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Classical Mechanics

ClassicalMechanicsAnintroductorycourseRi chardFitzpatrickAssociateProfessor ofPhysicsTheUniversity :.. classicalmechanics?.. xes.. cant gures..122 Motionin1 ..263 Motionin3 .. parallelogram..444 Newton' .. 's rstlawofmotion.. 'ssecondlawofmotion.. 'slaw.. 'sthirdlawofmotion.. ,pulleys,andinclines.. elds.. 'slaw.. general1-dimensionalpotential.. rotationa vector?.. pointparticle.. multi-componentsystem.. laminarobjectina gravitational eld.. stretchedstring.. :ThesourceswhichI consultedmostfrequentlywhilstdevelopingt hiscourseare: ,Thirdedition(Holt,Rinehart,& Winston,NewYorkNY, 1977). , , ,Fourthedition, (JohnWiley& Sons,NewYorkNY, 1992).Encyclop diaBrittanica:Fifteenthedition(Encyclop diaBrittanica,ChicagoIL,1994).

Physics for scientists and engineers: R.A. Serway, and R.J. Beichner, Fifth edition, Vol. 1 (Saunders College Publishing, Orlando FL, 2000). 1.2 What is classical mechanics? Classical mechanics is the study of the motion of bodies (including the special case in which bodies remain at rest) in accordance with the general principles

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Transcription of Classical Mechanics

1 ClassicalMechanicsAnintroductorycourseRi chardFitzpatrickAssociateProfessor ofPhysicsTheUniversity :.. classicalmechanics?.. xes.. cant gures..122 Motionin1 ..263 Motionin3 .. parallelogram..444 Newton' .. 's rstlawofmotion.. 'ssecondlawofmotion.. 'slaw.. 'sthirdlawofmotion.. ,pulleys,andinclines.. elds.. 'slaw.. general1-dimensionalpotential.. rotationa vector?.. pointparticle.. multi-componentsystem.. laminarobjectina gravitational eld.. stretchedstring.. :ThesourceswhichI consultedmostfrequentlywhilstdevelopingt hiscourseare: ,Thirdedition(Holt,Rinehart,& Winston,NewYorkNY, 1977). , , ,Fourthedition, (JohnWiley& Sons,NewYorkNY, 1992).Encyclop diaBrittanica:Fifteenthedition(Encyclop diaBrittanica,ChicagoIL,1994).

2 Physicsfor , , Fifthedition, (SaundersCollegePublishing,OrlandoFL,200 0). classicalmechanics?Classicalmechanicsis thestudyofthemotionofbodies(includingthe specialcaseinwhichbodiesremainatrest)ina ccordancewiththegeneralprinciples rstenunciatedbySirIsaacNewtoninhisPhilos ophiaeNaturalisPrincipiaMath-ematica(168 7),commonlyknownasthePrincipia. Classicalmechanicswasthe rstbranchofPhysicstobediscovered,andis , classicalmechanicshasmanyim-portantappli cationsinotherareasofscience,suchasAstro nomy( , celestialmechanics),Chemistry( , thedynamicsof molecularcollisions),Geology( ,thepropagationofseismicwaves,generatedb yearthquakes,throughtheEarth'scrust),and Engineering( , theequilibriumandstabilityofstructures).

3 Classi-calmechanicsis alsoofgreatsigni ,thesequenceofeventsleadingtothediscover yofclassicalmechanics startingwiththeground-breakingworkofCope rnicus,continuingwiththeresearchesofGali leo,Kepler, andDescartes,andculminatingin classicalmechanics?ofNewton involvedthecompleteoverthrowoftheAristot elianpictureoftheUniverse,whichhadprevio uslyprevailedformorethana millennium,anditsreplacementbya recognizablymodernpictureinwhichhumankin dnolongerplayeda ,including:Translationalmotion motionbywhicha bodyshiftsfromonepointinspacetoanother( , themotionofa bullet redfroma gun).Rotationalmotion motionbywhichanextendedbodychangesorient ation,withrespecttootherbodiesinspace,wi thoutchangingposition( , themotionofa spinningtop).

