth s magnetic field

Solution to HW14 Fall-2002

. (7.1.1) This centripetal acceleration is provided by centripetal force. It is directed towards the center of the circle and has a magnitude

NUMBERS, MATHEMATICS AND EQUATIONS

Chapter 2. Kinematics in One Dimension. Kinematics deals with the concepts that are needed to describe motion.

Cambridge Assessment International Education Cambridge Ordinary Level. Published

Information for Physics 1201 Midterm I Wednesday, February 20

Physics 101 Math Review. Solutions

SAFE HANDS & IIT-ian's PACE EDT-04 (JEE) Solutions

14. Which shows the direction of the centripetal force acting on a mass spun in a vertical circle?

14. Which shows the direction of the centripetal force acting on a mass spun in a vertical circle?

Concept Category 2. Trigonometry & The Unit Circle

CHAPTER 6 -- ENERGY. Approach #2: Using the component of mg along the line of d:

= m. Suppose the speed of a wave on a string is given by v = Κ τμ

Phy 213: General Physics III 6/14/2007 Chapter 28 Worksheet 1

39th International Physics Olympiad - Hanoi - Vietnam Theoretical Problem No. 1 /Solution. Solution

UGANDA ADVANCED CERTIFICATE OF EDUCATION INTERNAL MOCK 2016 PURE MATHEMATICS. 3 hours

Surface and Contact Stress

LHS Mathematics Department Honors Pre-Calculus Final Exam 2002 Answers

Differentiation Applications 1: Related Rates

CHAPTER 6 WORK AND ENERGY

SPH3U1 Lesson 06 Kinematics

CHAPTER 1. Learning Objectives

ECE 2100 Circuit Analysis

Conceptual Dynamics SDC. An Interactive Text and Workbook. Kirstie Plantenberg Richard Hill. Better Textbooks. Lower Prices.

6.3: Volumes by Cylindrical Shells

37 Maxwell s Equations

Lecture 5: Equilibrium and Oscillations

Physics 321 Solutions for Final Exam

Lecture 7: Damped and Driven Oscillations

Math 302 Learning Objectives

ASTRODYNAMICS. o o o. Early Space Exploration. Kepler's Laws. Nicolaus Copernicus ( ) Placed Sun at center of solar system

Subject: KINEMATICS OF MACHINES Topic: VELOCITY AND ACCELERATION Session I

Faculty of Engineering and Department of Physics Engineering Physics 131 Midterm Examination February 27, 2006; 7:00 pm 8:30 pm

( ) ( ) Pre-Calculus Team Florida Regional Competition March Pre-Calculus Team Florida Regional Competition March α = for 0 < α <, and

Homology groups of disks with holes

Corrections for the textbook answers: Sec 6.1 #8h)covert angle to a positive by adding period #9b) # rad/sec

Study Guide Physics Pre-Comp 2013

Chapter 9 Uniform Circular Motion

LEARNING : At the end of the lesson, students should be able to: OUTCOMES a) state trigonometric ratios of sin,cos, tan, cosec, sec and cot

M thematics. National 5 Practice Paper B. Paper 1. Duration 1 hour. Total marks 40

Course Stabilty of Structures

205MPa and a modulus of elasticity E 207 GPa. The critical load 75kN. Gravity is vertically downward and the weight of link 3 is W3

Kinematic transformation of mechanical behavior Neville Hogan

Chapter 6. Dielectrics and Capacitance

Fall 2013 Physics 172 Recitation 3 Momentum and Springs

Q1. In figure 1, Q = 60 µc, q = 20 µc, a = 3.0 m, and b = 4.0 m. Calculate the total electric force on q due to the other 2 charges.

CLASS XI SET A PHYSICS

, which yields. where z1. and z2

Honors Physics Final Review Summary

WYSE Academic Challenge Regional Mathematics 2007 Solution Set

Physics 2010 Motion with Constant Acceleration Experiment 1

Pattern Recognition 2014 Support Vector Machines

Lecture 2: Single-particle Motion

Introduction: A Generalized approach for computing the trajectories associated with the Newtonian N Body Problem

Lyapunov Stability Stability of Equilibrium Points

Lecture 6: Phase Space and Damped Oscillations

Module 4: General Formulation of Electric Circuit Theory

Sections 15.1 to 15.12, 16.1 and 16.2 of the textbook (Robbins-Miller) cover the materials required for this topic.

Aircraft Performance - Drag

Phys101 Second Major-061 Zero Version Coordinator: AbdelMonem Saturday, December 09, 2006 Page: 1

Physics 2B Chapter 23 Notes - Faraday s Law & Inductors Spring 2018

Trigonometric Ratios Unit 5 Tentative TEST date

Computational modeling techniques

M thematics. National 5 Practice Paper C. Paper 1. Duration 1 hour. Total marks 40

Chapter 3. AC Machinery Fundamentals. Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Higher Mathematics Booklet CONTENTS

Math 105: Review for Exam I - Solutions

Transcription:

ENGI 4430 Parametric Vectr Functins Page -01. Parametric Vectr Functins (cntinued) Any nn-zer vectr r can be decmpsed int its magnitude r and its directin: r rrˆ, where r r 0 Tangent Vectr: dx dy dz dr T If the parameter t is time, then the tangent vectr is als the velcity vectr, d r dr v, whse magnitude is the speed v. T The unit tangent is T dr dr Arc Length In In : s x y 3 : s x y z s x y z t t t t dx dy dz dr The vectr d r pints in the directin f the tangent T t the curve defined parametrically by t r r. dr dr dr dr dr T T [unit tangent = rate f change f r with respect t distance travelled alng the curve.] [Hwever, arc length s is rarely a cnvenient parameter.]

ENGI 4430 Parametric Vectr Functins Page -0 Example.01 (a) Find the arc length alng the curve defined by T r 1 1 t 4 t sin t 4 cs t sin t, frm the pint where t = 0 t the pint where t = 4π. (b) Find the unit tangent T. dx 1 1 cs 1 cs sin sin 4 4 (a) t t t t dy 1 sin t sin t cs t sin t cs t 4 4 dz cst dr sin t sin t cs t cs t T dr sin 4 t sin t cs t cs t sin t sin t cs t cs t 1sin t cs t 1 1 L 1 t 0 0 4 4 4 0 Therefre L 4 (b) T dr dr dr But 1 t "fr all t". Therefre T sin t sin t cst cst [Nte that, in this example, t itself is the arc length frm the pint 0, 1 4, 0, (where t = 0). There are very few curves fr which the parameterizatin is this cnvenient!]

ENGI 4430 Parametric Vectr Functins Page -03 Arc Length fr a Plar Curve Fr a plar curve defined by r f x f cs y f sin. Using the abbreviatins,, the parameter is and r f, r f, c cs, s sin, dx dy rc rs and rs rc d d dx dy r c rrcs r s r s rrsc d d r c s r s c r d dr rc Therefre the arc length L alng the plar curve r f frm t is dr L r d d Example.0 Find the length L f the perimeter f the cardiid r 1 cs 0, r 1 cs 1 c dr sin s d dr r d 1 c c s c 1c

ENGI 4430 Parametric Vectr Functins Page -04 Example.0 (cntinued) But 1 cs x cs x. Set x x dr r cs d L cs d cs d 0 0 Using symmetry in the hrizntal axis, L cs d 4 cs d 4 sin 81 0 0 0 0 Therefre the perimeter f the cardiid curve is L = 8. Nte: Fr and, cs cs, nt cs 0 cs 0! d Example.03 Find the arc length alng the spiral curve r ae a 0, frm t. dr r ae ae d ae ae ae d L d a e d a e d L a e e

ENGI 4430 Parametric Vectr Functins Page -05 Overview f Nrmal and Binrmal: Fr a curve in, there is a unique nrmal line at every pint where the unit tangent vectr is defined: There are nly tw chices fr the unit nrmal vectr. N is chsen t pint in the directin in which the curve is turning. This definitin fails wherever the unit tangent des nt exist. This definitin als fails at all pints f inflexin and wherever the curve is a straight line. Hwever, fr a curve in 3, there is a nrmal plane at each pint, nt a nrmal line. Frm the infinite number f different directins fr a nrmal vectr, we need t identify a unique directin fr a principal nrmal. Again, we shall chse the directin in which the unit tangent vectr is turning at each pint. T 1 T T 1 Using the prduct rule f differentiatin, T T 0 T 0 d r T 0 T (Nte: a unit vectr can never be zer). Select the principal nrmal N t be the directin in which the unit tangent is, instantaneusly, changing: N N and N are therefre parallel t d T. The unit principal nrmal then fllws: N

