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Global Global edition edition For these Global editions, the editorial team at Pearson has collaborated with educators across the world to address a wide range P of subjects and requirements, equipping students with the best possible h y learning tools. this Global edition preserves the cutting-edge approach s A i c and pedagogy of the original, but also features alterations, customization, S s t r and adaptation from the north american version. at fo e g r ic A S p c p i r e o a n c h t i w s it t h s M a o n d e d rn e P h n y g s ic i s n e Physics for Scientists and engineers e r s A Strategic Approach with Modern Physics eF do itU ir FoUrth edition ot nh randall d. Knight K n i g this is a special edition of an established title widely h t used by colleges and universities throughout the world. Pearson published this exclusive edition for the benefit of students outside the United States and Canada. if you purchased this book within the United States or Canada, edGl you should be aware that it has been imported without ito iob a the approval of the Publisher or author. nl Pearson Global Edition Knight_04_1292157429_Final.indd 1 16/07/16 10:43 AM Useful Data Me Mass of the earth 5.98*1024 kg Re Radius of the earth 6.37*106 m g Free-fall acceleration on earth 9.80 m/s2 G Gravitational constant 6.67*10-11 N m2/kg2 kB Boltzmann’s constant 1.38*10-23 J/K R Gas constant 8.31 J/mol K NA Avogadro’s number 6.02*1023 particles/mol T0 Absolute zero -273°C s Stefan-Boltzmann constant 5.67*10-8 W/m2 K4 p Standard atmosphere 101,300 Pa atm v Speed of sound in air at 20°C 343 m/s sound mp Mass of the proton (and the neutron) 1.67*10-27 kg me Mass of the electron 9.11*10-31 kg K Coulomb’s law constant (1/4pP0) 8.99*109 N m2/C2 P0 Permittivity constant 8.85*10-12 C2/N m2 m0 Permeability constant 1.26*10-6 T m/A e Fundamental unit of charge 1.60*10-19 C c Speed of light in vacuum 3.00*108 m/s h Planck’s constant 6.63*10-34 J s 4.14*10-15 eV s U Planck’s constant 1.05*10-34 J s 6.58*10-16 eV s aB Bohr radius 5.29*10-11 m Common Prefixes Conversion Factors Prefix Meaning Length Time femto- 10-15 1 in = 2.54 cm 1 day = 86,400 s pico- 10-12 1 mi = 1.609 km 1 year =3.16*107 s nano- 10-9 1 m = 39.37 in Pressure micro- 10-6 1 km = 0.621 mi 1 atm = 101.3 kPa = 760 mm of Hg milli- 10-3 Velocity 1 atm =14.7 lb/in2 centi- 10-2 1 mph = 0.447 m/s Rotation kilo- 103 1 m/s = 2.24 mph = 3.28 ft/s 1 rad =180°/p=57.3° mega- 106 Mass and energy 1 rev =360°=2p rad giga- 109 1 u = 1.661 *10-27 kg 1 rev/s =60 rpm terra- 1012 1 cal = 4.19 J 1 eV =1.60*10-19 J Mathematical Approximations Binominal approximation: (1+x)n ≈1+nx if xV 1 Small-angle approximation: sin u ≈tan u≈u and cos u≈1 if uV 1 radian Greek Letters Used in Physics Alpha a Mu m Beta b Pi p Gamma Γ g Rho r Delta ∆ d Sigma g s Epsilon P Tau t Eta h Phi Φ f Theta ϴ u Psi c Lambda l Omega Ω v A00_KNIG7429_04_GE_FEP.indd 1 15/07/16 9:44 pm Problem-Solving Strategies and Model Boxes PROBLEM-SOLVING STRATEGY PAGE MODEL PAGE 1.1 Motion diagrams 35 2.1 Uniform motion 57 1.2 General problem-solving strategy 43 2.2 Constant acceleration 68 2.1 Kinematics with constant 4.1 Projectile motion 110 acceleration 69 4.2 Uniform circular motion 119 4.1 Projectile motion problems 110 4.3 Constant angular acceleration 121 6.1 Newtonian mechanics 156 5.1 Ball-and-spring model of solids 136 7.1 Interacting-objects problems 189 6.1 Mechanical equilibrium 154 8.1 Circular-motion problems 217 6.2 Constant force 158 10.1 Energy-conservation problems 265 6.3 Friction 164 11.1 Conservation of momentum 292 8.1 Central force with constant r 208 12.1 Rotational dynamics problems 331 9.1 Basic energy model 231 17.1 Interference of two waves 498 11.1 Collisions 299 19.1 Work in ideal-gas processes 542 12.1 Rigid-body model 317 19.2 Calorimetry problems 552 12.2 Constant torque 332 21.1 Heat-engine problems 601 12.3 Static equilibrium 333 22.1 Electrostatic forces and 14.1 Molecular model of gases and liquids 380 Coulomb’s law 636 14.2 Ideal fluid 395 23.1 The electric field of multiple point 15.1 Simple harmonic motion 428 charges 653 16.1 The wave model 460 23.2 The electric field of a continuous 18.1 Solids, liquids, and gases 513 distribution of charge 659 19.1 Thermodynamic energy model 546 24.1 Gauss’s law 695 22.1 Charge model 626, 628 25.1 Conservation of energy in charge 22.2 Electric field 640 interactions 719 23.1 Four key electric fields 652 25.2 The electric potential of a continuous distribution of charge 727 26.1 Charge escalator model of a battery 745 28.1 Resistor circuits 802 29.1 Three key magnetic fields 824 29.1 The magnetic field of a current 825 33.1 Wave model of light 971 30.1 Electromagnetic induction 871 34.1 Ray model of light 983 36.1 Relativity 1066 38.1 Photon model of light 1115 40.1 Quantum-mechanics problems 1168 38.2 The Bohr model of the atom 1122 A00_KNIG7429_04_GE_FEP.indd 2 19/07/16 10:07 am ph y s ic s for scientists and engineers a strategic approach fourth edition with modern physics global edition . randall d knight California Polytechnic State University San Luis Obispo Boston Columbus Indianapolis New York San