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Shaper-assisted ultraviolet cross correlator Jens Möhring, 1 Tiago Buckup, 1,2 and Marcus Motzkus 1,2, * 1 Physikalische Chemie, Philipps Universität Marburg, Hans-Meerwein-Strasse, D-35043 Marburg, Germany 2 Physikalisch-Chemisches Institut, Ruprecht-Karls-Universität Heidelberg, Im Neuenheimer Feld 229, D-69120 Heidelberg, Germany *Corresponding author: [email protected]heidelberg.de Received December 9, 2009; revised March 26, 2010; accepted March 29, 2010; posted April 30, 2010 (Doc. ID 121265); published May 24, 2010 We successfully demonstrate the characterization of phase- and amplitude-modulated broadband UV pulses with a shaper-assisted cross-correlation setup. A two-dimensional pulse modulator, operated in the diffractive shaping mode, is used to generate an inherently temporally overlapped reference beam. To greatly improve the usability of this method, we combined this setup with a split-mirror UV autocorrelator based on a solar-blind photo- multiplier tube as sensitive nonlinearity. This allows sensitive characterization of the Fourier-limited pulses down to a few picojoules, as well as complex-shaped ultrashort UV pulses, typically occurring in coherent control experiments. © 2010 Optical Society of America OCIS codes: 320.0320, 320.5540, 320.7160, 040.7190. Progress in ultrafast experiments in the UV range, espe- cially the application of shaped pulse forms, requires flexible and user-friendly pulse characterization techni- ques. Ideally, characterization methods should work with low pulse energies, be independent of external refer- ences, and be capable of giving the most direct temporal representation of the pulse. To account for these criteria in the UV spectral range, two challenges have yet to be met. Day-to-day usability demands a highly manageable characterization setup; hereby, especially, the lack of temporal overlap with an external reference greatly sim- plifies the experimental effort. This requirement is, in principle, satisfied by an autocorrelator (AC); however, neither the sign of a chirp nor the temporal pulse shape can be measured directly by an AC. This issue can be solved by introduction of an external reference, e.g., in spectral interferometry techniques [1], although at the cost of a much more laborious setup. The application of a two-dimensional (2D) spatial light modulator (SLM) can address this challenge in a very efficient way. SLMs can be used as dispersionless interferometers and as out- standing tools for full management and characterization of the spectral phase [24]. Moreover, in this context, 2D SLMs offer even more potential for flexible characteriza- tion schemes unpaired by other SLMs [5]. The second important challenge is a convenient nonli- nearity to enable high-sensitivity UV pulse characteriza- tion in the nanojoule energy regime. Presently, ACs, e.g., with the Kerr effect as nonlinearity, are effective tools only for high UV pulse energy characterization [6]. Because of the lack of second-order phase-matching materials in the UV, only the additional effort of either a three-beam AC setup [7] or the introduction of an external reference [8] can increase the sensitivity of characterization. Photo- detectors showing only a two-photon response, widely used in the visible and near-IR (NIR) regions for auto- correlation measurements, avoid the problems of phase matching, handling of vacuum UV radiation, and external references. In this regard, two-photon photoelectron emis- sion from the cathode of a solar-blind photomultiplier (PMT) is an ideal candidate for UV pulse characterization. Proof-of-principle experiments already illustrated the fea- sibility of this concept, although the UV pulses were with energies in the microjoule region [9]. In order to address these two issues in the characteriza- tion of UV pulses, we combine the sensitivity of a two- photon absorption (TPA) PMT with the beam steering and phase modulation capability of a 2D SLM. This way, we are able to generate an inherently temporally over- lapped and spatially separated reference beam using a dif- fractive shaping scheme [10]: spatial splitting of such an unmodified reference and a modulated working pulse yields two separated beams and allows us to perform ex- act cross-correlation (XAC) measurements [Fig. 1]. The cross correlation is hereby executed in a split-mirror AC, offering the benefits of both techniques within the same setup. To enable the required direct 2D UV phase modulation, a special modulator technology based on a microelectro- mechanical system (MEMS) mirror arrays (MEMS Phase Former Kit, Fraunhofer IPMS) is applied [1113]. The SLM setup offers now an optimized duty cycle (333 Hz, software upgrade enables 30 μs minimum on time) and broadband pulse handling capability (sub-35 fs). This reflective modulator controls spectral phases by a pixe- lated structure (200 × 240 pixels) of individually electro- static deflectable aluminum micromirrors. The pulse shaper is operated in a reflective 4f setup, where the ima- ging component is a cylindrical mirror (f ¼ 254 mm) and a 1200 g mm -1 grating acts as the dispersive element. The microstructure of the mirror generates a relatively strong 2D diffraction pattern. However, the beams gen- erated by diffractive shaping can be easily separated from these artifacts by introduction of a spatial aperture. Altogether, the energy throughput of the complete 4f setup is around 5%10%, mainly caused by mirror and grating losses. For full control over the electric field by a phase-only modulator and to introduce the capability of spatial split- ting of the two beams, a diffractive shaping scheme is used [10]. Hereby, along the vertical axis of the SLM, where no spectral dispersion takes place, a grating is written directing the shaped beam into its first diffractive order [see Fig. 1(a) for two exemplary phase patterns]. For spectral phase modulation of the pulse, the phase of this grating is shifted. To obtain amplitude modulation, the groove depth of the grating is reduced. As a blazed grating structure is generated by a sawtooth function, energy can be directed into first or minus first order 1816 OPTICS LETTERS / Vol. 35, No. 11 / June 1, 2010 0146-9592/10/111816-03$15.00/0 © 2010 Optical Society of America

