The availability of laser sources generating optical pulses of ultrashort duration (i.e. less than 10 picoseconds) has given the possibility to analyze the time dynamics of phenomena in specific media on time scales of picoseconds to attoseconds. These laser pulses are characterized by a broad spectrum of optical frequencies, the frequency range Δv being related to the minimum duration of the pulse Δt (also known as the Fourier Transform Limit) by the approximate relationship Δv≈1/Δt, implying Δv values exceeding 0.1 TeraHertz (THz).
A particularly effective method in the state of the art to achieve the study of time dynamics is the pump and probe technique, wherein an original laser pulse is used to produce two secondary pulses, named respectively pump pulse and probe pulse. The pump pulse excites the medium under study at time t0, and the probe pulse suitably delayed by a time δt with respect to the pump pulse is used to monitor some properties of the medium under study at time t0+δt. Repeating this experiments for different delay times δt yields a kind of slow motion picture of the ultrafast dynamics For instance, the probe pulse may traverse the medium and measuring its intensity can be used to monitor optical absorption as a function of time. An interesting variation of the pump and probe technique is Terahertz spectroscopy, wherein the pump pulse is sent to an electro-optic generator, to excite an electrical pulse in the THz range of frequencies. Examples of electro-optic generators are a photoconductor with an applied voltage or anon-linear optical material capable of optical rectification. An electro-optic detector is submitted to the probe pulse and to the THz wave, after it has interacted with the medium understudy. This achieves sampling of the THz wave. Such electro-optic detectors produce a signal proportional to the product of the THz wave electric field and the probe pulse energy. An implementation of an electro-optic detector can for instance use the polarization rotation in an electro-optic medium generated by the THz wave field, such rotation being measured by the transmission of the probe pulse through a suitable combination of the electro-optic medium and polarizers. A photoconductor polarized by the THz field and excited by the probe pulse can also be used as a detector.
In general, these measurements involve problems of sensitivity due to the small magnitude of the effects involved and to the short duration of the sampling probe pulse. It is usually necessary to sum the measurement observed over a number of successive laser pulses to obtain a meaningful result. Because measurements will always be subject to drifts of different origins, it is also desirable to vary rapidly the relevant parameter, in the present case the time delay, so that drifts can be minimal during the time of measurement. A desirable measurement condition, is thus to obtain a full measurement of the relevant delay interval in as short a time as possible, then repeat this measurement a sufficient number of times, summing separately the values for each individual δt, in order to improve the signal to noise ratio. From these considerations, it is clear that a scanning method for the delay δt is required with the maximum possible repetition rate. Also, a high precision for the delay is desirable leading to criteria for the stability and the magnitude of the delay difference between successive optical pulses.
In the state of the art, two main scanning methods have been used. The first one uses a mechanical delay line, wherein the delay is controlled by the different in length of two separate optical paths, for the pump and probe pulse respectively. This method leads to notoriously low scanning rates, typically limited to a few tens of Hertz, due to the inertia of the mechanical components. It is thus inadequate for rapid scanning Faster techniques have been developed based on rotatable mirrors or quickly moving loudspeaker diaphragms, which can attain scan rates of 100 Hz up to a few kHz. However, with a time jitter between scansfar exceeding one femtosecond, these techniques are less precise and therefore unsuitable for analyzing processes occurring on few femtosecond and attosecond timescales.
The second method, described for instance in “Bartels et al. 2007” (Bartels, A., R. Cerna, C. Kistner, A. Thoma, F. Hudert, C. Janke, and T. Dekorsy. 2007. “Ultrafast time-domain spectroscopy based on high-speed asynchronous optical sampling.” Review of Scientific Instruments 78 (3): 035107), uses no mechanical delay, but instead relies on two separate laser sources for the pump and probe pulse respectively. These sources each generate a train of pulses, but the pulse repetition frequency is chosen to be slightly different for the pump and probe sources, by an amount df=f2−f1., where f2 and f1 are the probe and pulse repetition frequencies respectively. Hence for each successive pulse/probe pairs, the time difference between pulse and probe will be increased by a value dt=1/f1−1/f2. Using typical values of 100 MHz for f1 and f2 and 10−4 of relative difference df/f , it is possible to obtain 10000 different sampling points, by increments of 1 ps, in the scanning range of amplitude 0 to 10 ns, and a repetition rate of 10 KHz. The same reasoning applied to a 1 GHz repetition rate source yields a range of 1 ns and a repetition rate of 100 KHz. This method is generally referred as asynchronous optical sampling (ASOPS). Besides the complexity and cost associated with the requirement for two sources, the latter method has two disadvantages. First, many studies are interested in delay ranges significantly shorter than 1-10 ns. Consequently, a large part of the data measured is insignificant and lost. Second the synchronization between the two sources is done by electronic means and limited by inherent electronic jitter. The scan precision in the state of the art does not reach values below 50 fs. This is of the same order as the minimum difference of delay between successive pulses.
