超快光学 第19章 放大.ppt

上传人:牧羊曲112 文档编号:6394909 上传时间:2023-10-26 格式:PPT 页数:50 大小:5.91MB
返回 下载 相关 举报
超快光学 第19章 放大.ppt_第1页
第1页 / 共50页
超快光学 第19章 放大.ppt_第2页
第2页 / 共50页
超快光学 第19章 放大.ppt_第3页
第3页 / 共50页
超快光学 第19章 放大.ppt_第4页
第4页 / 共50页
超快光学 第19章 放大.ppt_第5页
第5页 / 共50页
点击查看更多>>
资源描述

《超快光学 第19章 放大.ppt》由会员分享,可在线阅读,更多相关《超快光学 第19章 放大.ppt(50页珍藏版)》请在三一办公上搜索。

1、The Amplification of Ultra-short Laser Pulses,Francois Salin Center for Intense Lasersand Applications(CELIA)Universit Bordeaux I,Francesalincelia.u-bordeaux.frGilles Darpentigny(CELIA),Vincent Bagnoud(LLE)Antoine Courjaud,Clemens Honninger,Eric Mottay(Amplitude Systemes),Luc Vigroux(Amplitude Techn

2、ologies)and some additional stuff from Dan Mittleman,Rice,Pulse compressor,t,t,Solid state amplifier,t,Dispersive delay line,t,Short pulse oscillator,Mostof this lecture courtesy of,Pulse energy vs.Repetition rate,Rep rate(pps),Pulse energy(J),Oscillator,Cavity-dumped oscillator,RegA,Regen,Regen+mul

3、tipass,Regen+multi-multi-pass,1 W average power,A t,What are the goals in ultrashort pulse amplification?,Ipeak=,E,Increase the energy(E),Decrease the duration(t),Decrease the area of the focus(A).,Maximum intensity on target,Needed to start the experiment,Needed to get useful results,Pave=E r,Signa

4、l is proportional to the number of photons on the detector per integration time.,Maximum average power at the detector,Pulseenergy,Rep rate,Pulseenergy,Beam area,Pulse length,Issues in Ultrafast Amplification and Their Solutions,Pulse length discrepancies:Multi-pass amplifiers and regenerative ampli

5、fiers(“Regens”).Damage:Chirped-Pulse Amplification(CPA)Gain saturation:Frantz-Nodvick EquationGain narrowing:Birefringent filtersThermal effects:cold and wavefront correctionSatellite pulses,Contrast,and Amplified Spontaneous Emission:Pockels cellsSystems cost lots of money:Earn more money,Cavity Du

6、mping,Before we consider amplification,recall that the intracavity pulse energy is 50 times the output pulse energy.So we have more pulse energy.How can we get at it?,What if we instead used two high reflectors,let the pulse energy build up,and then switch out the pulse?This is the opposite of Q-swi

7、tching:it involves switching from minimum to maximum loss,and its called“Cavity Dumping.”,Cavity dumping:the Pockels cell,A Pockels cell is a device that can switch a pulse(in and)out of a resonator.Its used in Q-switches and cavity dumpers.A voltage(a few kV)can turn a crystal into a half-or quarte

8、r-wave plate.,V,If V=0,the pulse polarization doesnt change.,If V=Vp,the pulse polarization switches to its orthogonal state.,Abruptly switching a Pockels cell allows us to extract a pulse from a cavity.This allows us to achieve 100 times the pulse energy at 1/100 the repetition rate(i.e.,100 nJ at

9、1 MHz).,Pockels cell(voltage may be transverse or longitudinal),Polarizer,Amplification of Laser Pulses,in General,Very simply,a powerful laser pulse at one color pumps an amplifier medium,creating an inversion,which amplifies another pulse.,Nanosecond-pulse laser amplifiers pumped by other ns laser

10、s are commonplace.,Laser oscillator,Amplifier medium,Pump,Energy levels,Jpump(lpump/lL),lL,lpump,Single-pass Amplification Math,Assume a saturable gain medium and J is the fluence(energy/area).Assume all the pump energy is stored in the amplifier,but saturation effects will occur.,At low intensity,t

11、he gain is linear:,At high intensity,the gain“saturates”and hence is constant:,Intermediate case interpolates between the two:,Jsto=stored pump fluence=Jpump(lpump/lL)Jsat=saturation fluence(material dependent),Single-pass Amplification Math,where the small signal gain per pass is given by:,This dif

12、ferential equation can be integrated to yield the Frantz-Nodvick equation for the output of a saturated amplifier:,Frantz-Nodvick equation,G,0,exp(,g,0,L),exp(,J,sto,J,sat,),Higher pumping(Jsto)means higher efficiency and higher saturation and so lower gain.So you can have high gain or high extracti

13、on efficiency.But not both.,Gain,Extraction efficiency(Jout/Jsto),J,sto,/J,sat,Jout/Jin,Another problem with amplifying ultrashort laser pulses,Another issue is that the ultrashort pulse is so much shorter than the(ns or ms)pump pulse that supplies the energy for amplification.,So should the ultrash