4 Oscillatory motion motionwhichcontinuallyrepeatsin timewitha xedperiod( , themotionofa pendulumina grandfatherclock).Circular motion motionbywhicha bodyexecutesa circularorbitaboutanother xedbody[ , the(approximate)motionoftheEarthaboutthe Sun].Ofcourse,thesedifferenttypesofmotio ncanbecombined:forinstance,themotionofa properlybowledbowlingballconsistsofa combinationoftrans-lationalandrotational motion,whereaswavepropagationis a , , , thesubdivisionofmechanicswhichis obviouslyofgreatimportanceincivilenginee ring:forinstance,theprinciplesofstaticsw ereusedtodesignthebuildinginwhichthislec tureis takingplace,soastoensurethatit rstprincipleofanyexactscienceismeasureme nt. , ,ormass, length,mass, andtime ,andmostengineers,is calledthemkssystem afterthe rstinitialsofthenamesoftheunitsoflength, mass,andtime,respectively, , themeter, thekilogram, themeter(symbolm),whichwasformerlythedis -tancebetweentwoscratchesona platinum-iridiumalloybarkeptattheInter-n ationalBureauofMetricStandardinS evres,France,butis nowde nedasthedistanceoccupiedby1; 650;763:73wavelengthsof lightof massis thekilogram(symbolkg),whichis de nedasthemassofa platinum-iridiumalloycylinderkeptattheIn ternationalBureauofMetricStandardinS evres, thesecond(symbols),whichwasformerlyde nedintermsoftheEarth'srotation,butis nowde nedasthetimefor9; 192;631.

5 770oscillationsassociatedwiththetransiti onbetweenthetwohyper nelevelsof ,classicalmechanicsalsodealswithderivedq uantities, suchasvelocity, acceleration,momentum, xesmentum, ,mass, ,therefore,thecorrespondingcombinationso fthemksunitsoflength,mass, ,a velocitycanbereducedtoa lengthdividedbya ,themksunitsofvelocityaremeterspersecond :[v] =[L][T]=m s-1:( )Here,vstandsfora velocity,Lfora length,andTfora time,whereastheoperator[ ]representstheunits,ordimensions, masstimesa velocity. Hence,themksunitsofmomentumarekilogram-m eterspersecond:[p] = [M][v] =[M][L][T]=kgm s-1:( )Here,pstandsfora momentum,andMfora , xesmksunitsarespeci , mksunitstendtobecomeratherunwieldywhende alingwithmotionsonverysmallscales( , themotionsofmolecules)orverylargescales( , themotionofstarsintheGalaxy).

6 Inordertohelpcopewiththisproblem,a setofstandardpre xeshasbeendevised,whichallowthemksunitso flength,mass,andtimetobemodi edsoastodealmoreeasilywithverysmallandve rylargequantities:thesepre xesarespeci ,akilometer(km)represents103m,ananometer (nm)represents10-9m,andafemtosecond(fs)r epresents10-15s. Thestandardpre xSymbolFactorPre xSymbol1018exa-E10-1deci-d1015peta-P10-2 centi-c1012tera-T10-3milli-m109giga-G10- 6micro- 106mega-M10-9nano-n103kilo-k10-12pico-p1 02hecto-h10-15femto-f101deka-da10-18atto -aTable1:Standardpre , theobsoletecgs(centimeter-gram-second)sy stemandtheevenmoreobsoletefps(foot-pound -second)systemarestillinusetoday, althoughtheircontinuedem-ploymentis nowstronglydiscouragedinscienceandengine ering(exceptintheUS!)

