Physics 141. Lecture 14. Frank L. H. Wolfs Department of Physics and Astronomy, University of Rochester, Lecture 14, Page 1

Similar documents
Physics 207: Lecture 20. Today s Agenda Homework for Monday

Linear Momentum. Center of Mass.

Week 8: Chapter 9. Linear Momentum. Newton Law and Momentum. Linear Momentum, cont. Conservation of Linear Momentum. Conservation of Momentum, 2

Week 11: Chapter 11. The Vector Product. The Vector Product Defined. The Vector Product and Torque. More About the Vector Product

Week 9 Chapter 10 Section 1-5

Physics 181. Particle Systems

Chapter 3 and Chapter 4

Chapter 11 Angular Momentum

Physics 207 Lecture 13. Lecture 13

Lecture 16. Chapter 11. Energy Dissipation Linear Momentum. Physics I. Department of Physics and Applied Physics

Conservation of Angular Momentum = "Spin"

10/23/2003 PHY Lecture 14R 1

10/9/2003 PHY Lecture 11 1

Angular Momentum and Fixed Axis Rotation. 8.01t Nov 10, 2004

Physics for Scientists and Engineers. Chapter 9 Impulse and Momentum

PHYSICS 231 Review problems for midterm 2

Week3, Chapter 4. Position and Displacement. Motion in Two Dimensions. Instantaneous Velocity. Average Velocity

Conservation of Energy

Physics 53. Rotational Motion 3. Sir, I have found you an argument, but I am not obliged to find you an understanding.

Recitation: Energy, Phys Energies. 1.2 Three stones. 1. Energy. 1. An acorn falling from an oak tree onto the sidewalk.

PY2101 Classical Mechanics Dr. Síle Nic Chormaic, Room 215 D Kane Bldg

1.3 Hence, calculate a formula for the force required to break the bond (i.e. the maximum value of F)

Study Guide For Exam Two

First Law: A body at rest remains at rest, a body in motion continues to move at constant velocity, unless acted upon by an external force.

CHAPTER 8 Potential Energy and Conservation of Energy

Chapter 8: Potential Energy and The Conservation of Total Energy

Chapter 8. Potential Energy and Conservation of Energy

Part C Dynamics and Statics of Rigid Body. Chapter 5 Rotation of a Rigid Body About a Fixed Axis

PHYS 1441 Section 002 Lecture #15

Chapter 7. Potential Energy and Conservation of Energy

Ground Rules. PC1221 Fundamentals of Physics I. Linear Momentum, cont. Linear Momentum. Lectures 17 and 18. Linear Momentum and Collisions

THERMAL DISTRIBUTION IN THE HCL SPECTRUM OBJECTIVE

Chapter 3. r r. Position, Velocity, and Acceleration Revisited

Physics 5153 Classical Mechanics. D Alembert s Principle and The Lagrangian-1

Physics 240: Worksheet 30 Name:

TIME OF COMPLETION NAME SOLUTION DEPARTMENT OF NATURAL SCIENCES. PHYS 2211, Exam 2 Section 1 Version 1 October 18, 2013 Total Weight: 100 points

Physics 111: Mechanics Lecture 11

coordinates. Then, the position vectors are described by

Chapter 11 Torque and Angular Momentum

11. Dynamics in Rotating Frames of Reference

Physics 231. Topic 8: Rotational Motion. Alex Brown October MSU Physics 231 Fall

Rigid body simulation

So far: simple (planar) geometries

Spring Force and Power

Chapter 07: Kinetic Energy and Work

Center of Mass and Linear Momentum

CHAPTER 7 ENERGY BALANCES SYSTEM SYSTEM. * What is energy? * Forms of Energy. - Kinetic energy (KE) - Potential energy (PE) PE = mgz

PHYS 1443 Section 002

Modeling of Dynamic Systems

PHYS 705: Classical Mechanics. Newtonian Mechanics

10/24/2013. PHY 113 C General Physics I 11 AM 12:15 PM TR Olin 101. Plan for Lecture 17: Review of Chapters 9-13, 15-16

in state i at t i, Initial State E = E i

Physics 207 Lecture 6

Please initial the statement below to show that you have read it

Important Dates: Post Test: Dec during recitations. If you have taken the post test, don t come to recitation!