It is the aim of the present invention to provide a scanning method, with rates of more than 1kHz, scanning amplitude of order 10 ps and precision of 1 fs or better. The method is based on acousto-optic diffraction under Bragg conditions, denominated as Bragg diffraction, the principles of which are described for instance in “Xu and Stroud” (Xu, Jieping, and Robert Stroud. 1992. Acousto-Optic Devices: Principles, Design, and Applications. Wiley-Interscience, June.). The acousto-optic Bragg diffraction of ultrashort optical pulses, with broad frequency bandwidth, by multifrequency acoustic pulses has been described in the art, in particular in “Kaplan and Tournois 2002” (Kaplan, D., and P. Tournois. 2002. “Theory and performance of the acousto optic programmable dispersive filter used for femtosecond laser pulse shaping.” Journal de Physique IV Proceedings 12 (5): 69-75. doi:10.1051/jp4:20020098).
Considering first monochromatic optical and acoustic waves, it is known, that the diffraction of an optical wave by an acoustic wave satisfies the following phase conservation rule at any given point:
φ=φ0+Φ+constant (1)
where the respective phases φ, φ0 and Φ of the diffracted wave, incident wave and acoustic wave are indicated. We consider a monochromatic acoustic real strain field of the form:
s=s
0·Cos({right arrow over (K)}·{right arrow over (r)}−ΩT)
where s0 is a constant, {right arrow over (r)} is the position vector, {right arrow over (K)} the acoustic wave vector, Ω the angular frequency associated with the acoustic wave and T the corresponding time, written as a capital letter. This field can be considered as the superposition of complex components proportional to Exp(iΦ) and Exp(−iΦ) where
Φ={right arrow over (K)}·{right arrow over (r)}−ΩT
The theory of Bragg diffraction states that relation (1) has to be satisfied at all points in space for efficient diffraction, in a bulk medium, which leads to the wavevector conservation rule (Bragg law):
{right arrow over (k)}={right arrow over (k)}
0
+ε·{right arrow over (K)}
where {right arrow over (k)} and {right arrow over (k)}0 are respectively the diffracted and incident optical wavector and ε is either +1 or −1 depending of which of the acoustic complex components has been used to satisfy the Bragg law. A frequency conservation rule is also necessary, but because acoustic frequencies are very small compared to the optical frequencies, it is appropriate to neglect the frequency change in the diffraction (Doppler effect) compared to the optical signal spectral bandwidth, and thus consider that the optical diffracted wave has the same angular frequency ω=2πv as the incident wave.
Under conditions where Bragg law is satisfied, eq(1) implies the following relation.
φ=φ0+ε·Ω˜T+constant (2)
For a given material, given geometric conditions and given optical frequencies, Ω is related to ω. A person skilled in the art, taking into account the frequency dependence of optical indices of refraction, can derive from Bragg law the precise form relationship, which can be calculated with a high degree of precision. In the limit case, where the acoustic velocity does not depend on acoustic frequency and the optical indices of refraction do not depend on optical frequency, it is easily derived that Ω is proportional to ω with a proportionality factor K of order 10−7 to 10−5, depending on materials and geometric configurations. The people skilled in the art can then synthesize a multifrequency acoustic signal, with frequencies matching the frequencies present in the optical signal. This multifrequency acoustic signal will have the form of an acoustic pulse, whose time shape is the Fourier transform of its complex spectrum.
