Lecture 5: Equilibrium and Oscillations

Similar documents
Lecture 6: Phase Space and Damped Oscillations

Lecture 7: Damped and Driven Oscillations

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

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

Solution to HW14 Fall-2002

AP Physics Kinematic Wrap Up

Kinematic transformation of mechanical behavior Neville Hogan

Kinetics of Particles. Chapter 3

Chapter 3 Kinematics in Two Dimensions; Vectors

Physics 321 Solutions for Final Exam

CHAPTER 8b Static Equilibrium Units

Study Guide Physics Pre-Comp 2013

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

Equilibrium of Stress

1 Course Notes in Introductory Physics Jeffrey Seguritan

Trigonometric Ratios Unit 5 Tentative TEST date

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

PHYS 219 Spring semester Lecture 02: Coulomb s Law how point charges interact. Ron Reifenberger Birck Nanotechnology Center Purdue University

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

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

PHYS 314 HOMEWORK #3

PHYSICS 151 Notes for Online Lecture #23

Calculus Placement Review. x x. =. Find each of the following. 9 = 4 ( )

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

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

Honors Physics Final Review Summary

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

1 PreCalculus AP Unit G Rotational Trig (MCR) Name:

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

Chapter 5: Force and Motion I-a

Review for the final exam (Math 127)

Work, Energy, and Power

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

Rigid Body Dynamics (continued)

CESAR Science Case The differential rotation of the Sun and its Chromosphere. Introduction. Material that is necessary during the laboratory

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

x x

Lecture 2: Single-particle Motion

Interference is when two (or more) sets of waves meet and combine to produce a new pattern.

Chapter 9 Vector Differential Calculus, Grad, Div, Curl

ENGI 4430 Parametric Vector Functions Page 2-01

Plan o o. I(t) Divide problem into sub-problems Modify schematic and coordinate system (if needed) Write general equations

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

Q x = cos 1 30 = 53.1 South

Fall 2013 Physics 172 Recitation 3 Momentum and Springs

Physics 2010 Motion with Constant Acceleration Experiment 1

Thermodynamics Partial Outline of Topics

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

making triangle (ie same reference angle) ). This is a standard form that will allow us all to have the X= y=

Chemistry 20 Lesson 11 Electronegativity, Polarity and Shapes

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

Matter Content from State Frameworks and Other State Documents

Preparation work for A2 Mathematics [2017]

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

f = µ mg = kg 9.8m/s = 15.7N. Since this is more than the applied

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

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

Introduction to Spacetime Geometry

37 Maxwell s Equations

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

Aircraft Performance - Drag

Harmonic Motion (HM) Oscillation with Laminar Damping

CLASS XI SET A PHYSICS

Computational modeling techniques

Thermodynamics and Equilibrium

Function notation & composite functions Factoring Dividing polynomials Remainder theorem & factor property

Lab 11 LRC Circuits, Damped Forced Harmonic Motion

Figure 1a. A planar mechanism.

Surface and Contact Stress

Physics 101 Math Review. Solutions

CHAPTER 6 WORK AND ENERGY

AP CHEMISTRY CHAPTER 6 NOTES THERMOCHEMISTRY

CHAPTER 5. Solutions for Exercises

Dispersion Ref Feynman Vol-I, Ch-31

WYSE Academic Challenge Sectional Physics 2007 Solution Set

ELECTRON CYCLOTRON HEATING OF AN ANISOTROPIC PLASMA. December 4, PLP No. 322

LHS Mathematics Department Honors Pre-Calculus Final Exam 2002 Answers

Electric Current and Resistance

I. Analytical Potential and Field of a Uniform Rod. V E d. The definition of electric potential difference is

Computational modeling techniques

Department of Economics, University of California, Davis Ecn 200C Micro Theory Professor Giacomo Bonanno. Insurance Markets

Part a: Writing the nodal equations and solving for v o gives the magnitude and phase response: tan ( 0.25 )

Cop yri ht 2006, Barr Mabillard.

This section is primarily focused on tools to aid us in finding roots/zeros/ -intercepts of polynomials. Essentially, our focus turns to solving.

Preparation work for A2 Mathematics [2018]

L a) Calculate the maximum allowable midspan deflection (w o ) critical under which the beam will slide off its support.

We can see from the graph above that the intersection is, i.e., [ ).

Higher. Specimen NAB Assessment

AP Physics. Summer Assignment 2012 Date. Name. F m = = + What is due the first day of school? a. T. b. = ( )( ) =

Lyapunov Stability Stability of Equilibrium Points

Professional Development. Implementing the NGSS: High School Physics

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

SPH3U1 Lesson 06 Kinematics

Hooke s Law (Springs) DAVISSON. F A Deformed. F S is the spring force, in newtons (N) k is the spring constant, in N/m

ENGI 1313 Mechanics I

Putting Scientific Notation to Work

ECE 2100 Circuit Analysis

EEO 401 Digital Signal Processing Prof. Mark Fowler

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?