CHAPTER 10 ROTATIONAL MOTION

A particle in a state of uniform motion remain in that state of motion unless acted upon by external force.

Page 1. Physics 131: Lecture 14. Today s Agenda. Things that stay the same. Impulse and Momentum Non-constant forces

Spring 2002 Lecture #13

Moments of Inertia. and reminds us of the analogous equation for linear momentum p= mv, which is of the form. The kinetic energy of the body is.

Rotational Dynamics. Physics 1425 Lecture 19. Michael Fowler, UVa

Classical Mechanics ( Particles and Biparticles )

Chapter 11: Angular Momentum

PHYS 1443 Section 004 Lecture #12 Thursday, Oct. 2, 2014

PHYS 1441 Section 002 Lecture #16

Linear Momentum. Center of Mass.

A Tale of Friction Basic Rollercoaster Physics. Fahrenheit Rollercoaster, Hershey, PA max height = 121 ft max speed = 58 mph

EN40: Dynamics and Vibrations. Homework 4: Work, Energy and Linear Momentum Due Friday March 1 st

Chapter 7: Conservation of Energy

Mechanics Cycle 3 Chapter 9++ Chapter 9++

ENGN 40 Dynamics and Vibrations Homework # 7 Due: Friday, April 15

Physics 231. Topic 8: Rotational Motion. Alex Brown October MSU Physics 231 Fall

SCHOOL OF COMPUTING, ENGINEERING AND MATHEMATICS SEMESTER 2 EXAMINATIONS 2011/2012 DYNAMICS ME247 DR. N.D.D. MICHÉ

Angular momentum. Instructor: Dr. Hoi Lam TAM ( 譚海嵐 )

AP Physics 1 & 2 Summer Assignment

GAUTENG DEPARTMENT OF EDUCATION SENIOR SECONDARY INTERVENTION PROGRAMME PHYSICAL SCIENCES GRADE 12 SESSION 1 (LEARNER NOTES)

Physics 106 Lecture 6 Conservation of Angular Momentum SJ 7 th Ed.: Chap 11.4

Physics 114 Exam 2 Fall 2014 Solutions. Name:

τ rf = Iα I point = mr 2 L35 F 11/14/14 a*er lecture 1

Period & Frequency. Work and Energy. Methods of Energy Transfer: Energy. Work-KE Theorem 3/4/16. Ranking: Which has the greatest kinetic energy?

Physics 114 Exam 3 Spring Name:

Physics 2A Chapters 6 - Work & Energy Fall 2017

Physics 2A Chapter 3 HW Solutions

Physics 3A: Linear Momentum. Physics 3A: Linear Momentum. Physics 3A: Linear Momentum. Physics 3A: Linear Momentum

Integrals and Invariants of Euler-Lagrange Equations

Physics 121. Thursday, February 28, Department of Physics and Astronomy, University of Rochester

Work is the change in energy of a system (neglecting heat transfer). To examine what could

EMU Physics Department

Physics 115. Molecular motion and temperature Phase equilibrium, evaporation

Gravitational Acceleration: A case of constant acceleration (approx. 2 hr.) (6/7/11)

Mechanics Physics 151

Physics 2A Chapter 9 HW Solutions

K = 100 J. [kg (m/s) ] K = mv = (0.15)(36.5) !!! Lethal energies. m [kg ] J s (Joule) Kinetic Energy (energy of motion) E or KE.

EN40: Dynamics and Vibrations. Homework 7: Rigid Body Kinematics

Week 6, Chapter 7 Sect 1-5

PHYS 1441 Section 001 Lecture #15 Wednesday, July 8, 2015

Conservation of Energy

Momentum. Momentum. Impulse. Momentum and Collisions

STATISTICAL MECHANICS

Lecture 20: Noether s Theorem

Transcription:

Physcs 141. Lecture 14. Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 1

Physcs 141. Lecture 14. Course Informaton: Lab report # 3. Exam # 2. Mult-Partcle Systems (Chapter 9): The center of mass of a mult-partcle system. The momentum prncple for mult-partcle systems. The energy prncple for multple-partcle systems. The moton of the center of mass and varable mass systems. Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 2