Derivating (2) with respect to optical angular frequency, one finds that the time delay τ of the diffracted optical wave is:
which demonstrates that the diffraction produces a time dependent delay, i.e. delay scanning. The sign of this scan is determined by e and can be designed by the person skilled in the art to be positive or negative depending on the geometry used to satisfy Bragg law. The required function of scan delay is thus accomplished. If the differential of the acoustic frequency has a non negligible dependence upon frequency, i.e. if the factor K is not a constant, then the delay will be different for different spectral regions of the optical signal, i.e. the signal will be subject to some modifications of its time shape during the scanning process. This problem will be addressed in the final section of this description. For the time being, the relationship Ω=K·ω will be assumed, with the aim of simplifying the description of the invention principle.
In the art, the use of acoustic diffraction to control the spectral phase of an optical signal, by the phase of an acoustic signal using eq. (1), has been described in particular in “Kaplan and Tournois 2002”, “Molchanov et al. 2010” Molchanov, V Ya, Sergey I Chizhikov, Oleg Y. Makarov, Efim A Khazanov, and Vladislav N Ginzburg. 2010. Acoustooptical delay lines for femtosecond pulse shaping based on crystal materials with strong acoustic anisotropy. In Vol. 7789. Proceedings of SPIE—The International Society for Optical Engineering. Bellingham, Wash., ETATS-UNIS: Society of Photo-Optical Instrumentation Engineers and “Pierre Tournois 2000” (Tournois, Pierre. 2000. Device for controlling light pulses by a programmable acoustooptic device. June 6) as a mean to achieve a given optical pulse time shape. In “Molchanov et al. 2010”, the authors use the denomination “dispersive acousto-optic delay line” to describe the apparatus achieving this function. In the patent “Pierre Tournois 2000” the inventor addresses more specifically the use of this effect to control pulse compression in ultrafast amplifier system. In the three above references and similar references in the state of the art, the acoustic time variation between successive optical pulses is not considered, the acoustic shape being used to control the spectral phase within each pulse. None of these above references teaches the use of the acoustic signal time dependence to produce a time scan of the global delay of successive pulses subjected to the acousto-optic interaction (e.g. the probe pulses), compared to the delay of the same pulses not subjected to the acousto-optic interaction. (e.g. the pump pulses). The person trained in the art can secondarily adapt the phase of the acoustic signal at each frequency, to impart a given time shape to e.g. the probe pulse, but this is not claimed as an innovative feature of the present invention. In fact, within the scope of the present invention, the spectral phase dependence of e.g. the probe pulse upon the acoustic signal is a drawback mentioned in the previous paragraph and discussed in the final section of this description.
More specifically, if a train of pulses is generated with a time difference ΔT between each successive pulse, splitting each pulse into a pair of two replica and making one of them interact with the acoustic signal, will yield a time delay between the pair that will vary for each pulse instance. The delay characterizing the pair corresponding to the nth pulse in the train, will be given by
τ=n·εK·ΔT+constant (4)
This accomplishes the goal of the invention to achieve delay scanning between successive pulses. For K=10−7 and ΔT=10 ns, K·ΔT=0.1 fs is significantly shorter than the 50 fs precision limit of ASOPS. Because of the compactness, it is possible to design short optical paths thus easing the requirement of stability of the optical path difference. The scan repetition rate is the inverse of the propagation time of typically 30 microseconds, i.e. of order 30 kHz.
A favorable condition for the operation of the invention will be one where the acoustic beam is collinear with the acoustic wave thus increasing the length of interaction. “Voloshinov 1992” (Voloshinov, Vitaly B. 1992. “Close to collinear acousto-optical interaction in paratellurite.” Optical Engineering 31: 2089. doi:10.1117/12.58877) and “Chang 1992” Chang, I. C. 1992. “Collinear beam acousto-optic tunable filters.” Electronics Letters 28 (13) (June 18): 1255-1256. doi:10.1049/e1:19920793 have taught how Bragg diffraction devices can be designed with collinear acoustic and optic propagation. The acousto-optic material used must be birefringent and acoustically anisotropic. The diffraction involves acoustic shear waves and the polarization of the input wave and the diffracted wave are at right angle. Examples of suitable materials for this purpose are Paratelllurite (TeO2), Calomel (Hg2Cl2) and Lithium Niobate (LiNbO3).
The invention will be better understood, by considering the following example of realization.