Francisco Hoboken Amsterdam Cape Town Dubai London Madrid Milan Munich Paris Montréal Toronto Delhi Mexico City São Paulo Sydney Hong Kong Seoul Singapore Taipei Tokyo A01_KNIG7429_04_GE_FM.indd 1 05/08/16 1:46 pm Editor-in-Chief: Jeanne Zalesky Acquisitions Editor: Darien Estes Acquisitions Editor, Global Editions: Abhijit Baroi Project Manager: Martha Steele Program Manager: Katie Conley Project Editor, Global Editions: K.K. Neelakantan Senior Manufacturing Controller, Global Editions: Kay Holman Media Production Manager, Global Editions: Vikram Kumar Senior Development Editor: Alice Houston, Ph.D. Art Development Editors: Alice Houston, Kim Brucker, and Margot Otway Development Manager: Cathy Murphy Program and Project Management Team Lead: Kristen Flathman Production Management: Rose Kernan Design Manager: Mark Ong Cover Designer: Lumina Datamatics Illustrators: Rolin Graphics Rights & Permissions Project Manager: Maya Gomez Rights & Permissions Management: Rachel Youdelman Photo Researcher: Eric Schrader Manufacturing Buyer: Maura Zaldivar-Garcia Executive Marketing Manager: Christy Lesko Cover Photo Credit: Everett Historical/Shutterstock.com Acknowledgements of third party content appear on page C-1 to C-2, which constitutes an extension of this copyright page. PEARSON, ALWAYS LEARNING and MasteringPhysics® are exclusive trademarks in the U.S. and/or other countries owned by Pearson Education, Inc. or its affiliates. Pearson Education Limited Edinburgh Gate Harlow Essex CM20 2JE England and Associated Companies throughout the world Visit us on the World Wide Web at: www.pearsonglobaleditions.com © Pearson Education Limited 2017 The right of Randall D. Knight to be identified as the author of this work has been asserted by him in accordance with the Copyright, Designs and Patents Act 1988. Authorized adaptation from the United States edition, entitled Physics for Scientists and Engineers: A Strategic Approach with Modern Physics,4/e, ISBN 978-0-13-394265-1, by Randall D. Knight published by Pearson Education © 2017. All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted in any form or by any means, electronic, mechanical, photocopying, recording or otherwise, without either the prior written permission of the publisher or a license permitting restricted copying in the United Kingdom issued by the Copyright Licensing Agency Ltd, Saffron House, 6–10 Kirby Street, London EC1N 8TS. All trademarks used herein are the property of their respective owners. The use of any trademark in this text does not vest in the author or publisher any trademark ownership rights in such trademarks, nor does the use of such trademarks imply any affiliation with or endorsement of this book by such owners. British Library Cataloguing-in-Publication Data A catalogue record for this book is available from the British Library 10 9 8 7 6 5 4 3 2 1 ISBN 10: 1-292-15742-9 ISBN 13: 978-1-292-15742-9 Typeset by Cenveo® Publisher Services Printed and bound in Malaysia A01_KNIG7429_04_GE_FM.indd 2 05/08/16 1:50 pm About the Author Randy Knight taught introductory physics for 32 years at Ohio State University and California Polytechnic State University, where he is Professor Emeritus of Physics. Professor Knight received a Ph.D. in physics from the University of California, Berkeley and was a post-doctoral fellow at the Harvard-Smithsonian Center for Astrophysics before joining the faculty at Ohio State University. It was at Ohio State that he began to learn about the research in physics education that, many years later, led to Five Easy Lessons: Strategies for Successful Physics Teaching and this book, as well as College Physics: A Strategic Approach, co- authored with Brian Jones and Stuart Field. Professor Knight’s research interests are in the fields of laser spectroscopy and environmental science. When he’s not in front of a computer, you can find Randy hiking, sea kayaking, playing the piano, or spending time with his wife Sally and their five cats. A01_KNIG7429_04_GE_FM.indd 3 18/07/16 2:52 pm 9.1 Energy Overview 207 Energy Overview 9.1 Energy. It’s a word you hear all the time, and everyone has some sense of what energy means. Moving objects have energy; energy is the ability to make things happen; energy is associated with heat and with electricity; we’re constantly told to conserve energy; living organisms need energy; and engineers harness energy to do useful things. Some scientists consider the law of conservation of energy to be the most important of all the laws of nature. But all that in due time—first we have to start with the basic ideas. Just what is energy? The concept of energy has grown and changed with time, and it is not easy to define in a general way just what energy is. Rather than starting with a formal definition, we’re going to let the concept of energy expand slowly over the course of several chapters. Our goal is to understand the characteristics of energy, how energy is used, and how energy is transformed from one form into another. It’s a complex story, so we’ll take it step by step until all the pieces are in place. Some important forms of energy Kinetic energy K Potential energy U Thermal energy E th 46 CHAPTER 2 Kinematics in One Dimension A research-driven approach, Built from the ground up on physics education research and crafted using key ideas from lear1n42 iCnHAgPT ERt 6h Dyenamoics rI: Myo,ti onK Alonng ai gLinhe t has set the fine-tuned for even greater Exercises and Problems 259 standard for eff ective and accessible pedagogical materials in Kinetic energy is the energy of motion. Potential energy is stored energy associated Thermal energy is the sum of the micro- All moving objects have kinetic energy. with an object’s position. The roller coaster’s scopic kinetic and po5t5e.n t||i|a l Pernoetrogniess and neutrons (together called nucleons) are held 61. || The potential energy for a particle that can move along the The more massive an object or the faster gravitational potential energy depends on of all ethe ataomss ande bontdo-sg ethtohaet rm inafk teh- eu pn uucleuss ofe an a toma byn a fordce ca llesd thte sturong dexn-axis tis U =sAx2u+B scin pcx/Le, whsere As, B, and L are constants. physics. In this fourth edition, Knight continues to refi ne and it moves, the larger its kinetic energy. its height above the ground. the object. An object has more thermal force. At very small separations, the strong force between two What is the force on the particle at (a) x=0, (b) x=L/2, and (c) energy when hot than wnhuecnl ecoonlds .is larger than the repulsive electrical force between two x=L? 1 2 expand the instructional techniques to take students further. protons—hence its name. But the strong force quickly weakens 62. || A particle that can move along the x-axis experiences an as the distance between the protons increases. A well-established interaction force Fx= 3x2-5x N, where x is in m. Find an model for the potential energy of two nucleons interacting via the expression for the system’s potential energy. The Energy Principle strong force is 63. || An object moving i1n the xy-p2lane is subjected to the force Fu= 2xy ni +x2 nj N, where x and y are in m. ❮❮ Section 7.1 introduced interaction diagrams and the very important distinction REVISED COVERUA=UG0 E1- Ae-xN/x0 D ORGANIZATIONa. TGhe IpaVrtiEcle mINoveSs frTomR thUe oCrigiTn tOo thRe pSoi nt with coordinates NEW AND UPDATED LEARNING TOOLS PROMOTE DEEPER AND between the system, those objects whose motion and interactions we wish to a1, b by mov2ing first along the x-axis to a, 0 , then parallel analyze, and the environment, objects external to the system but exerting forces where x is the dGistaRncEe bAetT3weEenR th eC 4ceHnteOrs oIf CtheE t wAo nNuclDe- FLEXIBILITY BETTER-CONNECTED UNDERSTANDING osyns ttehme .s yWsthemy?. BTehcea musoes te nimerpgoyr tiasn nt ostt espo mine a dni seenmerbgoyd aienda,l yesthise rise atol sculebastralyn cdee;f iint’es tthhee oUn0s ,= x60 . 0is* a 1c0o-n11s tJa.nt having the value x0 =2.0*10-15 m, and b. tT1oah ,te hb pe2 a ybr-tyaic xmlieso .m vHionovgwe sf mifrrsuotcm ah l towhneog ro ktrh idgeoi nye -stao tx htihese ft oporo c1ien0 t,d wbo2?it, ht hceono rpdainraaltleesl Quantum effects are essential for a proper understand- wptwteaehrnnsoaihe vtetanFhisericInsegrnoGhf o tyuUoi oinnw tRraon mimElletef o i’ 9ee easls.nnbld1ols et yd. msi, ril te Cnglateosuhttyhtinsoehge etem Uinrmt tnaaoh,eagt itteensct.ea hsr ta Sl m Ewe ltope hrsfeeaemyne nsltce . ghiae irdeTfoelrgne ig hycelaeayaean rplo rwgleocelifyrycna goa.t,tng ohyrfiA. etre bc’i E Wssamoes lt ynthlltaiho,yssrt neh.tanec ey Tnrighemn vs khen afam eieotistn hrsirs idgo emyctushyn as nes te oloeoyd c remfsfhs fniytaaeon eesh nnrtmstraogmeegys ,remsy k sgdte,e ie yon.nnai m.fesYeen re.trdongignc uoyyes ’,toer l tglnc ih onyaereent:nr e sgc.k ryoybWiasn,gec tenwe teit’tinihlrzmclagie cein nhtewnsht enfriiiorstoseghr dtrmi yhdugt eheceKydneae,, FpIeGrUspReEHc 9eta.i1Tvt ehKA eoi n snseyy tEEseistcnnentvemeSerimyrrg hsgoy-tayn5 eesa.m6m nde.Pdvne oeino camii|tv1e|rfwnd trestaf.oe g6og nrnotnyA7tv ihktt h aomieiEeia b*enfnnr2ylse yslygeeWn. esn,16 .utw u tic0of ttc cohkerrr- lkaor2regecf7esnn o reh bks in s crl gFmosett 5ox,ilca oae.gkb=0nnalNmsciUtwe ulcod csoit,*tsnaiE eho hb vt2a dhl lcerheWea1eet0 baierhtwhtd 0atr?wrstq a-eem-adu!eu tauem1ndcrK ,aslv5e5C eaaheg s.eeetnimxbteSsPtce nseeihhnulleTsiW Hlitde,eeeedrtdO nnp,y , tci fd cNf asg hP to e1aitoa heeuAt igan o pinec,pcr.1stnTarusn 0oot lid rewO aeyrPthiicd an Kee nb vn ar td*m a.hi dhTTms stlth esWgeol nepH,oeletix li o1, yih pErfIyocptnieh nrmNer0e ghamfclikat dm ociRtgKe e-mitennzh xd h?u oc ei1rm oosee1 tde tat5nseai ls smh1’ Outnstnnw psmshsna.ia aatet6deuiti ipeitratntt du ndpnu. Remh ra etl ltteu e dnp ebomAtSrldmoemrGrh pdui omreinu o asareq ., eott t=apep ppe wcuow lhATufsnob1r bphepho 2f t saoesjhsseu e oe lernNnihiis tomc teca rnenspoahekanw t eoicew i sngcgguafepelpItusrh e eroncmtlZtetu 2 ypaa eee rsmneovioet/esiononrnttrsf-rfs.Atfxdyoi ue nof ia oeeisuel asTnmt0ctlernhc tidhcesi.torsoaaoIs2esp he coO.ayn rstl n5n i up t02a(ndoeassrWk1to.src gr ,iNf ceem co bop w/isgr ta)mtakyorilolo a rp6laanknuo4lnnespcwpi.dyd n.m ie02(|bcaFbsakn | gu degm... eg imn =fnnA wtITttT11a/reqsohhtssaao)g hh1nr iu eedtcel,,ttgtm2nee r ahhahbbxyo uxyebppei-l-22 ybscat ia cmaas x a 2tnijbbixtxrrao,esa-or ttyyeipi +amcnciitfescsxr .ccc ixtmm..(oco sv ll k 3uph.niHeeHg nurm 2seooy t aoem=.smmoovrvo njon tewH/1sw0uwii2s eoov1r)nne- o.v vv iNg6g mmnweea ,ffAgsstuu iii dwm rrffvccvissrrhhehnauoott ne cammawfwctorhllehooeoo r dttew cnrnrhh xkTk eggeeo ox ?a ddprtootynkhhioorrc-d ee:iiepe dggR sslyxyoiioa --nn ttecnaaahhk sttexrxeee ooe tt i i fhfss ittPoios hherntt rrooo eec csfpm oeuepp1ur alb0oo.ddsc1ijii,,oooe enn0b?n? cttd2 tww o,,e 2?ttd2iihhtt8 hhee1t nnocc oo pptooaahrrrreddaa iillfnnlloeeaallrtt ceettooess NerrodteeemvaxEaaemtpslWr -oh aewannna!noast ddMarib sl tlldo heOos ve siniemnidD tr meu pdiaEalenolitpL idfiszoile ocoanBlalyti vitnOieoinigdonn X— ntgsmes rEtp aohmarSnraroesa etbe l eocnlydexafzehm pnvisanl iensibmglc.coe iTpea tpal l heytecphed opibes mnlie uint eteptf hdxtulhee tnx’ es-, MFCooOrMLMiauvu nnmiD amoasotd tvvshEisteftaffiet ssa2lLor= nm ta=nt=i h itoa s2g w e vntivah i. is+sicoit2sc t:2 ab+h l cMvl+ij l nieecays eoco2∆ls: tdena∆w taess rti+stl∆ata hf ansta12 itcipa oloaassn1cn rit∆csfie tcttal2lheneMFT■2er t  am hrpa OSC teiicaoct oacrfavDntntretiiii. nliccEcheolgt raeiLfnavo’rsti enic6o tafni.ono3.ryn c :em A iavscs0ig sitpnsavsas siTatrhusae SHdn latlePorecea raceuliTirze gdaphtolhboeeen tort d tasloltaial thnlo it ooeelpfinse n s pm eiiussra xercafvos=a.necsntmeat.n sm tn.ttt.otion. Friction Ppuulslh or theB eunte rsgyyst eomf tsh oe fsteynst edmo ,i neittehrearc ti nwcirteha stihnegir i te n(evnierorgnym aedndt.e Td)h oosr ed einctreeraascitnigon ist (cehnaenrggye ETnheregrmy caaln be trCanh Isenfmoitriimcaalelldy the block is1 at rest at2 x=0 m. What is the block’s spee-2d 65.- 2Wc. riI1tse tah ir2se aal icsotincs perrovbatleivme ffoorr cwe?hich the energ1y ba2r chart shown in wniozrek wedh eenx aamndp lheos,w h etolp uinseg rsetucuderrnitnsg t om roedceolgs-, a acceleration changes. ■■    KRoinlleitnigc ffrriiccttiioonn:: OOppppoosseess mmooTtthiieoo nnsl owwpEeiix tteihhsrc vissffe.kr 1==6mmrk n n.. Mto othtieo nsu irsf areclea.tive when it has been pulled to x=4.0 m? ■  Graphically: removed). We say that interactions with the environment transfer energy into or Heat 57. || A syWstoermk has potential energy FIGURE P10.65 correctly shows the energy at the beginning and end key critical-thinking skill. out of the system. Interestingly, there are only two ways to transfer energy. One is Energy removed of the problem. by mechanical means, using forces to push and pull on the system. A process that Environment U x =x+1Nsie1nw.t6on2 ’s ar saeddco/vmnad lnxawc Fue=dm aut aopppliiecs t oR obojeccts kwehotse Ip mnPr oaPrsbsrol odeobmpelse.u mnFolosst r ci6 hoe6aan ncgtheh .r Toohfu agtth’hse 6se8, yyoouu aarree gtoiven the equation used to solve a fs max = mmksnnf Static KiTfnrheicteti icoobnj erceta cshliepss fws mhaexn. static as a particle move1s 2over thea rna enx1cg1eell e0n tm ass…um2xpt2…ionp fo rm ba.lls and bicycles, but what abao.u t Wsomriettehi nag r leikael ias rtoicck eptr oblem for which this is the correct equation. Sintcarteica sferisc ttoio mnatch Kasi ntheeti co bfrjeicctti omno ivse cso.nstant a. Where are the equilibriutmhmaast spl oaosrseeis st oiaol vsneigdsn wiifniitc hta hmntio sam mreaonnutungmte o? rfa tmhears sth aasn iatcs cfeuleerl aitsio bnu. brWn.e ed’lD?l lProaroowkb al ett mhones e ob ifme vfpaoorrryteian-ngat nd-after pictorial representation. the push or pull. 0 Rest Moving Push or pull force b. For each, is it a point of esxtaambplele .or unstable equilibrium? c. Finish the solution of the problem. 6 Dynamics I: Motion NEW! ADV58A. N|w| iCtAh E ppDoatre tnictilea l tehnaet rcgayn moveiwn eafalFluIkoGe inUnncRg ceE o dt1m 1hb.py2ea 9 g rxrsiash-ovaoniwxt ytsio so at rh irdesor rcaopkgcae.k tPr eebtt ’reshoi tnafhpg rs aup i srtst oi.y spT seahlt rlieeosm dcmk ba eyyt intnho det ebteehp rh usigsptha colyef rwbeuahrleinrsietni cgg,r bafvuueitt liy gb inuso tvr eninrogyt FraeImGpoUreuRsnEet 1 no1t.fa 2tf9uio enAl. obfe afo rroec-kaentd b-aufrtneirn pg icat somriaalll Along a LineM03_KNIG2651_04_SE_C02.indd 46 9/13/15 8:41 PM TadOd PevICenS m aso roep ftiloexniabli slietcyt ions U x gm=raatvhAietym a-altliocBws sto uos ctoo munpdliecrastteadn.d R tohcek eests penrotipaulsls oiof nro wckiteht gprraovpiutyls iios na wCihthaloluent gmea Pkrionbgl tehme E (J)Before: m vx 1Tasa5p chm2ceee ei llpdeeCo .roHawftA eeorPsvf TeuthErl iRt1sh 5e6r0n u oDsmtry mponhfoa tmuinhs ei lcp esjles aIstn: eteMh ntaogonit n ai oe sn Along a Line M11_KNIG2651_04_SE_C09.indd 207 9/28/15 5:35i Pn Mthxe2 end-oxf-chapter problems. 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A sprong-loaded toy guTnh e smhaosos otsf thai s 2lit0tl eg p acpkl1eats o2tfi cbu rbnaedll f.u eW1l ish2 tahet mass lCosath bnyad th lielm reocpnk1regot: vmeefu dePl =ur-so2idn1mbg. l eMmastse2ringPhysics® data, strength of gravity. An object in free fall is weightless. B FuG Summary, consolidating and is the launch speed if tMhaet hsempraotincagll yc, tohne smtainnuts siisg n 4te0ll,s0 u0s 0th,a tw thiet hm ass of thee xbupranendd fu etlh (eth er gaansegs)e a nodf physics and math skills TERMS AND NOTATION the units you found in pthaer tr oack, eat nmdas st haree cshparnogningg iins ocpopomsipter deisrescetdio ns. Phys6isc9ta.ul ly|d|,| ewneA tk snp oewwn itdhlula tl uudmsme6 its0o ,f osromlveed pfrroomb lae msmsa.ll ball of mass m on a string M07_KNIG2651_04_SE_C06.indd 131 equilibrium model weigh9t/13/15 8:09 PM rolling friction drag coefficient, C structuring understanding. 10 cm? Assume the barrseol tihse ferxihcatuisot nglaesesss .have a positive mass. of length L. As FIGURE CP10.69 shows, a peg is height h=L/3 cfloant-setaanrtth-f oarpcper omxoimdealtion ccooeeffffiicciieenntt ooff kstianteitci cf rfircitcitoionn, ,m msk c oefrfifcictiioenn,t mofr rolling terminal speed, vterm M07_KNIG2651_04_SE_C06.indd 152 9/13/15 8:12 PM M13_KNIG2651_04_SE_C11.indd 281 9/28/15 5:23 PM A01_KNIG7429_04_GE_FM.indd 4 18/07/16 2:52 pm M12_KNIG2651_04_SE_C10.indd 259 9/28/15 5:29 PM 9.1 Energy Overview 207 Energy Overview 9.1 Energy. It’s a word you hear all the time, and everyone has some sense of what energy means. Moving objects have energy; energy is the ability to make things happen; energy is associated with heat and with electricity; we’re constantly told to conserve energy; living organisms need energy; and engineers harness energy to do useful things. Some scientists consider the law of conservation of energy to be the most important of all the laws of nature. But all that in due time—first we have to start with the basic ideas. Just what is energy? The concept of energy has grown and changed with time, and it is not easy to define in a general way just what energy is. Rather than starting with a formal definition, we’re going to let the concept of energy expand slowly over the course of several chapters. Our goal is to understand the characteristics of energy, how energy is used, and how energy is transformed from one form into another. It’s a complex story, so we’ll take it step by step until all the pieces are in place. Some important forms of energy Kinetic energy K Potential energy U Thermal energy E th 46 CHAPTER 2 Kinematics in One Dimension A research-driven approach, Built from the ground up on physics education research and crafted using key ideas from lear1n42 iCnHAgPT ERt 6h Dyenamoics rI: Myo,ti onK Alonng ai gLinhe t has set the fine-tuned for even greater Exercises and Problems 259 standard for eff ective and accessible pedagogical materials in Kinetic energy is the energy of motion. Potential energy is stored energy associated Thermal energy is the sum of the micro- All moving objects have kinetic energy. with an object’s position. The roller coaster’s scopic kinetic and po5t5e.n t||i|a l Pernoetrogniess and neutrons (together called nucleons) are held 61. || The potential energy for a particle that can move along the The more massive an object or the faster gravitational potential energy depends on of all ethe ataomss ande bontdo-sg ethtohaet rm inafk teh- eu pn uucleuss ofe an a toma byn a fordce ca llesd thte sturong dexn-axis tis U =sAx2u+B scin pcx/Le, whsere As, B, and L are constants. physics. In this fourth edition, Knight continues to refi ne and it moves, the larger its kinetic energy. its height above the ground. the object. An object has more thermal force. At very small separations, the strong force between two What is the force on the particle at (a) x=0, (b) x=L/2, and (c) energy when hot than wnhuecnl ecoonlds .is larger than the repulsive electrical force between two x=L? 1 2 expand the instructional techniques to take students further. protons—hence its name. But the strong force quickly weakens 62. || A particle that can move along the x-axis experiences an as the distance between the protons increases. A well-established interaction force Fx= 3x2-5x N, where x is in m. Find an model for the potential energy of two nucleons interacting via the expression for the system’s potential energy. The Energy Principle strong force is 63. || An object moving i1n the xy-p2lane is subjected to the force Fu= 2xy ni +x2 nj N, where x and y are in m. ❮❮ Section 7.1 introduced interaction diagrams and the very important distinction REVISED COVERUA=UG0 E1- Ae-xN/x0 D ORGANIZATIONa. TGhe IpaVrtiEcle mINoveSs frTomR thUe oCrigiTn tOo thRe pSoi nt with coordinates NEW AND UPDATED LEARNING TOOLS PROMOTE DEEPER AND between the system, those objects whose motion and interactions we wish to a1, b by mov2ing first along the x-axis to a, 0 , then parallel analyze, and the environment, objects external to the system but exerting forces where x is the dGistaRncEe bAetT3weEenR th eC 4ceHnteOrs oIf CtheE t wAo nNuclDe- FLEXIBILITY BETTER-CONNECTED UNDERSTANDING osyns ttehme .s yWsthemy?. 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Friction Ppuulslh or theB eunte rsgyyst eomf tsh oe fsteynst edmo ,i neittehrearc ti nwcirteha stihnegir i te n(evnierorgnym aedndt.e Td)h oosr ed einctreeraascitnigon ist (cehnaenrggye ETnheregrmy caaln be trCanh Isenfmoitriimcaalelldy the block is1 at rest at2 x=0 m. What is the block’s spee-2d 65.