Course nformaton. Labs: Lab report # 3 wll be due on Frday October 28 at noon. Lab # 4 wll take place on Monday October 31 n B&L 407. Exam # 2: Date: Tuesday October 25 between 8 am and 9.30 am. Locaton: Hoyt. Chapters covered: 5, 6, 7, 8, and 9. Note: some sectons n Chapter 9 (those dealng wth rotatonal moton, moment of nerta, etc.) wll not be covered untl later n the course and wll appear on exam # 3. Detals wll be provded durng the exam revew. Format: same as exam # 1 (and yes, there wll be a non-physcs queston,.., but you know the answer). Revew: Frday 10/21 between 4 pm and 6 pm n B&L 106. Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 3

Rocket propulson. Observed n Hoyt. Notce the shadow of the exhaust on the screen. Projectle Moton. The launch Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 4

Rocket propulson. Observed n Hoyt. The collson Remanng exhaust. Frank L. H. Wolfs The destroyed rocket. Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 5

Locaton of the center of mass? In two or three dmensons the calculaton of the center of mass s very smlar, except that we need to use vectors. If we are not dealng wth dscreet pont masses we need to replace the sum wth an ntegral. r cm = 1 M V rdm Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 6

Moton of the center of mass. Non-relatvstc lmt. Ma cm can be rewrtten n terms of the forces on the ndvdual components: M a cm = d dt ( Mv cm ) = d P cm dt = F = F net,ext The moton of the center of mass s thus only determned by the external forces. Forces exerted by one part of the system on other parts of the system are nternal forces and the sum of all nternal forces cancels. Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 7

Moton of the center of mass. Lnear momentum. Now consder the specal case where there are no external forces actng on the system: d P tot dt = 0 Ths equatons tells us that the total lnear momentum of the system s constant. In the case of an extended object, we fnd the total lnear momentum by addng the lnear momenta of all of ts components: P tot = M v cm = m v = p Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 8

Systems wth varable mass. Rocket moton s an example of a system wth a varable mass: M ( t + dt) = M ( t) + dm As a result of dumpng the exhaust, the rocket wll ncrease ts velocty: v ( t + dt) = v ( t) + dv Mass of exhaust. dm < 0 kg Snce ths s an solated system, lnear momentum must be conserved. The ntal momentum s equal to p = M ( t)v ( t) Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 9

Systems wth varable mass. The fnal lnear momentum of the system s gven by p f = M ( t) + dm ( ) + dv ( )U ( )( v t ) + dm where U s the velocty of the exhaust. Conservaton of lnear momentum therefore requres that M ( t)v t ( ) = M ( t) + dm ( ) + dv ( )( v t ) + dm The exhaust has a fxed velocty U 0 wth respect to the engne. U 0 and U are related n the followng way: U U 0 = v ( t) + dv ( )U Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 10

Systems wth varable mass. Conservaton of lnear momentum can now be rewrtten as M ( t)v ( t) = M ( t) + dm ( ) + dv or We conclude ( )( v t ) + ( dm ) v t M ( t)v ( t) = M ( t) v t ( dm )U 0 = M ( t) ( dv) ( ( ) + dv +U 0 ) ( )+ dv ( dm )U 0 Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 11

Systems wth varable mass. The prevous equaton can be rewrtten as dm dt U 0 = M t ( ) dv ( t ) In ths equaton: dm/dt = -R where R s the rate of fuel consumpton. U 0 = -u where u s the (postve) velocty of the exhaust gasses relatve to the rocket. dv/dt s the acceleraton of the rocket. Ths equaton can be rewrtten as RU 0 = Ma rocket whch s called the frst rocket equaton. Ths equaton can be used to fnd the velocty of the rocket (second rocket equaton): v f = v + u ln M M f dt Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 12

Rocket propulson at the U or R. Introducng the Nmbus 4000. A unque present. See Mke Culver for orders. Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 13

3 Mnute 52 Second Intermsson Snce payng attenton for 1 hour and 15 mnutes s hard when the topc s physcs, let s take a 3 mnute 52 second ntermsson. You can: Stretch out. Talk to your neghbors. Ask me a quck queston. Enjoy the fantastc musc. Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 14