A Radio Frequency (RF) generator 17 is used to generate a signal containing acoustic frequencies matching the optical frequencies of the optical pulse for the purpose of acoustic diffraction. This signal takes the form of an RF pulse of duration Ta, which is fed to the transducer 18 of the acousto-optic device 16 by appropriate matching circuitry 17. The geometry of the device is chosen so that the acoustic path 19 involves the acoustic pulse first traveling to the optical input face F1, being reflected on F1, traveling to the optical output face F2, being reflected on F2, then being dissipated by some suitable arrangement. During the propagation time of duration Tp between F1 and F2, the acoustic pulse 20 can interact with the incoming successive probe pulses and produce diffracted pulses, whose delay will vary for every successive pulse, according to equation 4.
The diffracted output probe pulse is entered as a probe pulse into an experimental set up together with the input pump pulse. The example experimental set up shown as example is a THz experiment comprising a photoconductor as THz generator 21, driven by the pump pulse, a medium of THz interaction 22, a photoconductor 23 as THz detector submitted to the THz field and the probe pulse and a electronic data acquisition and averaging module 24 which receives the detector output and produces an average value as the detected signal as a function of delay. A trigger signal 25 produced by the RF generator 17 and received by the data acquisition module 24 is necessary to provide synchronization between scanning and acquisition.
If the experiment does not allow for a dead time, a scheme must be provided to duplicate the interaction zone. For instance, two different optical paths, having each a separate acoustic device, with different synchronization conditions can be used, such that one device is in the proper T2-T4 zone of operation, while the other is in dead time conditions. Alternatively, a single device with multiple transducers and multiple corresponding acoustic paths, may be manufactured. Rapidly actively switching the probe signal, from one optical path to the next is a requirement. Ideally, this should be done in a time shorter than the separation between successive optical pulses.
Hereafter are described methods to operate under conditions of non-constant
We now address the limitations introduced by the dependence on ω of
This dependence is related to the dependence of the optical index parameters upon frequency and the corresponding changes in the wavevector conservation configuration. It is well known that for many materials there exists frequency domains where the index of refraction varies little with frequency. For instance, this is the case for Paratellurite in the vicinity of 3 micron wavelength. Experiments in this wavelength region, can use the invention even for broadband pulses.
Alternatively, in other wavelength regions, such as the vicinity of 0.8 micron where many ultrafast laser sources are operated, the condition for proper operation will be that the variation of delay over the total spectrum and for the full time range Tp, be significantly smaller that the intrinsic Fourier Transform Limit of the pulse duration for the total spectrum. It will then have a negligible effect on the experiment. Since the delay variation is proportional to the bandwidth and the Fourier Transform Limit inversely proportional to the bandwidth, the condition will be satisfied for small enough bandwidth. For operation in the vicinity of 800 nm, a bandwidth of 10 nm is a typical upper limit to satisfy the condition.
For larger bandwidths, a scheme such as the one shown in
be different from each other in the wavelength range of interest. If we use proper geometries, insuring that:
1: the factor ε is of opposite sign for both devices in eq 2,
2:
are equal for both devices.
The time broadening of both devices will cancel out, while the scanning effect will be
τ=(K1−K2)·T+constant
These conditions can for instance be satisfied using Paratellurite and Calomel for a wavelength near 1.5 micrometer.
Another approach is in some cases possible. It is known in the state of the art that the bandwidth and duration of ultrafast optical pulses can be modified by non linear interaction. As an example, interaction in a rare gas is described in “Schenkel et al. 2003 (Schenkel, B., J. Biegert, U. Keller, C. Vozzi, M. Nisoli, G. Sansone, S. Stagira, S. De Silvestri, and O. Svelto. 2003. “Generation of 3.8-fs pulses from adaptive compression of a cascaded hollow fiber supercontinuum.” Optics Letters 28 (20) (October 15): 1987-1989. doi:10.1364/OL.28.001987) and shown to increase the spectral bandwidth of a given pulse from tens of nanometers to hundreds of nanometers. The corresponding Fourier Transform Limit pulse duration will be reduced from the order of 100 fs to the order of 10 fs. A device performing this function will be labeled a broadener. In the diagram of
Number | Date | Country | Kind |
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12155266.5 | Feb 2012 | EP | regional |
Filing Document | Filing Date | Country | Kind |
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PCT/EP2013/052748 | 2/12/2013 | WO | 00 |