- 2Wc. riI1tse tah ir2se aal icsotincs perrovbatleivme ffoorr cwe?hich the energ1y ba2r chart shown in wniozrek wedh eenx aamndp lheos,w h etolp uinseg rsetucuderrnitnsg t om roedceolgs-, a acceleration changes. ■■    KRoinlleitnigc ffrriiccttiioonn:: OOppppoosseess mmooTtthiieoo nnsl owwpEeiix tteihhsrc vissffe.kr 1==6mmrk n n.. Mto othtieo nsu irsf areclea.tive when it has been pulled to x=4.0 m? ■  Graphically: removed). We say that interactions with the environment transfer energy into or Heat 57. || A syWstoermk has potential energy FIGURE P10.65 correctly shows the energy at the beginning and end key critical-thinking skill. out of the system. Interestingly, there are only two ways to transfer energy. One is Energy removed of the problem. by mechanical means, using forces to push and pull on the system. A process that Environment U x =x+1Nsie1nw.t6on2 ’s ar saeddco/vmnad lnxawc Fue=dm aut aopppliiecs t oR obojeccts kwehotse Ip mnPr oaPrsbsrol odeobmpelse.u mnFolosst r ci6 hoe6aan ncgtheh .r Toohfu agtth’hse 6se8, yyoouu aarree gtoiven the equation used to solve a fs max = mmksnnf Static KiTfnrheicteti icoobnj erceta cshliepss fws mhaexn. static as a particle move1s 2over thea rna enx1cg1eell e0n tm ass…um2xpt2…ionp fo rm ba.lls and bicycles, but what abao.u t Wsomriettehi nag r leikael ias rtoicck eptr oblem for which this is the correct equation. Sintcarteica sferisc ttoio mnatch Kasi ntheeti co bfrjeicctti omno ivse cso.nstant a. Where are the equilibriutmhmaast spl oaosrseeis st oiaol vsneigdsn wiifniitc hta hmntio sam mreaonnutungmte o? rfa tmhears sth aasn iatcs cfeuleerl aitsio bnu. brWn.e ed’lD?l lProaroowkb al ett mhones e ob ifme vfpaoorrryteian-ngat nd-after pictorial representation. the push or pull. 0 Rest Moving Push or pull force b. For each, is it a point of esxtaambplele .or unstable equilibrium? c. Finish the solution of the problem. 6 Dynamics I: Motion NEW! ADV58A. N|w| iCtAh E ppDoatre tnictilea l tehnaet rcgayn moveiwn eafalFluIkoGe inUnncRg ceE o dt1m 1hb.py2ea 9 g rxrsiash-ovaoniwxt ytsio so at rh irdesor rcaopkgcae.k tPr eebtt ’reshoi tnafhpg rs aup i srtst oi.y spT seahlt rlieeosm dcmk ba eyyt intnho det ebteehp rh usigsptha colyef rwbeuahrleinrsietni cgg,r bafvuueitt liy gb inuso tvr eninrogyt FraeImGpoUreuRsnEet 1 no1t.fa 2tf9uio enAl. obfe afo rroec-kaentd b-aufrtneirn pg icat somriaalll Along a LineM03_KNIG2651_04_SE_C02.indd 46 9/13/15 8:41 PM TadOd PevICenS m aso roep ftiloexniabli slietcyt ions U x gm=raatvhAietym a-altliocBws sto uos ctoo munpdliecrastteadn.d R tohcek eests penrotipaulsls oiof nro wckiteht gprraovpiutyls iios na wCihthaloluent gmea Pkrionbgl tehme E (J)Before: m vx 1Tasa5p chm2ceee ei llpdeeCo .roHawftA eeorPsvf TeuthErl iRt1sh 5e6r0n u oDsmtry mponhfoa tmuinhs ei lcp esjles aIstn: eteMh ntaogonit n ai oe sn Along a Line M11_KNIG2651_04_SE_C09.indd 207 9/28/15 5:35i Pn Mthxe2 end-oxf-chapter problems. 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A sprong-loaded toy guTnh e smhaosos otsf thai s 2lit0tl eg p acpkl1eats o2tfi cbu rbnaedll f.u eW1l ish2 tahet mass lCosath bnyad th lielm reocpnk1regot: vmeefu dePl =ur-so2idn1mbg. l eMmastse2ringPhysics® data, strength of gravity. An object in free fall is weightless. B FuG Summary, consolidating and is the launch speed if tMhaet hsempraotincagll yc, tohne smtainnuts siisg n 4te0ll,s0 u0s 0th,a tw thiet hm ass of thee xbupranendd fu etlh (eth er gaansegs)e a nodf physics and math skills TERMS AND NOTATION the units you found in pthaer tr oack, eat nmdas st haree cshparnogningg iins ocpopomsipter deisrescetdio ns. Phys6isc9ta.ul ly|d|,| ewneA tk snp oewwn itdhlula tl uudmsme6 its0o ,f osromlveed pfrroomb lae msmsa.ll ball of mass m on a string M07_KNIG2651_04_SE_C06.indd 131 equilibrium model weigh9t/13/15 8:09 PM rolling friction drag coefficient, C structuring understanding. 10 cm? Assume the barrseol tihse ferxihcatuisot nglaesesss .have a positive mass. of length L. As FIGURE CP10.69 shows, a peg is height h=L/3 cfloant-setaanrtth-f oarpcper omxoimdealtion ccooeeffffiicciieenntt ooff kstianteitci cf rfircitcitoionn, ,m msk c oefrfifcictiioenn,t mofr rolling terminal speed, vterm M07_KNIG2651_04_SE_C06.indd 152 9/13/15 8:12 PM M13_KNIG2651_04_SE_C11.indd 281 9/28/15 5:23 PM A01_KNIG7429_04_GE_FM.indd 5 18/07/16 2:52 pm M12_KNIG2651_04_SE_C10.indd 259 9/28/15 5:29 PM 10.4 Conservation of Energy 243 A STRUCTURED AND CONSISTENT APPROACH BUILDS MasteringPhysics THE ULTIMATE RESOURCE PROBLEM-SOLVING SKILLS AND CONFIDENCE BEFORE, DURING, AND AFTER CLASS With a research-based 4-step problem-solving BEFORE CLASS PROBLEM-SOLVING STRATEGY 10.1 framework used throughout the text, students learn the importance of making assumptions Energy-conservation problems (in the MODEL step) and gathering informa- NEW! INTERACTIVE PRELECTURE VIDEOS NEW! DYNAMIC STUDY MODULES (DSMs) con- tion and making sketches (in the VISUALIZE MODEL Define the system so that there are no external forces or so that any address the rapidly growing movement toward pre-lecture tinuously assess students’ performance in real time to provide external forces do no work on the system. If there’s friction, bring both surfaces step) before treating the problem mathemati- into the system. Model objects as particles and springs as ideal. teaching and flipped classrooms. These whiteboard-style personalized question and explanation content until students cally (SOLVE) and then analyzing their results VISUALIZE Draw a