Energy of mult-partcle systems. Knetc and potental energy. In order to determne the (mechancal) energy of a multplepartcle system we need to determne both ts knetc energy and ts potental energy: The knetc energy of the system wll be the sum of the knetc energy of the center-of-mass and the knetc energy of the moton of the partcles wth respect to the center of mass. The potental energy of the system may or may not depend on the poston of the center of mass: The gravtatonal potental energy can be expressed n terms of the poston of the center of mass. The electrostatc potental energy depends on the poston of charges, not on the poston of mass, and does not depend on the poston of the center of mass. Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 15

Energy of mult-partcle systems. Knetc energy. The knetc energy of a multple-partcle system wll have two components: The translatonal component: the knetc energy assocated wth the moton of the center of mass. The relatve component: the knetc energy assocated wth the moton of the partcles wth respect to the center of mass. Ths type of moton an be vbratonal, rotatonal, a combnaton of these two, etc. The decomposton of the knetc energy nto ts components can be carred out wth a bt of effort. Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 16

Energy of mult-partcle systems. Knetc energy. Consder a mult-partcle system for whch we have specfed the poston of the center of mass r cm, and the poston of the partcle wth respect to the center of mass r. The knetc energy of partcle s equal to K = 1 2 m = 1 2 m d dt ( r cm + r ) 2 = 1 2 m v cm + v 2 ( v cm + v )( v cm + v ) = 1 2 m { v 2 cm + 2v cm v 2 + v } The total knetc energy of the system s thus equal to K = 1 2 m vcm2 + v cm m v + 1 2 m v 2 Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 17

Energy of mult-partcle systems. Knetc energy. K = 1 2 m vcm2 + v cm m v + 1 2 m v 2 v cm m v = v cm d dt m r = v cm d dt ( 0) = 0 1 2 m vcm2 = 1 2 Mvcm2 = K translatonal Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 18

Energy of mult-partcle systems. Knetc energy. We thus see that K = 1 2 Mv 2 + 1 cm 2 m v 2 = K translatonal + K relatve The relatve knetc energy (relatve to the center of mass of the system) can be equal to The vbratonal knetc energy (e.g. the vbratonal moton of atoms n an element). The rotatonal knetc energy (e.g. energy assocated wth the rotaton of a wheel)... Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 19

Energy of mult-partcle systems. Potental energy. Consder a mult-partcle system located close to the surface of the earth. The gravtatonal potental energy of ths system s equal to U = m gy = g m y = = gmy cm The gravtatonal potental energy thus depends on the vertcal poston of the center of mass of the system. Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 20

Conservaton of lnear momentum. An example. Two blocks wth mass m 1 and mass m 2 are connected by a sprng and are free to slde on a frctonless horzontal surface. The blocks are pulled apart and then released from rest. What fracton of the total knetc energy wll each block have at any later tme? m1 v1 v2 m2 Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 21

Conservaton of lnear momentum. An example. The system of the blocks and the sprng s a closed system, and the horzontal component of the external force s 0 N. The horzontal component of the lnear momentum s thus conserved. Intally the masses are at rest, and the total lnear momentum s thus 0 kg m/s. At any pont n tme, the veloctes of block 1 and block 2 are related: m1 v1 v2 m2 v 2 = m 1 m 2 v 1 Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 22

Conservaton of lnear momentum. An example. The knetc energes of mass m 1 and m 2 are thus equal to m1 v1 v2 m2 K 1 = 1 2 m v 2 1 1 K 2 = 1 2 m v 2 = 1 2 2 2 1 ( ) 2 = 1 2 m 2 m 2 v 2 m 1 ( ) 2 m 1 v 1 = m 1 K m 2 m 1 m 1 2 The fracton of the total knetc energy carred away by block 1 s equal to f 1 = K 1 K t = K 1 K 1 + K 2 = K 1 K 1 + m 1 m 2 K 1 = m 2 m 1 + m 2 Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 23

Next lecture: collsons. Conservaton of Lnear Momentum at RHIC (STAR Experment). Frank L. H. Wolfs Department of Physcs and Astronomy, Unversty of Rochester, Lecture 14, Page 24