Lecture 13: Electrochemical Equilibria

Transcription:

Lecture 5: Equilibrium and Oscillatins

Energy and Mtin Last time, we fund that fr a system with energy cnserved, v = ± E U m ( ) ( ) One result we see immediately is that there is n slutin fr velcity if E < U This represents a frbidden regin fr the particle

With this knwledge, we can quickly determine whether a particle s mtin is bunded r nt: E U(X) E E 3 E 4 E 5 0 5 3 4 6 7 8

Equilibrium If several frces are acting n a system, it is ften imprtant t understand the situatin in which all f them cancel t zer this is called equilibrium If all the frces are cnservative, equilibria ccur when F = U = s we can determine the equilibrium psitins frm the ptential alne Fr eample, cnsider the ne-dimensinal ptential belw: 0 U(X) = equilibrium pint

There are three distinct varieties f equilibria. The tw that ccur mst ften are:. Stable: in this case, when an bject is displaced frm the equilibrium psitin, it will tend t mve back twards equilibrium. Unstable: In this case, an bject displaced frm equilibrium will accelerate away frm the equilibrium psitin T determine whether and equilibrium is stable r unstable, we Taylr-epand the ptential near the equilibrium pint: du d U U ( ) = U ( ) + ( ) + ( ) 3 3 d U + ( ) 3 6 +

T simplify this further, nte that:. We can chse t set the rigin f the crdinate system at the equilibrium pint. We are free t set the value f the ptential t zer there 3. Since we re epanding abut an equilibrium pint, the first derivative must be zer. With all this, we have: 3 d U 3 d U U ( ) = 3 + + 6 Stability is determined by the sign f If it s psitive, equilibrium is at a lcal minimum f U Stable If it s negative, equilibrium is at a lcal maimum f U Unstable d U

What abut the case where d U = 0? Need t lk at leading nn-zer term in the epansin 3 d U 0 : Unstable 3 4 d U > 0 : Stable 4 4 d U < 0 : Unstable 4 If all terms in the epansin are 0, the equilibrium is neutral

Oscillatins Yu prbably remember studying the mtin f a mass attached t a spring that beys Hke s law: F = k where is the displacement frm the equilibrium length f the spring T understand why yu spent s much time n this, cnsider a general frce near a stable equilibrium pint Can be Taylr-epanded as: ( ) df d F = + + + F F 0 S, near the equilibrium pint, df F ( )

This is f the same frm as Hke s Law, with k df = S almst all small scillatins behave like a mass n a spring Thus it s imprtant t understand this type f mtin We start frm Newtn s secnd law: F = m = k k + ω = 0; ω m This is a straightfrward differential equatin a sine r csine functin fr (t) will wrk. General frm f result is: ( ) = Asin ( ω t δ ) t Amplitude Angular frequency Phase A and δ depend n initial cnditins; ω des nt

Energy f Oscillatr We can directly find the energy f the scillatr: ( E = T + U = m + k ) = + + + ( ( ) ( ) ) = ka cs ωt + δ + sin ωt + δ = ka ( mω cs( ) sin ( ) ) A ωt δ ka ωt δ Nte that this desn t depend n time Cnservatin f energy really wrks! The frequency and perid f scillatin are: ω k ν = = τ = = π π π m ν m k

Oscillatins in Multiple Dimensins The previus discussin was fine fr scillatin in a single dimensin In general, thugh, we want t deal with the situatin where: F = kr N big deal we can cnsider ne cmpnent at a time: F = m = k F = m = k S we just need t slve the same equatin as befre, nce fr each dimensin Slutins are: ( ) = sin ( ω + δ ) ( ) = sin ( ω + δ ) t A t t A t Nte that frequency is the same in each directin

The Tw-Dimensinal Case We can find the path taken by a particle underging twdimensinal scillatin Easiest if we start with a little trick rewrite as: ( ω δ δ δ ) ( ω δ ) ( δ δ ) ( ω δ ) ( δ δ ) = A sin t + + = A sin t + cs + cs t + sin = A cs + sin A A ( δ δ ) ( δ δ ) ( δ δ ) sin ( δ δ ) ( δ δ ) ( δ δ ) ( δ δ ) A sin ( δ δ ) A A cs = A A A A A cs + A cs = A A sin

Finally, we have: A A A cs δ δ + A = A A sin δ δ δ This is the equatin fr an ellipse ( ) ( ) Nte that the shape f the ellipse depends nly n the relative amplitudes and difference in phase between the mtin in each directin δ = δ δ = 0 30 δ δ = 90 δ δ 0 = δ δ = 80

Lissajus Curves The tw-dimensinal mtin becmes even mre interesting if the frequencies are different in each dimensin As lng as the rati f frequencies is a ratinal number, the mtin is still peridic: 7 ω = ω 5 δ δ = 90 Nte that there are 7 maima in and 5 maima in

If the rati f the tw frequencies is nt ratinal, the mtin wn t be peridic Eventually, every pint between in the rectangle defined by A and A will be reached: