Periodic Poling of Stoichiometric Lithium Tantalate for High-Average Power Frequency Conversion

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VG04-123 Periodic Poling of Stoichiometric Lithium Tantalate for High-Average Power Frequency Conversion Douglas J. Bamford, David J. Cook, and Scott J. Sharpe Physical Sciences Inc. Jeffrey Korn and Peter F. Moulton Q-Peak, Inc. Presented at Solid State and Diode Laser Technical Review, Albuquerque, NM June 9, 2004 Poster Presentation Physical Sciences Inc. 2110 Omega Road, Suite D San Ramon, CA 94583

PPSLT: A New Nonlinear Optical Material VG04-123-1 AFRL has supported the development of high-average power solid state lasers, often with operating wavelengths in the nearinfrared region of the spectrum PPSLT can be used to shift the output wavelengths of these laser systems to other regions of the spectrum to fill specific needs Shifting to shorter wavelengths (into the visible region of the spectrum) is useful for adaptive optics (589 nm sodium guidestar radiation); compact visible sources also have great commercial potential (projection displays, biomedical instruments, etc.) Shifting to longer wavelengths (into the mid-infrared region of the spectrum) is useful for infrared counter-measures and remote chemical sensing

Physical Properties Responsible for the Promise of PPSLT VG04-123-2 Stoichiometric lithium tantalate (SLT) is a ferroelectric material, which means the unit cell of the crystal has a permanent electric dipole moment and can be re-oriented by applying an electric field ( domain inversion ) By applying a patterned electric field, one can change a single crystal of SLT into a patterned material, periodically poled SLT (PPSLT); this patterning leads to an increase in the nonlinear optical performance of the material ( quasi-phasematching, QPM)

Physical Properties Responsible for the Promise of PPSLT (Continued) VG04-123-3 In comparison with other ferroelectric materials, SLT has these advantages: it is less susceptible to optical damage, leading to more stable output power at a given temperature and to lower operating temperatures lower electric fields are needed to achieve domain inversion, making it possible to produce thicker crystals with higher power-handling capability it has better transparency in the ultraviolet region of the spectrum, leading to the production of radiation with shorter wavelengths

How to Fabricate and Test PPSLT Devices Procure wafer of stoichiometric lithium tantalate (SLT) from an appropriate vendor VG04-123-4 Cover one surface of wafer with a patterned insulator, then apply a metal overcoat to that pattern Apply a pulse of high voltage Etch the wafer in hydrofluoric acid to reveal the domain pattern Dice the wafer into chips and polish the end faces Shine a high-power near-infrared laser into one end of the crystal and measure the visible radiation coming out the other end

Periodic Poling Apparatus: Schematic and Photograph Computer-controlled system for creating high-voltage pulses, recording current and voltage Wafer covered with patterned photoresist, Cr/Au on the plus-z face; electrical contact using electrolyte-soaked lens tissue VG04-123-5 Computer HV Control D/A HV Enable Voltage Monitor A/D Current Monitor SR560 Preamplifier G=10 In Out Glassman 30 kv Power Supply Out In In 1000x Probe 1000x Probe +z -z Wafer LiCl Au/Cr F-2495c Voltage turned off automatically when desired charge or pulse length has been reached

Scaling to Short Periods: Macroscopic View VG04-123-6 Three-inch diameter, 0.5 mm thick wafers from Deltronic Crystal Industries Pattern (revealed by etching) contains grating-like structures with periods ranging from 5.8 µm to 11.2 µm Reproducible, wafer-scale poling process

Scaling to Short Periods: Microscopic View VG04-123-7 Magnified pictures taken of the minus-z face (the face which did not contain the patterned photoresist) QPM gratings with periods 10.8 µm (left), 7.6 µm (right); useful for generating yellow and green radiation, respectively Reasonable quality for these periods over a 50-mm length

Scaling to Still-Shorter Periods: Microscopic View QPM period = 6.0 µm; useful for generating blue-green radiation VG04-123-8 More work needed to achieve (or better) this quality on wafer scale

Scaling to 2 mm Thickness: Macroscopic, Microscopic Views 50 mm diameter, 2 mm thick wafers used QPM period = 17.4 µm; useful for frequency-doubling of telecom lasers VG04-123-9 Further work needed to minimize domain merges on wafer scale, and to scale the wafer diameter from 50 mm to 76.2 mm

High Power Laser Tests: Schematic and Photograph Q-Peak Nd:YLF input laser based on multi-pass slab (MPS) technology Average power up to 6 W at 1047 nm; can be operated in continuous-wave mode, or in a variety of pulse formats VG04-123-10 L1 L2 Nd: YLF Laser λ/2-plate Polarizing Cube PPSLT Oven M1 1047 nm Power Meter 523 nm Power Meter M2 G-5076 PPSLT crystals with three different lengths (10, 20, 30 cm) mounted inside resistively-heated oven

Laser Testing: Phase-Matching Curve VG04-123-11 SHG converts 1047 nm input radiation to 523.5 nm Power at 523.5 nm monitored as a function of temperature of PPSLT crystal; QPM grating with period of 7.4 µm, length of 30 mm Relative second-harmonic power 1.0 0.8 0.6 0.4 0.2 0.0 141.2 141.4 141.6 141.8 142.0 142.2 142.4 142.6 Temperature (C) Phase-matching temperature and bandwidth agree reasonably well with predictions based on published Sellmeier equation of Bruner et al. (Optics Letters, 28, 194-196 (2003)) G-5507

Laser Testing: Conversion Efficiency in Continuous-Wave Regime SHG efficiency measured as a function of incident power at 1047 nm Measured powers corrected for Fresnel reflection losses 7% VG04-123-12 6% Conversion Efficiency 5% 4% 3% 2% y = 0.0104x 1% 0% 0 1 2 3 4 5 6 Fundamental Power (W) Linear relationship observed, as expected when the input beam is not depleted by the interaction Fitted slope gives a device efficiency of 1.0%/W G-5417

Laser Testing: Calculation of Effective Nonlinear Optical Coefficient VG04-123-13 Spatial profile of weakly-focused laser beam calculated from known beam properties using Gaussian beam propagation formulas Device efficiency given by the following equation: η dev = πn 2ω 2 1h n 2 1h 2h d ε 2 2 L eff 3 0c W 2 0 where ω 1h is the frequency of the fundamental beam, d eff is the effective nonlinear coefficient, L is the interaction length, n 1h and n 2h are indices of refraction, and W 0 is the laser spot size Calculated value of d eff is 7.4 pm/v, close to the expected value of 10.2 pm/v for an ideal QPM structure with perfect uniformity and perfect phasematching This value of d eff can be used in predictions of device performance For comparison, periodically poled lithium niobate (PPLN) devices can have d eff = 17 pm/v, but suffer from stability, power handling, and UV transparency issues

Laser Testing: Summary of Performance in Continuous-Wave Regime VG04-123-14 Quantity Fundamental wavelength Chip length, L η dev η nor = η dev /L Fundamental power Second-harmonic power Value 1047 nm 3.0 cm 1.0%/W 0.3%/W-cm 5.5 W 300 mw 300 mw of green radiation generated, with no evidence of beam distortion due to photorefraction

Laser Testing: Conversion Efficiency in Pulsed Regime Data obtained for a variety of QPM periods, pulse formats, and crystal lengths 35% VG04-123-15 Conversion efficiency 30% 25% 20% 15% 7.4mic,100ns,20KHz,20mm 7.4mic,200ns,20KHz,20mm 10% 7.4mic,50ns,10KHz,20mm 7.4mic,200ns,20KHz,20mm,set2 5% 7.3mic,100ns,20KHz,20mm 7.4mic,100ns,20KHz,10mm 0% 0 5 10 15 20 25 30 35 40 Peak Intensity (MW/cm 2 ) G-542 1 Conversion efficiency levels off at ~30% in the 20 mm long chip, lower than expected based on the cw results; small phase-matching errors in the depleted-pump regime may be responsible

Laser Testing: Summary of Best Performance in Pulsed Regime Quantity Fundamental wavelength Laser repetition rate Laser pulse length Chip length Peak conversion efficiency Fundamental peak intensity Fundamental average power Fundamental pulse energy Second-harmonic average power Second-harmonic pulse energy Value 1047 nm 20 KHz 100 ns 2.0 cm 31% 20 MW/cm 2 2.5 W 125 µj 780 mw 39 µj VG04-123-16 780 mw of green radiation generated Optical damage (surface and bulk) observed at the highest intensities; more work needed to understand its cause

MWIR Absorption Spectra of SLT, CLN VG04-123-17 Optical parametric oscillators (OPOs) based on congruent lithium niobate (CLN) are limited to wavelengths less than 4 microns because of absorption; reliable absorption data for SLT are not available in the literature FTIR spectra taken on X-cut, 1 mm thick wafers of SLT, CLN 100 90 80 CLN SLT Transmittance (%) 70 60 50 40 30 20 10 0 Path length=1 mm along X-axis Polarization parallel to Z-axis 3 4 5 6 7 8 Wavelength (microns) G-3019 SLT not significantly more transparent than CLN in the 4.0-4.5 micron wavelength range; therefore, PPSLT is not promising for extending OPOs to longer wavelengths

Summary and Conclusions VG04-123-18 Periodic poling of commercially available SLT wafers from two suppliers (Oxide Corporation and Deltronic) carried out Wafer-scale poling achieved for periods as short as 7.3 µm on 0.5 mm thick substrates Promising results obtained for periods as short as 5.8 µm on 0.5 mm thick substrates, and for periods as short as 17.4 µm on 2.0 mm thick substrates SHG of a Nd:YLF laser in PPSLT has produced 300 mw of average green power in the cw regime, with a device efficiency of 1.0%/W SHG has also produced 780 mw of average green power in the pulsed regime, with a conversion efficiency of 31% Future work will include extending short-period poling to thicker substrates, examining scaling to higher average powers