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1、1IntroductiontoEectiveFieldTheoryBarryR.HolsteinaaDepartmentofPhysics-LGRTUniversityofMassachusetts,Amherst,MA010031.IntroductionThebasicideabehindeectiveeldtheory(EFT)methodsistodescribenatureintermsofafullyconsistentquantumeldtheory,butonewhichisv
2、alidinalimitedenergyrange.NowstrictlyspeakingthismeansthatalmostanytheoryisanEFTexceptstringtheoriesthattrytobeatheoryofeverything(TOE).Indeedeventhequintessentialquantumeldtheory
3、quantumelectrodynamics
4、isanEFTinthatitmustbreakdownattheveryhighestenerg
5、ies.Infactwerepresentthehighenergycontributionintermsofacontertermwhich,togetherwiththedivergentcomponentfromtheloopintegration,wetintermsoftheexperimentalmassandcharge.Inordertogetabetterfeelforthisideaitisusefultoconsiderasimplerexamplefromtheregimeo
6、fordinaryquantummechanics
7、thatofRayleighscattering,orwhytheskyisblue.1.1.RayleighScatteringBeforeproceedingtoQCD,let'srstexamineeectiveeldtheoryinthesimplercon-arXiv:nucl-th/0010015v14Oct2000textofordinaryquantummechanics,inordertogetfamiliarwiththei
8、dea.Specically,weexaminethequestionofwhytheskyisblue,whoseanswercanbefoundinananal-ysisofthescatteringofphotonsfromthesunbyatomsintheatmosphere
9、Comptonscattering.[1]Firstweexaminetheproblemusingtraditionalquantummechanicsand,forsimplicity,considerelast
10、ic(Rayleigh)scatteringfromsingle-electron(hydrogen)atoms.TheappropriateHamiltonianisthen(p~ eA~)2H=+e(1)2mandtheleading
11、O(e2)
12、amplitudeforComptonscatteringisgivenbytheFeynmandiagramsshowninFigure1as"e2=m1X^<0jp~e i~qf~rjn>^fiAmp=
13、 p^i^f+2!i2!fmn!i+E0 En!#^<0jp~ei~qi~rjn>^