ENGI 4430 Parametric Vectr Functins Page -06 The unit binrmal is at right angles t bth tangent and principal nrmal: B cnstant B TN the curve lies entirely in ne plane (the plane defined by T ˆ and N). ˆ The three vectrs frm an rthnrmal set (they are mutually perpendicular and each ne is a unit vectr; that is, magnitude = 1). All three unit vectrs are undefined where the curve suddenly reverses directin, (such as at a cusp). Curvature: The derivative f the unit tangent with respect t distance travelled alng a curve is the principal nrmal vectr, N. Its directin is the unit principal nrmal N. Its magnitude is a measure f hw rapidly the curve is turning and is defined t be the curvature: dr N N N 1 The radius f curvature is. The radius f curvature at a pint n a curve is the radius f the circle which best fits the curve at that pint. Example.01 (cntinued) s (c) Find the curvature at any pint fr which s 0, fr the curve 1 1 4 4 r s s sin s cs s sin s where s is the arc length frm the pint 0, 1 4, 0. T Frm part (b): sin s T sin scs s cs s

ENGI 4430 Parametric Vectr Functins Page -07 Example.01 (c) (cntinued) sin s cs s sin s N cs s sin s cs s sin s sin s s 1 sin s 1 1 1 sin s It then fllws that the unit principal nrmal vectr at every pint is sin s 1 N N cs s 1 sin s sin s A Maple plt f this curve is available frm the demnstratin files sectin f the web site, www.engr.mun.ca/~ggerge/4430/dems/index.html.

ENGI 4430 Parametric Vectr Functins Page -08 Anther frmula fr curvature: Let d r and d r r s r, then d r d r T r s T r st s (prduct rule f differentiatin) But N s 3 rr st s T s N 0 s B rr s 3, but s r. Therefre r r 3 r If the parameter t is time, then the curvature frmula is als va 3 v where v v acceleratin. is the speed (scalar), the vectr v is the velcity and the vectr a is the

ENGI 4430 Parametric Vectr Functins Page -09 Example.04 Find the curvature and the radius f curvature fr the helix, given in parametric frm by x = cs t, y = sin t, z = t. Assume SI units. Let c = cs t, s = sin t. c s c r s c s v r a r t 1 0 ˆi s c s s r r ˆj c s c c kˆ 1 0 s c 1 rr s c 1 r s c 1 rr 1 3 r Therefre and 1 1 m cnstant 1 m

ENGI 4430 Parametric Vectr Functins Page -10 Surfaces f Revlutin Cnsider a curve in the x-y plane, defined by the equatin y = f (x). If it is swept nce arund the line y = c, then it will generate a surface f revlutin. At any particular value f x, a thin crss-sectin thrugh that surface, parallel t the y-z plane, will be a circular disc f radius r, where r f x c Let us nw view the circular disc face-n, (s that the x axis and the axis f rtatin are bth pinting directly ut f the page and the page is parallel t the y-z plane). Let (x, y, z) be a general pint n the surface f revlutin. Frm this diagram, ne can see that r yc z Therefre, the equatin f the surface generated, when the curve y = f (x) is rtated nce arund the axis y = c, is y c z f x c Special case: When the curve y = f (x) is rtated nce arund the x axis, the equatin f the surface f revlutin is r y z f x y z f x

ENGI 4430 Parametric Vectr Functins Page -11 Example.05 Find the equatin f the surface generated, when the parabla the x axis. y 4ax is rtated nce arund The slutin is immediate: the equatin f the surface is y z 4ax, 4 f x ax which is the equatin f an elliptic parablid, (actually a special case, a circular parablid). A Maple wrksheet fr this surface is available frm the demnstratin files sectin f the ENGI 4430 web site. The Curved Surface Area f a Surface f Revlutin Fr a rtatin arund the x axis, the curved surface area swept ut by the element f arc length s is apprximately the prduct f the circumference f a circle f radius y with the length s. A y s Integrating alng a sectin f the curve y = f (x) frm x = a t x = b, the ttal curved surface area is xb A f x xa Fr a rtatin f y = f (x) abut the axis y = c, the curved surface area is xb A f x c f x c dx xa a dx Therefre and b b A f x c 1 f x dx a dy 1 dx dx

ENGI 4430 Parametric Vectr Functins Page -1 Example.06 Find the curved surface area f the circular parablid generated by rtating the prtin f the y 4cx c 0 x a 0 x b a abut the x axis. parabla frm t A xb y xa b a y dx dx d d [Chain rule:] dx dx y 4cx y 4cx y y 4c y c y 4 4 1 dy 1 c 1 c x c dx dx y 4cx x A b a c x x c x 1/ dx 4 c x c dx b a Therefre x c 3/ 4 c 3 b a 8 c A b c a c 3 3/ 3/

ENGI 4430 Parametric Vectr Functins Page -13 Area Swept Out by a Plar Curve r = f (θ) A Area f triangle 1 r r r sin But the angle is small, s that sin and the increment r is small cmpared t r. Therefre 1 A r A 1 r d Example.07 Find the area f a circular sectr, radius r, angle. r = cnstant, 1 1 1 A r d r r Therefre A 1 r Full circle: A r.