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Shaper-assisted ultraviolet cross correlatorJens Möhring,1 Tiago Buckup,1,2 and Marcus Motzkus1,2,*

1Physikalische Chemie, Philipps Universität Marburg, Hans-Meerwein-Strasse, D-35043 Marburg, Germany2Physikalisch-Chemisches Institut, Ruprecht-Karls-Universität Heidelberg, Im Neuenheimer Feld 229, D-69120 Heidelberg, Germany

*Corresponding author: [email protected]‑heidelberg.de

Received December 9, 2009; revised March 26, 2010; accepted March 29, 2010;posted April 30, 2010 (Doc. ID 121265); published May 24, 2010

We successfully demonstrate the characterization of phase- and amplitude-modulated broadband UV pulses witha shaper-assisted cross-correlation setup. A two-dimensional pulse modulator, operated in the diffractive shapingmode, is used to generate an inherently temporally overlapped reference beam. To greatly improve the usabilityof this method, we combined this setup with a split-mirror UV autocorrelator based on a solar-blind photo-multiplier tube as sensitive nonlinearity. This allows sensitive characterization of the Fourier-limited pulsesdown to a few picojoules, as well as complex-shaped ultrashort UV pulses, typically occurring in coherentcontrol experiments. © 2010 Optical Society of America

OCIS codes: 320.0320, 320.5540, 320.7160, 040.7190.

Progress in ultrafast experiments in the UV range, espe-cially the application of shaped pulse forms, requiresflexible and user-friendly pulse characterization techni-ques. Ideally, characterization methods should work withlow pulse energies, be independent of external refer-ences, and be capable of giving the most direct temporalrepresentation of the pulse. To account for these criteriain the UV spectral range, two challenges have yet tobe met.Day-to-day usability demands a highly manageable

characterization setup; hereby, especially, the lack oftemporal overlap with an external reference greatly sim-plifies the experimental effort. This requirement is, inprinciple, satisfied by an autocorrelator (AC); however,neither the sign of a chirp nor the temporal pulse shapecan be measured directly by an AC. This issue can besolved by introduction of an external reference, e.g., inspectral interferometry techniques [1], although at thecost of a much more laborious setup. The applicationof a two-dimensional (2D) spatial light modulator (SLM)can address this challenge in a very efficient way. SLMscan be used as dispersionless interferometers and as out-standing tools for full management and characterizationof the spectral phase [2–4]. Moreover, in this context, 2DSLMs offer even more potential for flexible characteriza-tion schemes unpaired by other SLMs [5].The second important challenge is a convenient nonli-