7 Conversionbetweendifferentsystemsofunits is,inprinciple,perfectlystraightforward, but,inpractice,a frequentsourceoferror. Witness,forex-ample, esthevariousconversionfactorsbetweenmks, cgs, ,ratherconfusingly(unlessyouareanenginee rin theUS!),a poundis a unitof force, (1ft=12in),theyard(1ya=3ft),andthemile(1 mi=5; 280ft).Additionalnon-standardunitsofmass includetheton(intheUS,1ton=2; 000lb;intheUK,1ton=2; 240lb),andthemetricton(1tonne=1; 000kg).Finally, additionalnon-standardunitsoftimeinclude theminute(1min=60s),thehour(1hr=3; 600s),theday(1da=86;400s),andtheyear(1yr =365:26da=31;558;464s). cant gures1 cm=10-2m1 g=10-3kg1 ft=0:3048m1 lb=4:448N1 slug=14:59kgTable2 cant guresInthiscourse,youareexpectedtoperfor mcalculationstoa relativeaccuracyof1% , tothreesigni cant gures.

8 Sinceroundingerrorstendtoaccumulatedurin glengthycalculations,theeasiestwayin whichto achievethisaccuracyis toperformallintermediatecalculationstofo ursigni cant gures, andthentoroundthe nalresultdowntothreesigni cant oneofthequantitiesinyourcalculationturns outtothethesmalldifferencebetweentwomuch largernum-bers,thenyoumayneedtokeepmoret hanfoursigni cant ,youarestronglyurgedtousescienti cnotationinallofyourcalculations:theuseo fnon-scienti cnotationis generallya yourcalculatorsarecapableofoperatingina modeinwhichallnumbers(notjustverysmallor verylargenumbers)aredisplayedinscienti ,length,mass,andtimearethreefundamentall ydifferentquantitieswhicharemeasuredin ,therefore,makesnosensefora prospectivelawofphysicstoexpressanequali tybetween(say)a lengthanda ,theexamplelawm=l;( )wheremis a massandlis a length, ( ) is invalid(asa lawof physics),is to , ifm=linmksunits,thenm6= fpsunits,becausetheconversionfactorswhic hmustbeappliedtotheleft-andright-handsid esdiffer.

9 Physicistsholdverystronglytotheassumptio nthatthelawsofphysicspossessobjectiverea lity: inotherwords, thisassumptionis thata lawofphysicsmusttakethesameforminallposs iblesystemsofunitsthataprospectiveobserv ermightchoosetoemploy. Theonlywayinwhichthiscanbethecaseis if , thequantitiesontheleft-andright-handside softheequalitysigninanygivenlawofphysics musthavethesamedimensions( , thesamecombinationsof length,mass,andtime).A dimensionallyconsistentequationnaturally takesthesameforminallpossiblesystemsofun its, ,letusconsiderwhatis probablythemostfamousequationinphysics:E =m c2:( )Here,Eistheenergyofa body,misitsmass, [M][L2]=[T2], andthedimensionsofvelocityare[L]=[T]. Hence,thedimensionsoftheleft-handsideare [M][L2]=[T2],whereasthedimensionsoftheri ght-handsideare[M] ([L]=[T])2= [M][L2]=[T2].

10 It followsthatEq.( ) ,E=m c2holdsgoodinmksunits,incgsunits,infpsun its, c, orE=m c3, thenhiserrorwouldhavebeenimmediatelyappa renttootherphysicists, ,E=m c2representstheonlysimple,dimensionallyc onsistentwayofcombininganenergy, a mass,andthevelocityoflightina , shouldbenotedthatdimensionalanalysisis offairlylimitedappli-cability, andis a poorsubstituteforanalysisemployingtheact uallawsof physics;nevertheless,it is specialeffectsstudiowantsto lma ,thestudiomightmakea scalemodelofthetower, :TheLeaningTowerof Pisais (say)1 mtall,andthen lmthemodelfallingover. Theonlyproblemis thattheresultingfootagewouldlookcomplete lyunrealistic,becausethemodeltowerwouldf allovertooquickly. Thestudiocouldeasily xthisproblembyslowingthe bywhatfactorshouldthe lmbesloweddowninordertomakeit lookrealistic?


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