ENGI 4430 Parametric Vectr Functins Page -14 Example.08 Find the area swept ut by the plar curve r ae ver, (where a 0 and ). The cnditin prevents the same area being swept ut mre than nce. If then ne nee t subtract areas that have been cunted mre than nce [the red area in the diagram] 1 1 e A a e d a Therefre a A e e 4 In general, the area bunded by tw plar curves and is r f and r g and the radius vectrs 1 A f g d

ENGI 4430 Parametric Vectr Functins Page -15 Radial and Transverse Cmpnents f Velcity and Acceleratin At any pint P (nt at the ple), the unit radial vectr ˆr pints directly away frm the ple. The unit transverse vectr ˆθ is rthgnal t ˆr and pints in the directin f increasing θ. vectrs frm an rthnrmal basis fr. Unlike the Cartesian î and ĵ, if θ is nt cnstant then ˆr and ˆθ will be variable unit vectrs. Examine ˆr and ˆθ at tw nearby times t and t t: These The magnitudes f the unit vectrs can never change. By definitin, the magnitude f any unit vectr is always 1. Only the directins can change. Examine the difference in the unit radial vectr at these tw times. The tw lnger sides f this issceles triangle are bth 1 r ˆ. The tw larger angles are each equal t /. Clearly the angle between r ˆ t and the incremental vectr r ˆ appraches a right angle as t (and therefre ) appraches zer. ˆ t ˆ t. Therefre the derivative f r is parallel t Sine rule: Als, frm triangle gemetry (the sine rule), rˆ rˆ and r ˆ 1 (unit vectr) sin sin / As t 0, sin and sin / sin / 1 rˆ 1 rˆ drˆ d drˆ d ˆ 1 t t a b c sin A sin B sin C

ENGI 4430 Parametric Vectr Functins Page -16 d ˆ ( is parallel t Als, frm triangle gemetry (the sine rule), ˆ ˆ sin sin / Nw examine the difference in the unit transverse vectr at these tw times. The tw lnger sides f this issceles triangle are bth 1. Clearly the angle between ˆ t and the incremental vectr ˆ appraches a right angle as t (and therefre ) appraches zer. Therefre the derivative f ˆ t pints radially inwar r ˆ t ). and ˆ 1 As t 0, sin and sin / sin / 1 ˆ 1 ˆ d ˆ d d ˆ d rˆ 1 t t Therefre the derivatives f the tw [nn-cnstant] plar unit vectrs are drˆ d ˆ and d ˆ d ˆ r Using the verdt ntatin t represent differentiatin with respect t the parameter t, these results may be expressed mre cmpactly as rˆ ˆ and ˆ rˆ The radial and transverse cmpnents f velcity and acceleratin then fllw: r r rˆ v r r rˆ r rˆ r rˆ r ˆ v r and v r radial transverse r rˆ r rˆ ˆ ˆ ˆ r r r a v r r rˆ r ˆ r ˆ r rˆ r r rˆ r r ˆ a radial a transverse 1 d r The transverse cmpnent f acceleratin can als be written as atr r

ENGI 4430 Parametric Vectr Functins Page -17 Example.09 A particle fllws the path r, where the angle at any time is equal t the time: t 0. Find the radial and transverse cmpnents f acceleratin. r t r 1 r 0 v r rˆ r ˆ rˆ t ˆ v 1 t ˆ a r r r r r ˆ t rˆ ˆ Therefre a 4 t ar t and atr Example.10 Fr circular mtin arund the ple, with cnstant radius r and cnstant angular velcity, the velcity vectr is purely tangential, v r ˆ, and the acceleratin vectr is ˆ a r r r r r r r which matches the familiar result that centrifugal r centripetal acceleratin radially inward. ˆ ˆ r, directed