14、ort pulse arrive early or late?,Early:,Late:,Pump energy arrives too late and is wasted.,time,pump,pump,time,Energy decays and is wasted.,In both cases,pump pulse energy is wasted,and amplification is poor.,So we need many passes.,All ultrashort-pulse amplifiers are multi-pass.,This approach achieve

15、s much greater efficiency.,The ultrashort pulse returns many times to eventually extract most of the energy.,Two main amplification methods,Multi-pass amplifier,Regenerative amplifier,Another multi-pass amplifier,A Pockels cell(PC)and a pair of polarizers are used to inject a single pulse into the a

16、mplifier.,Regenerative amplifier geometries,This is used for 10-20-Hz repetition rates.It has a larger spot size in the Ti:sapphire rod.,The Ti:Sapphire rod is 20-mm long and doped for 90%absorption.,This design is often used for kHz-repetition-rate amplifiers.,Pulse intensities inside an amplifier

17、can become so high that damage(or at least small-scale self-focusing)occurs.Solution:Expand the beam and use large amplifier media.Okay,we did that.But thats still not enough.Solution:Expand the pulse in time,too.,Okay,so what next?,Chirped-Pulse Amplification,Chirped-pulse amplification in-volves s

18、tretching the pulse before amplifying it,and then compressing it later.,We can stretch the pulse by a factor of 10,000,amplify it,and then recompress it!,G.Mourou and coworkers 1983,CPA is THE big development.,Pulse compressor,t,t,Solid state amplifier,t,Dispersive delay line,t,Short pulse oscillato

19、r,Stretching and compressing ultrashort pulses,Okay,this looks just like a“zero-dispersion stretcher”used in pulse shaping.But when d f,its a dispersive stretcher and can stretch fs pulses by a factor of 10,000!With the opposite sign of d-f,we can compress the pulse.,Pulse stretcher,A pulse stretche

20、r,This device stretches an 18-fs pulse to 600 psa factor of 30,000!A ray trace of the various wavelengths in the stretcher:,Alexandrite,Ti:sapphire,Excimers,Nd:Glass,Dyes,Direct Amplification,Fluence(J/cm2),Pulse Duration(fs),CPA vs.Direct Amplification,CPA achieves the fluence of long pulses but at

21、 a shorter pulse length!,Regenerative Chirped-Pulse Amplification at 100 kHz rep rates with a cw pump,Coherent RegA amplifier,A fs oscillator requires only 5 W of green laser power.An Argon laser provides up to 50 W.Use the rest to pump an amplifier.Today,we use an intracavity-doubled Nd:YLF pump la

22、ser(10W).,Microjoules at 250 kHz repetition rates!,Regenerative chirped-pulse amplification with a kHz pulsed pump,Wavelength:800 nm(Repetition rates of 1 to 50 kHz)High Energy:2 mJ at 1 kHz Picosecond:80 ps,0.7 mJ at 1 kHzShort Pulse:0.7 mJ at 1 kHz,Spectra Physics regen:the“Spitfire”,Pump laser fo

23、r ultrafast amplifiers,Coherent“Corona”,high power,Q-switched green laser in a compact and more reliable diode-pumped package,15 mJ(ns)at a 10 kHz rep rate(150W ave power!),Extracted energy,Beam diameter,Pump power 100 W,Average Power,Rep rate,Average power for high-power Ti:Sapphire regens,These av

24、erage powers are high.And this pump power is also.If you want sub-100fs pulses,however,the energies will be less.,CPA is the basis of thousands of systems.Its available commercially in numerous forms.It works!,But there are some issues,especially if you try to push for really high energies:,Amplifie

25、d spontaneous emission(ASE)Gain saturation:gain vs.extraction efficiencyGain narrowingThermal aberrationsContrast ratioDamage threshold vs extraction efficiency,Amplified Spontaneous Emission(ASE),Fluorescence from the gain medium is amplified before(and after)the ultrashort pulse arrives.This yield

26、s a 10-30 ns background with low peak power but large energy.Depends on the noise present in the amplifier at t=0ASE shares the gain and the excited population with the pulse.,Amplification reduces the contrast by a factor of up to 10.,Gain Narrowing(and ASE),On each pass through an amplifier,the pu

27、lse spectrum gets multiplied by the gain spectrum,which narrows the output spectrumand lengthens the pulse!As a result,the pulse lengthens,and it can be difficult to distinguish the ultrashort pulse from the longer Amplified Spontaneous Emission(ASE),Gain narrowing example,Ti:sapphire gain cross sec

28、tion,10-fs sech2 pulse in,Normalized spectral intensity,Cross section(*10-19 cm2),Wavelength(nm),65-nm FWHM,32-nm FWHM,Factor of 2 loss in bandwidth for 107 gainMost Terawatt systems have 1010 small signal gain,longer pulse out,Beating gain narrowing,Introduce some loss at the gain peak to offset th

