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ID:41906675
大小:1.96 MB
页数:44页
时间:2019-09-04
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1、拉曼光谱分析法RemoteRamanAnalysisonPlanetaryMissionsToallowRamanspectroscopyatrangeof10'sofmeters.ThisNASA-fundedprojectisaimedatMarslandersorlandersonotherplanets,butalsohasterrestrialuses.激光拉曼光谱基本原理Rayleigh散射:弹性碰撞;无能量交换,仅改变方向;Raman散射:非弹性碰撞;方向改变且有能量交换;Rayleigh散射Raman散
2、射E0基态,E1振动激发态;E0+h0,E1+h0激发虚态;获得能量后,跃迁到激发虚态.(1928年印度物理学家RamanCV发现;1960年快速发展)hE0E1V=1V=0h0h0h0h0+E1+h0E0+h0h(0-)激发虚态基本原理1.Raman散射Raman散射的两种跃迁能量差:E=h(0-)产生stokes线;强;基态分子多;E=h(0+)产生反stokes线;弱;Raman位移:Raman散射光与入射光频率差;ANTI-STOKES0-RayleighS
3、TOKES0+0h(0+)E0E1V=1V=0E1+h0E2+h0hh0h(0-)Rayleigh/RamanTransitionsIRAbsorptionsRayleigh/RamanTransitionsandSpectraRayleigh/RamanTransitionsandSpectraTheSpectrumAcompleteRamanspectrumconsistsof:•aRayleighscatteredpeak(highintensity,samewavelengthase
4、xcitation)•aseriesofStokes-shiftedpeaks(lowintensity,longerwavelength)•aseriesofanti-Stokesshiftedpeaks(stilllowerintensity,shorterwavelength)•spectrumindependentofexcitationwavelength(488,632.8,or1064nm)SpectrumofCCl4,usinganAr+laserat488nm.RamanSpectroscopyAnot
5、herspectroscopictechniquewhichprobestherovibrationalstructureofmolecules.C.V.Ramandiscoveredin1928;receivedNobelPrizein1931.Canprobegases,liquids,andsolids.Mustusealasersourceforexcitation.Resurgenceinrecentyearsduetothedevelopmentofnewdetectorswithimprovedsensit
6、ivity.ShiftbackawayfromFT-RamantodispersiveRamanwithmultichanneldetectorsystems.InfraredandRamanSpectraofBenzeneIRRaman拉曼光谱与红外光谱分析方法比较SomeRamanAdvantagesHerearesomereasonswhysomeonewouldprefertouseRamanSpectroscopy.•Non-destructivetosamples(minimalsampleprep)•Hig
7、hertemperaturestudiespossible(don’tcareaboutIRradiation)•Easilyexaminelowwavenumberregion:100cm-1readilyachieved.•Bettermicroscopy;usingvisiblelightsocanfocusmoretightly.•Easysampleprep:waterisanexcellentsolventforRaman.Canprobesamplethroughtransparentcontainers(
8、glassorplasticbag).WatchforFluorescenceSpectrumofanthracene.A:usingAr+laserat514.5nm.B:usingNd:YAGlaserat1064nm.Wanttouseshortwavelengthbecausescatteringdepend
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