ENGI 4430 Parametric Vectr Functins Page -18 Tangential and Nrmal Cmpnents f Velcity and Acceleratin d Frm page.01, we knw that the velcity vectr is als the tangent vectr, vt r. dr The [scalar] speed is v v The speed is therefre the derivative with respect t time f distance travelled alng the curve. It fllws that v vt - the speed is als the tangential cmpnent f the velcity vectr. There are n cmpnents f velcity in the nrmal directins. The acceleratin vectr is dv d a v T But dv T v d d T T N N and v v N dv a T v N att an N Therefre the tangential cmpnent f acceleratin is the rate f change f speed (nt velcity) and is psitive if the particle is speeding up, negative if it is slwing dwn and zer if the speed is cnstant. It is als a ˆ T at va. v The nrmal cmpnent f acceleratin (in the directin f the unit principal nrmal) is never negative; bth the curvature and v are nn-negative at all times. There is never any cmpnent f acceleratin in the binrmal directin. dv dv dv Usually it is easiest t evaluate a a a and at first, then t find the nrmal cmpnent (and hence the curvature) frm a a a N T

ENGI 4430 Parametric Vectr Functins Page -19 Example.04 (cntinued) Find the tangential and nrmal cmpnents f velcity and acceleratin fr a particle travelling alng the helix, given in parametric frm by x = cs t, y = sin t, z = t. Hence find the curvature. Assume SI units. Frm page.09, cst sin t cst d d t sin t r cst v r sin t v a t 1 0 dv vt v t t a sin cs 1 T 0 The acceleratin is therefre purely nrmal. a t t a a a a cs sin 0 1 N T 1 Therefre t t v T ms and a 0T 1N ms 1 1 an v 1 and v m 1

ENGI 4430 Parametric Vectr Functins Page -0 Review f Lines [frm MATH 050] Given a pint,, P x y z knwn t be n a line L, a nn-zer vectr T and vectrs T d abc parallel t the line, r x y z and T OP x y z r, the equatins f the line may be expressed in the vectr frm r r d t t, r, prvided nne f a, b, c are zer, in the symmetric Cartesian frm x x y y z z a b c If, fr example, b = 0, but a and c are nn-zer, then the Cartesian frm becmes y y, x x z z a c Example.11 Find the Cartesian equatin f the line thrugh the pints (1, 3, 5) and (4, 1, 7). The vectr cnnecting the tw pints is an bvius chice fr the line directin vectr. a 4 1 3 d b 1 3 4 c 7 5 Either pint may be chsen as P. r x 1 y 3 z 5 The equatin f the line is x 1 y 3 z 5 3 4

ENGI 4430 Parametric Vectr Functins Page -1 Review f Planes [frm MATH 050] A plane is defined by tw vectrs [ is seen here edge-n ]. Its rientatin is determined by a nn-zer nrmal vectr T n A B C. Its lcatin is determined by the psitin vectr T OP x y z r f any ne pint P knwn t be n the plane. The vectr T r x y z is then the psitin vectr f a pint n the plane if and nly if r, equivalently, r n r n Ax By Cz D 0 where D r n Ax By Cz If u and v are tw nn-zer vectrs nt parallel t each ther and bth parallel t the plane, then a vectr parametric frm f the equatin f the plane is r r su t v, s, t The nrmal vectr t the plane is n u v, frm which the ther tw frms abve fllw. Example.1 Find the Cartesian equatin f the plane thrugh the pints (0, 3, 5), (, 4, 5) and (4, 1, 7) and find the equatin f the nrmal line t that plane that passes thrugh the rigin. The three pints define three vectrs, n pair f which are parallel t each ther but all three f which are parallel t the plane. Any tw f them will serve as vectrs u and v. 0 4 0 4 u 4 3 1 and 1 3 4 v 5 5 0 7 5 1 ˆi 1 1 n u v ˆj 1 kˆ 0 1 6 6

ENGI 4430 Parametric Vectr Functins Page - Example.1 (cntinued) Any nn-zer multiple f this vectr will als serve as a nrmal vectr t the plane. Therefre select n 1 6 T. Any f the three pints will serve as P. Chse r T 0 3 5 1 0 nr 3 0 6 30 36 6 5 The equatin f the plane is n r n r x y 6z 36 We can quickly check that all three given pints satisfy this equatin: 0 + (3) + 6(5) = 6 + 30 = 36 + (4) + 6(5) = + 8 + 30 = 36 4 + ( 1) + 6(7) = 4 + 4 = 36 The directin vectr fr the nrmal line is just the nrmal vectr t the plane, d n 1 6 T r 0 (the line passes thrugh the rigin). The equatins f the nrmal line fllw immediately x 0 y 0 z 0 1 6 [End f Chapter ]