超短脉冲强测量.pptx

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1、In order to measure an event in time,you need a shorter one.To study this event,you need a strobe light pulse thats shorter.But then,to measure the strobe light pulse,you need a detector whose response time is even shorter.And so onSo,now,how do you measure the shortest event?Photograph taken by Har

2、old Edgerton,MITThe Dilemma第1页/共44页Ultrashort laser pulses are the shortest technological events ever created by humans.Its routine to generate pulses shorter than 10-13 seconds in duration,and researchers have generated pulses only a few fs(10-15 s)long.Such pulses have many applications in physics

3、,chemistry,biology,and engineering.You can measure any eventas long as youve got a pulse thats shorter.So how do you measure the pulse itself?You must use the pulse to measure itself.But that isnt good enough.Its only as short as the pulse.Its not shorter.Techniques based on using the pulse to measu

4、re itself have not sufficed.第2页/共44页To determine the temporal resolution of an experiment using it.To determine whether it can be made even shorter.To better understand the lasers that emit them and to verify models of ultrashort pulse generation.To better study media:the better we know the light in

5、 and light out,the better we know the medium we study with them.To use pulses of specific intensity and phase vs.time to control chemical reactions:“Coherent control.”To understand pulse-shaping efforts for telecommunications,etc.Because its there.Why measure an ultrashort laser pulse?As a molecule

6、dissociates,its emission changes color(i.e.,the phase changes),revealing much about themolecular dynamics,not avail-able from the mere spectrum,or even the intensity vs.time.Excitation to excited stateEmissionGround stateExcited state第3页/共44页ExptTheoryLinearLinear or nonlinearmediumMeasuring the int

7、ensity and phase of the pulses into and out of a medium tells us as much as possible about the linear and nonlinear effects in the medium.Studying Media by Measuring the Intensity and Phase of Light PulsesWith a linear medium,we learn the mediums absorption coefficient and refractive index vs.With a

8、 nonlinear-optical medium,we can learn about self-phase modulation,for example,for which the theory is much more complex.Indeed,theoretical models can be tested.Time(fs)IntensityPhaseNonlinearEaton,et al.,JQE 35,451(1999).Time(fs)IntensityPhase第4页/共44页A laser pulse has the time-domain electric field

9、:EI(t)1/2 exp i0t i(t)IntensityPhase(t)=Re Equivalently,vs.frequency:exp -ij j(0)Spectral Phase(neglecting thenegative-frequencycomponent)E()=Re S()1/2We must measure an ultrashort laser pulsesintensity and phase vs.time or frequency.SpectrumKnowledge of the intensity and phase or the spectrum and s

10、pectral phaseis sufficient to determine the pulse.第5页/共44页t d dtThe instantaneous frequency:Example:“Linear chirp”Phase,(t)timetimeFrequency,(t)timeWed like to be able to measure,not only linearly chirped pulses,but also pulses with arbitrarily complex phases and frequencies vs.time.The phase determ

11、ines the pulses frequency(i.e.,color)vs.time.第6页/共44页The spectrometer measures the spectrum,of course.Wavelength variesacross the camera,and the spectrum can be measured for a single pulse.Pulse Measurement in the Frequency Domain:The SpectrometerCollimating Mirror“Czerny-Turner”arrangementEntrance

12、SlitCamera orLinear Detector ArrayFocusingMirrorGrating“Imaging spectrometers”allow many spectra to be measured simultaneously.Broad-bandpulse第7页/共44页Pulse Measurement in the Time Domain:DetectorsExamples:Photo-diodes,Photo-multipliersDetectors are devices that emit electrons in response to photons.

13、Detectors have very slow rise and fall times:1 nanosecond.As far as were concerned,detectors have infinitely slow responses.They measure the time integral of the pulse intensity from to+:The detector output voltage is proportional to the pulse energy.By themselves,detectors tell us little about a pu

14、lse.Another symbolfor a detector:DetectorDetector第8页/共44页Pulse Measurement in the Time Domain:Varying the pulse delaySince detectors are essentially infinitely slow,how do we make time-domain measurements on or using ultrashort laser pulses?Well delay a pulse in time.And how will we do that?By simpl

15、y moving a mirror!Since light travels 300 m per ps,300 m of mirror displacement yields a delay of 2 ps.This is very convenient.Moving a mirror backward by a distance L yields a delay of:Do not forget the factor of 2!Light must travel the extra distance to the mirrorand back!Translation stageInput pu

16、lse E(t)E(tt)MirrorOutput pulse第9页/共44页We can also vary the delay using a mirror pair or corner cube.Mirror pairs involve tworeflections and displace the return beam in space:But out-of-plane tilt yieldsa nonparallel return beam.Corner cubes involve three reflections and also displace the return bea

17、m in space.Even better,they always yield a parallel return beam:“Hollow corner cubes”avoid propagation through glass.Translation stageInputpulseE(t)E(tt)MirrorsOutput pulseEdmundScientific第10页/共44页Measuring the interferogram is equivalent to measuring the spectrum.Pulse Measurement in the Time Domai

18、n:The Michelson Interferometer Pulse energy (boring)Field autocorrelation(maybe interesting,but)The FT of the field autocorrelation is just the spectrum!Beam-splitterInputpulseDelaySlow detectorMirrorMirrorE(t)E(tt)第11页/共44页Okay,so how do we measure a pulse?V.Wong&I.A.Walmsley,Opt.Lett.19,287-289(19

19、94)I.A.Walmsley&V.Wong,J.Opt.Soc.Am B,13,2453-2463(1996)Result:Using only time-independent,linear filters,complete characterization of a pulse is NOT possible with a slow detector.Translation:If you dont have a detector or modulator that is fast compared to the pulse width,you CANNOT measure the pul

20、se intensity and phase.with only linear measurements,such as a detector,interferometer,or a spectrometer.We need a shorter event,and we dont have one.But we do have the pulse itself,which is a start.And we can devise methods for the pulse to gate itself using optical nonlinearities.第12页/共44页Pulse Me

21、asurement in the Time Domain:The Intensity AutocorrelatorCrossing beams in an SHG crystal,varying the delay between them,and measuring the second-harmonic(SH)pulse energy vs.delay yields the Intensity Autocorrelation:The Intensity Autocorrelation:DelayBeam-splitterInputpulseAperture eliminates input

22、 pulsesand also any SH created by the individual input beams.Slow detectorMirrorE(t)E(tt)MirrorsSHGcrystalLens第13页/共44页Single-Shot AutocorrelationWhile this effect introduces a range of delays on any given pulse andcould cause a broadening of the trace in multi-shot measurements,it allows us to meas

23、ure a pulse on a single laser shot if we use a largebeam and a large beam angle to achieve the desired range of delays.第14页/共44页Single-Shot Autocorrelationc2第15页/共44页Single-Shot AutocorrelationInput pulse(expanded in space to 1 cm)Beam-splitterSHGcrystalCameraE(t)E(tt)Cylindrical lens focuses the be

24、am in the vertical direction(for high intensity),while the delay varies horizontally.No mirrormoves!Crossing the beams at a large angle,focusing with a cylindrical lens,and detecting vs.transverse position yields the autocorrelation for a single pulse.Lens images crystal onto camera and hence delayo

25、nto position at cameraThe beam must have constant intensityvs.horizontal position to avoid biases.Aperture第16页/共44页Single-Shot Autocorrelation of Longer PulsesIf a longer pulse is to be measured,a larger range of delays is required.A longer range can be achieved using a dispersive element,such as a

26、prism or grating,which tilts the pulse fronts.Angular dispersion is undesired,however.Fortunately,if we need to use this trick,its because the pulse is long.As a result,its bandwidth is usually small,so angular dispersion is less of a problem(for pulses 10 ps).第17页/共44页Practical Issues in Autocorrel

27、ationGroup-velocity mismatch must be negligible,or the measurementwill be distorted.Equivalently,the phase-matching bandwidth mustbe sufficient.So very thin crystals(1 J).第30页/共44页When a shorter reference pulse is available:The Intensity Cross-CorrelationThe Intensity Cross-correlation:DelayUnknown

28、pulseSlow detectorE(t)Eg(tt)SFGcrystalLensReference pulseIf a shorter reference pulse is available(it need not be known),then it can be used to measure the unknown pulse.In this case,we perform sum-frequency generation,and measure the energy vs.delay.If the reference pulse is much shorter than the u

29、nknown pulse,then the intensity cross-correlation fully determines the unknown pulse intensity.第31页/共44页Pulse Measurement in the Time Domain:The Interferometric AutocorrelatorWhat if we use a collinear beam geometry,and allow the autocorrelatorsignal light to interfere with the SHG from each individ

30、ual beam?Developed by J-C DielsUsualAutocor-relationtermNewtermsAlso called the“Fringe-Resolved Autocorrelation”FilterSlow detectorSHGcrystalLensBeam-splitterInputpulseDelayMirrorMirrorE(t)E(tt)Michelson InterferometerDiels and Rudolph,Ultrashort Laser Pulse Phenomena,Academic Press,1996.第32页/共44页In

31、terferometric Autocorrelation MathThe measured intensity vs.delay is:Multiplying this out:where第33页/共44页The Interferometric Autocorrelation is thesum of four different quantities.Constant(uninteresting)Sum-of-intensities-weighted w“interferogram”of E(t)w(oscillates at w in delay)Intensity autocorrel

32、ationInterferogram of the second harmonic;equivalent to the spectrum of the SH w(oscillates at 2w in delay)The interferometric autocorrelation simply combines several measuresof the pulse into one(admittedly complex)trace.Conveniently,however,they occur with different oscillation frequencies:0,w,and