nearity to enable high-sensitivity UV pulse characteriza-tion in the nanojoule energy regime. Presently, ACs, e.g.,with theKerr effect asnonlinearity, are effective tools onlyfor high UV pulse energy characterization [6]. Because ofthe lack of second-order phase-matching materials in theUV, only the additional effort of either a three-beam ACsetup [7] or the introduction of an external reference [8]can increase the sensitivity of characterization. Photo-detectors showing only a two-photon response, widelyused in the visible and near-IR (NIR) regions for auto-correlation measurements, avoid the problems of phasematching, handling of vacuum UV radiation, and externalreferences. In this regard, two-photonphotoelectronemis-sion from the cathode of a solar-blind photomultiplier(PMT) is an ideal candidate for UV pulse characterization.Proof-of-principle experiments already illustrated the fea-sibility of this concept, although the UV pulses were withenergies in the microjoule region [9].

In order to address these two issues in the characteriza-tion of UV pulses, we combine the sensitivity of a two-photon absorption (TPA) PMT with the beam steeringand phase modulation capability of a 2D SLM. This way,we are able to generate an inherently temporally over-lapped and spatially separated reference beam using a dif-fractive shaping scheme [10]: spatial splitting of such anunmodified reference and a modulated working pulseyields two separated beams and allows us to perform ex-act cross-correlation (XAC) measurements [Fig. 1]. Thecross correlation is hereby executed in a split-mirror AC,offering the benefits of both techniques within the samesetup.

To enable the required direct 2D UV phase modulation,a special modulator technology based on a microelectro-mechanical system (MEMS) mirror arrays (MEMS PhaseFormer Kit, Fraunhofer IPMS) is applied [11–13]. TheSLM setup offers now an optimized duty cycle (333 Hz,software upgrade enables 30 μs minimum on time) andbroadband pulse handling capability (sub-35 fs). Thisreflective modulator controls spectral phases by a pixe-lated structure (200 × 240 pixels) of individually electro-static deflectable aluminum micromirrors. The pulseshaper is operated in a reflective 4f setup, where the ima-ging component is a cylindrical mirror (f ¼ 254 mm) anda 1200 g mm−1 grating acts as the dispersive element.The microstructure of the mirror generates a relativelystrong 2D diffraction pattern. However, the beams gen-erated by diffractive shaping can be easily separatedfrom these artifacts by introduction of a spatial aperture.Altogether, the energy throughput of the complete 4fsetup is around 5%–10%, mainly caused by mirror andgrating losses.

For full control over the electric field by a phase-onlymodulator and to introduce the capability of spatial split-ting of the two beams, a diffractive shaping scheme isused [10]. Hereby, along the vertical axis of the SLM,where no spectral dispersion takes place, a grating iswritten directing the shaped beam into its first diffractiveorder [see Fig. 1(a) for two exemplary phase patterns].For spectral phase modulation of the pulse, the phaseof this grating is shifted. To obtain amplitude modulation,the groove depth of the grating is reduced. As a blazedgrating structure is generated by a sawtooth function,energy can be directed into first or minus first order

1816 OPTICS LETTERS / Vol. 35, No. 11 / June 1, 2010

0146-9592/10/111816-03$15.00/0 © 2010 Optical Society of America

by mirroring the structure. The spatial period (dgrating ¼0:3 mm) of the diffractive pattern is chosen to guideshaped pulse and reference onto each half of the splitmirror in the correlator setup, respectively [as illustratedin Fig. 1(b)].In principle, the required delay between the shaped

pulse and reference can be generated in two differentways. The first method is to introduce the delay by the2D shaper using a linear phase; however, this comes withsome drawbacks: first, if the XAC delay is also generatedby the shaper, the phase modulation induced by the SLMitself is recursively characterized. A long-delay timerange can also introduce shaping artifacts into the refer-ence beam [14,15].These potential issues are solved by implementation of

a mechanical cross-correlation delay. The introduction ofsuch a delay line is straightforward if a split-mirror ACsetup is derived for this purpose. By using a split-mirrorcorrelation scheme, whereupon one mirror half ismounted on a piezo delay line equipped with capacitiveinternal position metrology (PI P-625.1CD), a precise, in-dependent calibration of the XAC time axis is guaran-teed. Further, an open-loop-driven mirror can acquire

XAC traces at a higher speed, enabling real-time charac-terization. In the present case the mirror is driven by atriangular waveform with a frequency of 0:5–2 Hz.