before-and-after pictorial representation and an energy bar animations provide an introduction to key topics with master the module with confidence. The DSMs cover basic (ASSESS). chart. A free-body diagram may be needed to visualize forces. embedded assessment to help students prepare and profes- math skills and key definitions and relationships for topics sors identify student misconceptions before lecture. across all of mechanics and electricity and magnetism. SOLVE If the system is both isolated and nondissipative, then the mechanical energy is conserved: Detailed PROBLEM-SOLVING Ki+Ui=Kf+Uf STRATEGIES for different topics and where K is the total kinetic energy of all moving objects and U is the total categories of problems (circular-motion potential energy of all interactions within the system. If there’s friction, then problems, calorimetry problems, etc.) Ki+Ui=Kf+Uf+ ∆Eth are developed throughout, each one built on the 4-step framework and carefully where the thermal energy increase due to friction is ∆Eth=fk ∆s. illustrated in worked examples. ASSESS Check that your result has correct units and significant figures, is reasonable, and answers the question. Exercise 14 716 CHAPTER 26 Potential and Field TACTICS BOX 26.1 DURING CLASS Finding the potential from the electric field ●1 Draw a picture and identify the point at which you wish to find the potential. Call this position f. ●2 Choose the zero point of the potential, often at infinity. Call this position i. NEW! LEARNING CATALYTICS™ is an interactive ●3 Establish a coordinate axis from i to f along which you already know or can 30-8 chapter 30 • Electromagnetic Induction classroom tool that uses students’ devices to engage them in ●4 eCaasrirlyy doeutte trhmei innet ethgera etiloecnt roifc Efiqeulda tcioonm 2p6o.n3e tnot fEins.d the potential. 1P30S8.S1. Tao fhr etehc getar cnaupgrhur lesanhrt o liwono stp hh eoo fwl ow otihpree a mws aait ghfnu renetcsictiis oftianen locdfe c tRihma. nDeg.r eLaswe tt h aar og uragphh menoarbel esso pinhsitsrtuiccatoterds ttoa sgkesn aenradt eth cilnaksisnrogo. mLe dairsnciunsgs iCoant aalnydt ics counterclockwise current be positive, a clockwise Exercise 1 current be negative. promote peer-to-peer learning to help students develop TACTICS BOXES give step-by-step procedures for critical-thinking skills. Instructors can take advantage of developing specific skills (drawing free-body diagrams, a. What is the magnetic flux through the loop at t=0? real-time analytics to find out where students are struggling b. Does this flux change between t=0 and t=t1? and adjust their instructional strategy. using ray tracing, etc.). c. Is there an induced current in the loop between t=0 and t=t1? d. What is the magnetic flux through the loop at t=t2? e. What is the change in flux through the loop between t1 and t2? f. What is the time interval between t1 and t2? g. What is the magnitude of the induced emf between t1 and t2? h. What is the magnitude of the induced current between t1 and t2? AFTER CLASS i. Does the magnetic field point out of or into the loop? j. Between t1 and t2, is the magnetic flux increasing or decreasing? k. To oppose the change in the flux between t1 and t2, should the magnetic field of the induced current point out of or into the loop? The REVISED STUDENT WORKBOOK l. Is the induced current between t1 and t2 positive or negative? NEW! ENHANCED ADAPTIVE FOLLOW-UPS is tightly integrated with the main text–allowing m. Does the flux through the loop change after t2? END-OF-CHAPTER are personalized assignments students to practice skM1il2l_sK NfIGro26m51_ t0h4_eS Et_eCx10t.’insd dT a24c3tics no.. IUs steh earlel tahnis i nindfuocremda ctiuornre tnot dinra twhe a l goroapp ahf otefr tth2e? induced current. Add appropriate labels on the QUES1T0/6I/1O5 N9:28S A Moffer stu- that pair Mastering’s powerful Boxes, work through the steps of Problem-Solv- vertical axis. dents instructional support content with Knewton’s adaptive ing Strategies, and assess the applicability of the when and where they need learning engine to provide Models. The workbook is referenced throughout it, including links to the individualized help to students the text with the icon . © 2017 Pearson Education. eafoTnred xh wto, mrmoenawgth-oa rrnkes mawseesdrig ifanetmeiodenbn,a tcsk. bTtaosehpsfeioigcsresne e samdtdu iahdspocetmonivntesecw esftpoorltrulikoog,wn gisln-e uctdaplu kswd eaii tndhhgdo olrcdeno.s rse prerequisite topics. M30_KNIG3162_04_SE_C30.indd 8 09/25/15 4:07 PM A01_KNIG7429_04_GE_FM.indd 6 18/07/16 2:52 pm M32_KNIG2651_04_SE_C26.indd 716 10/6/15 9:29 AM 10.4 Conservation of Energy 243 A STRUCTURED AND CONSISTENT APPROACH BUILDS MasteringPhysics THE ULTIMATE RESOURCE PROBLEM-SOLVING SKILLS AND CONFIDENCE BEFORE, DURING, AND AFTER CLASS With a research-based 4-step problem-solving BEFORE CLASS PROBLEM-SOLVING STRATEGY 10.1 framework used throughout the text, students learn the importance of making assumptions Energy-conservation problems (in the MODEL step) and gathering informa- NEW! INTERACTIVE PRELECTURE VIDEOS NEW! DYNAMIC STUDY MODULES (DSMs) con- tion and making sketches (in the VISUALIZE MODEL Define the system so that there are