33、 2w.第34页/共44页Interferometric Autocorrelation and StabilizationInterferometric Autocorrelation Traces for a Flat-phase Gaussian pulse:PulselengthFortunately,its not always necessary to resolve the fringes.With stabilizationWithout stabilizationTo resolve the w and 2w fringes,which are spaced by only

34、l and l/2,we must actively stabilize the apparatus to cancel out vibrations,which perturb the delay by many l.C.Rulliere,Femtosecond Laser Pulses,Springer,1998.第35页/共44页Interferometric Autocorrelation:ExamplesThe extent of the fringes(at w and 2w)indicates the approximate width ofthe interferogram,w

35、hich is the coherence time.If its the same as the w width of the the low-frequency component,which is the intensity w autocorrelation,then the pulse is near-Fourier-transform limited.w Unchirped pulse(short)Coherencetime PulselengthChirped pulse(long)Coherencetime PulselengthThe interferometric auto

36、correlation nicely reveals the approximate pulselength and coherence time,and,in particular,their relative values.Solid black lines have been added.They trace the intensity autocorrelation component(for reference).C.Rulliere,Femtosecond Laser Pulses,Springer,1998.第36页/共44页Does the interferometric au

37、tocorrelation yield the pulse intensity and phase?No.The claim has been made that the Interferometric Autocorrelation,combined with the pulse interferogram(i.e.,the spectrum),could do so Naganuma,IEEE J.Quant.Electron.25,1225-1233(1989).But the required iterative algorithm rarely converges.The fact

38、is that the interferometric autocorrelation yields little more information than the autocorrelation and spectrum.We shouldnt expect it to yield the full pulse intensity and phase.Indeed,very different pulses have very similar interferometric autocorrelations.第37页/共44页Pulses with Very Similar Interfe

39、rometric AutocorrelationsPulse#1IntensityPhasetFWHM=24fsPulse#2IntensityPhasetFWHM=21fsWithout trying to find ambiguities,we can just try Pulses#1 and#2:Despite the very different pulses,these IA traces are nearly identical!Chung and Weiner,IEEE JSTQE,2001.Interferometric Autocorrelations for Pulses

40、#1 and#2Difference:#1 and#2第38页/共44页Pulses with Very Similar Interferometric AutocorrelationsChung and Weiner,IEEE JSTQE,2001.Its even harder to distinguish the traces when the pulses are shorter,and there are fewer fringes.Consider Pulses#1 and#2,but 1/5 as long:Interferometric Autocorrelations for

41、 Shorter Pulses#1 and#2#1 and#2Pulse#1IntensityPhasetFWHM=4.8fs-20 -10 0 10 20Pulse#2IntensityPhasetFWHM=4.2fs-20 -10 0 10 20In practice,it would be virtually impossible to distinguish these traces also.Difference:第39页/共44页More Pulses with Similar Interferometric AutocorrelationsChung and Weiner,IEE

42、E JSTQE,2001.Without trying to find ambiguities,we can try Pulses#3 and#4:IntensityPhasetFWHM=37fsPulse#3IntensityPhasetFWHM=28fsPulse#4Interferometric Autocorrelations for Pulses#3 and#4Difference:#3 and#4Despite very different pulse lengths,these pulses have nearly identical IAs.第40页/共44页More Puls

43、es with Similar Interferometric AutocorrelationsShortening Pulses#3 and#4 also yields very similar IA traces:Interferometric Autocorrelations for Shorter Pulses#3 and#4Chung and Weiner,IEEE JSTQE,2001.Difference:Shortenedpulse(1/5as long)#3 and#4It is inappropriate to derive a pulse length from the

44、IA.IntensityPhasetFWHM=7.4fsPulse#3-40 -20 0 20 40IntensityPhasetFWHM=5.6fsPulse#4-40 -20 0 20 40第41页/共44页Interferometric Autocorrelation:Practical Details and ConclusionsA good check on the interferometric autocorrelation is that it should be symmetrical,and the peak-to-background ratio should be 8

45、.This device is difficult to align;there are five very sensitive degrees offreedom in aligning two collinear pulses.Dispersion in each arm must be the same,so it is necessary to insert a compensator plate in one arm.The typical ultrashort pulse is still many wavelengths long.So many fringes must typ

46、ically be measured:data sets are large,and scans are slow.It is difficult to distinguish between different pulse shapes and,especially,different phases from interferometric autocorrelations.Like the intensity autocorrelation,it must be curve-fit to an assumedpulse shape and so should only be used for rough estimates.第42页/共44页Questions:1.Please briefly introduce the characteristics of intensity autocorrelation(second-order),third-order autocorrelation,Interferometric Autocorrelations.第43页/共44页感感谢您的您的观看。看。第44页/共44页