29、e high gain there.,Gain and loss,Spectrum:before and after,Gain-Narrowing Conclusion,Gain narrowing can be beaten.We can use up to half of the gain bandwidth for a 4-level system.Sub-20 fs in Ti:sapphireSub-200 fs in Nd:glassSub-100 fs in Yb:XX,Intensity(arb.units),Wavelength(nm),Very broad spectra

30、can be created this way.,A 100-nm bandwidth at 800 nm can support a 10-fs pulse.,Heat deposition causes lensing and small-scale self-focusing.These thermal aberrations increase the beam size and reduce the available intensity.,Ipeak=,E,A T,We want a small focused spot size,but thermal aberrations in

31、crease the beam size,not to mention screwing it up,too.,Now the average power matters.The repetition rate is crucial,and wed like it to be high,but high average power means more thermal aberrations,Thermal Effects in Amplifiers,Low temperature minimizes lensing.,Calculations for kHz systemsCryogenic

32、 cooling results in almost no focal power,In sapphire,conductivity increases and dn/dT decreases as T decreases.,Murnane,Kapteyn,and coworkers,Static Wave-front Correction,2.5 times improvement in peak intensity has been achieved,CUOS,Dynamic Correction of Spatial Distortion,50 mm diameter37 actuato

33、rs,CUOS,Contrast ratio,Why does it take over 2 years between the first announcement of a new laser source and the first successful experiment using it?,Because the pulse has leading and following satellite pulses that wreak havoc in any experiment.If a pulse of 1018 W/cm2 peak power has a“little”sat

34、ellite pulse one millionth as strong,thats still 1 TW/cm2!This can do some serious damage!,Ionization occurs at 1011 W/cm2so at 1021 W/cm2 we need a 1010 contrast ratio!,Major sources of poor contrast,Nanosecond scale:pre-pulses from oscillatorpre-pulses from amplifierASE from amplifier,Picosecond s

35、cale:reflections in the amplifierspectral phase or amplitude distortions,0-1-2-3-4-5-6-7-8-9-10,Front,Back,time,Spectral phase aberrations,Pre-pulses,ASE,0,ps,10 ns,ns,FWHM,Amplified pulses often have poor contrast.,Log(Energy),Pre-pulses do the most damage,messing up a medium beforehand.,Typical 3r

36、d-order autocorrelation,Amplified pulses have pre-and post-pulses.,A Pockels cell“Pulse Picker”,A Pockels cell can pick a pulse from a train and suppress satellites.To do so,we must switch the voltage from 0 to kV and back to 0,typically in a few ns.,V,Time,Voltage,fewns,Switching high voltage twice

37、 in a few ns is quite difficult,requiring avalanche transistors,microwave triodes,or other high-speed electronics.,amplifier,oscillator,stretcher,compressor,Pockels cells,10-2-10-3,10 ns,Pockels cells suppress pre-and post-pulses.,Unfortunately,Pockels cells arent perfect.They leak 1%.,Contrast impr

38、ovement recipes,A Pockels cell improves the contrast by a few 100 to 1000.,We need at least 3 Pockels cells working in the best conditions:on axis(do not tilt Pockels cells)broadband high-contrast polarizers(not dielectric)fast rise time(2 ns 10-90%)collimated beamsTemperature drift is also a proble

39、m in Pockels cells.Also:Good pump synchronization gives a factor 3-10,Multiple-stage multi-pass amplifiers,1 kHz Multi-pass system at the University of Colorado(Murnane and Kapteyn),0.2 TW,4 mJ,20 fs pulse length,Closed loop cryogenic cooling 100K,5 x 1J,20 Hz Nd:YAG lasers,10 fs oscillator,stretche

40、r,100 Hz Regenerative amplifier,200 mJ,30 fs,100 Hz,High energy,high contrast 100-Hz system at CELIA,Pump beam,Ultrashort pulse-near field,Ultrashort pulse-far field,Amplified-pulse beam shapes,A 1-Joule Apparatus,Multi-Joule Systems,Nd:GlassEnergy 20 JoulesPulsewidth 40 TWRepetition rates every hou

41、r,Terawatt Laser SystemTi:sapphireEnergy 1 JoulePulsewidth 10 TWRepetition rates to 1 kHz,You can buy these lasers!,Lawrence Livermore National Labs High-Power Amplifiers,Laser Specifications,Even Higher Intensities!,National Ignition Facility(under construction),192 shaped pulses10.4 kJ per beam in UV(done)21 kJ per beam in IR(done)1.8 MJ total energy(planned)Pulses 0.2 to 25 ns in length,What to do with such high intensities,

展开阅读全文
相关资源
猜你喜欢
相关搜索
资源标签

当前位置:首页 > 生活休闲 > 在线阅读


备案号:宁ICP备20000045号-2

经营许可证:宁B2-20210002

宁公网安备 64010402000987号