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1、1IntroductiontoEectiveFieldTheoryBarryR.HolsteinaaDepartmentofPhysics-LGRTUniversityofMassachusetts,Amherst,MA010031.IntroductionThebasicideabehindeectiveeldtheory(EFT)methodsistodescribenatureintermsofafullyconsistentquantumeldtheory,butonewhichisvalidinalimitede
2、nergyrange.NowstrictlyspeakingthismeansthatalmostanytheoryisanEFTexceptstringtheoriesthattrytobeatheoryofeverything(TOE).Indeedeventhequintessentialquantumeldtheory
3、quantumelectrodynamics
4、isanEFTinthatitmustbreakdownattheveryhighestenergies.Infactwerepresentthehighen
5、ergycontributionintermsofacontertermwhich,togetherwiththedivergentcomponentfromtheloopintegration,wetintermsoftheexperimentalmassandcharge.Inordertogetabetterfeelforthisideaitisusefultoconsiderasimplerexamplefromtheregimeofordinaryquantummechanics
6、thatofRayleighscatt
7、ering,orwhytheskyisblue.1.1.RayleighScatteringBeforeproceedingtoQCD,let'srstexamineeectiveeldtheoryinthesimplercon-arXiv:nucl-th/0010015v14Oct2000textofordinaryquantummechanics,inordertogetfamiliarwiththeidea.Specically,weexaminethequestionofwhytheskyisblue,whosea
8、nswercanbefoundinananal-ysisofthescatteringofphotonsfromthesunbyatomsintheatmosphere
9、Comptonscattering.[1]Firstweexaminetheproblemusingtraditionalquantummechanicsand,forsimplicity,considerelastic(Rayleigh)scatteringfromsingle-electron(hydrogen)atoms.TheappropriateHami
10、ltonianisthen(p~ eA~)2H=+e(1)2mandtheleading
11、O(e2)
12、amplitudeforComptonscatteringisgivenbytheFeynmandiagramsshowninFigure1as"e2=m1X^<0jp~e i~qf~rjn>^fiAmp= p^i^f+2!i2!fmn!i+E0 En!#^<0jp~ei~qi~rjn>^