no external forces or so that any address the rapidly growing movement toward pre-lecture tinuously assess students’ performance in real time to provide external forces do no work on the system. If there’s friction, bring both surfaces step) before treating the problem mathemati- into the system. Model objects as particles and springs as ideal. teaching and flipped classrooms. These whiteboard-style personalized question and explanation content until students cally (SOLVE) and then analyzing their results VISUALIZE Draw a before-and-after pictorial representation and an energy bar animations provide an introduction to key topics with master the module with confidence. The DSMs cover basic (ASSESS). chart. A free-body diagram may be needed to visualize forces. embedded assessment to help students prepare and profes- math skills and key definitions and relationships for topics sors identify student misconceptions before lecture. across all of mechanics and electricity and magnetism. SOLVE If the system is both isolated and nondissipative, then the mechanical energy is conserved: Detailed PROBLEM-SOLVING Ki+Ui=Kf+Uf STRATEGIES for different topics and where K is the total kinetic energy of all moving objects and U is the total categories of problems (circular-motion potential energy of all interactions within the system. If there’s friction, then problems, calorimetry problems, etc.) Ki+Ui=Kf+Uf+ ∆Eth are developed throughout, each one built on the 4-step framework and carefully where the thermal energy increase due to friction is ∆Eth=fk ∆s. illustrated in worked examples. ASSESS Check that your result has correct units and significant figures, is reasonable, and answers the question. Exercise 14 716 CHAPTER 26 Potential and Field TACTICS BOX 26.1 DURING CLASS Finding the potential from the electric field ●1 Draw a picture and identify the point at which you wish to find the potential. Call this position f. ●2 Choose the zero point of the potential, often at infinity. Call this position i. NEW! LEARNING CATALYTICS™ is an interactive ●3 Establish a coordinate axis from i to f along which you already know or can 30-8 chapter 30 • Electromagnetic Induction classroom tool that uses students’ devices to engage them in ●4 eCaasrirlyy doeutte trhmei innet ethgera etiloecnt roifc Efiqeulda tcioonm 2p6o.n3e tnot fEins.d the potential. 1P30S8.S1. Tao fhr etehc getar cnaupgrhur lesanhrt o liwono stp hh eoo fwl ow otihpree a mws aait ghfnu renetcsictiis oftianen locdfe c tRihma. nDeg.r eLaswe tt h aar og uragphh menoarbel esso pinhsitsrtuiccatoterds ttoa sgkesn aenradt eth cilnaksisnrogo. mLe dairsnciunsgs iCoant aalnydt ics counterclockwise current be positive, a clockwise Exercise 1 current be negative. promote peer-to-peer learning to help students develop TACTICS BOXES give step-by-step procedures for critical-thinking skills. Instructors can take advantage of developing specific skills (drawing free-body diagrams, a. What is the magnetic flux through the loop at t=0? real-time analytics to find out where students are struggling b. Does this flux change between t=0 and t=t1? and adjust their instructional strategy. using ray tracing, etc.). c. Is there an induced current in the loop between t=0 and t=t1? d. What is the magnetic flux through the loop at t=t2? e. What is the change in flux through the loop between t1 and t2? f. What is the time interval between t1 and t2? g. What is the magnitude of the induced emf between t1 and t2? h. What is the magnitude of the induced current between t1 and t2? AFTER CLASS i. Does the magnetic field point out of or into the loop? j. Between t1 and t2, is the magnetic flux increasing or decreasing? k. To oppose the change in the flux between t1 and t2, should the magnetic field of the induced current point out of or into the loop? The REVISED STUDENT WORKBOOK l. Is the induced current between t1 and t2 positive or negative? NEW! ENHANCED ADAPTIVE FOLLOW-UPS is tightly integrated with the main text–allowing m. Does the flux through the loop change after t2? END-OF-CHAPTER are personalized assignments students to practice skM1il2l_sK NfIGro26m51_ t0h4_eS Et_eCx10t.’insd dT a24c3tics on.. UIss teh earlle tahnis i nindfuocremda ctiuornre tnot dinra twhe a l goroapp ahf otefr tth2e? induced current. Add appropriate labels on the QUES1T0/6I/1O5 N9:28S A Moffer stu- that pair Mastering’s powerful Boxes, work through the steps of Problem-Solv- vertical axis. dents instructional support content with Knewton’s adaptive ing Strategies, and assess the applicability of the when and where they need learning engine to provide Models. The workbook is referenced throughout it, including links to the individualized help to students the text with the icon . © 2017 Pearson Education. eafoTnred xh wto, mrmoenawgth-oa rrnkes mawseesdrig ifanetmeiodenbn,a tcsk. bTtaosehpsfeioigcsresne e samdtdu iahdspocetmonivntesecw esftpoorltrulikoog,wn gisln-e uctdaplu kswd eaii tndhhgdo olrcdeno.s rse prerequisite topics. M30_KNIG3162_04_SE_C30.indd 8 09/25/15 4:07 PM A01_KNIG7429_04_GE_FM.indd 7 18/07/16 2:52 pm M32_KNIG2651_04_SE_C26.indd 716 10/6/15 9:29 AM

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