For nonlinearity, a solar-blind PMT (Electron Tubes,9423B) with a cesium iodide photocathode is used [13].In TPA measurements, this PMT was used down to 15 pJat the photocathode, enabling low power, femtosecondUV cross- and autocorrelation. The TPA detector was ap-plied in the spectral range between 300 to 350 nm andshould be usable up to 440 nm, limited only by the quan-tum efficiency spectrum of the PMT. The high-frequencylimit of the AC is set by the increasing one-photon ab-sorption of the CsI photocathode, which may becomea serious issue between 250–290 nm. This effect has tobe especially considered when a PMT is chosen forTPA applications [13]. To extend the TPA detectionscheme to lower wavelengths, large bandgap materialsmust be used as the photocathode, and they must bescreened for parasitic pulse broadening effects.

To illustrate typical applications where a cross-correlation measurement is required, the characteriza-tion of a double pulse and the results of a third-orderphase modulation are shown in Figs. 2 and 3, respec-tively. Double-pulse generation is achieved by periodicphase (square wave) and amplitude (j sin j waveform)modulation based on the diffractive shaping scheme. Aperfect characterization of the resulting double pulseis shown in Fig. 2(a)]. The cross correlation clearlyshows that no zero-point artifacts are present in the

Fig. 1. (Color online) Principle of UV cross correlation andthe applied shaping scheme. (a) Comparison between diffrac-tive and conventional shaping patterns written on a 2Dphase-only modulator (SLM). The left part shows a zero phase,whereas on the right side, a quadratic phase is shown. In a dif-fractive shaping scheme, a grating, perpendicular to the planeof dispersion, is written on the SLM. This diffractive shaping isalso used to obtain the beam splitting shown in (b). (b) Princi-pal illustration of the cross-correlation setup consisting of asplit-mirror AC and a two-dimensional direct UV phase modu-lator operated in the diffractive shaping mode. The elements ofthe 4f setup for the SLM are omitted for clarity.

Fig. 2. (Color online) (a) Double pulse generated by diffrac-tive shaping and characterized by shaper-assisted XAC. TheXAC shows clean double-pulse generation without visible arti-facts due to the shaping. (b) Cross correlations of doublepulses; symmetric around time zero (left) and with one pulseat time zero (right). Here XAC shows the capability of measur-ing absolute time, which is not possible in AC measurements.

June 1, 2010 / Vol. 35, No. 11 / OPTICS LETTERS 1817

double-pulse structure, a diagnosis not possible by an ACmeasurement. Furthermore, the XAC measurementenables us to differentiate between a double pulse sym-metric around time zero and a temporal structure inwhich one replica is situated at time zero [see Fig. 2(b)].Figure 3 shows the temporal structure of two third-orderphase functions with opposite signs generated by theSLM.As the applied correlator is based on a standard split-

mirror correlator device, one can switch between anautocorrelation measurement and a cross correlationin the same setup with minimum amount of adjustment.The presented measurement scheme can also be ap-

plied on 2D visible or NIR phase modulators, such as li-quid crystal on silicon shapers. Further, the presentedsimple integration of a mechanical delay in a 2D sha-per-assisted spectroscopy technique [16] could relievethe mask from the linear phase load, increasing the op-erating range of these setups.In conclusion, we have successfully shown a UV

characterization scheme based on a shaper-assisted

cross-correlation measurement with high sensitivity.Altogether, its versatility and straightforward implemen-tation make the presented setup a particularly useful toolfor the characterization of shaped broadband UV pulses,especially for complex pulse forms encountered in emer-ging coherent control applications in the UV.

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Fig. 3. (Color online) Third-order phase functions character-ized by shaper-assisted cross correlation. A cross correlation iscapable of differentiating between the signs of a third-orderphase, such as is shown here.

1818 OPTICS LETTERS / Vol. 35, No. 11 / June 1, 2010