• High Power Laser Science and Engineering
  • Vol. 6, Issue 1, 01000e12 (2018)
Anne-Laure Calendron1、2、†, Joachim Meier1、3, Michael Hemmer1, Luis E. Zapata1, Fabian Reichert1、3, Huseyin Cankaya1、2、3, Damian N. Schimpf1, Yi Hua1、3, Guoqing Chang1、2, Aram Kalaydzhyan1, Arya Fallahi1, Nicholas H. Matlis1, and Franz X. Kärtner1、2、3、4
Author Affiliations
  • 1Center for Free-Electron Laser Science, Deutsches Elektronen Synchrotron, Notkestrasse 85, 22607 Hamburg, Germany
  • 2Centre for Ultrafast Imaging, University of Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany
  • 3Department of Physics, University of Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany
  • 4Department of Electrical Engineering & Computer Science & Research Laboratory of Electronics, MIT, Cambridge, MA 02139, USA
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    DOI: 10.1017/hpl.2018.5 Cite this Article Set citation alerts
    Anne-Laure Calendron, Joachim Meier, Michael Hemmer, Luis E. Zapata, Fabian Reichert, Huseyin Cankaya, Damian N. Schimpf, Yi Hua, Guoqing Chang, Aram Kalaydzhyan, Arya Fallahi, Nicholas H. Matlis, Franz X. Kärtner. Laser system design for table-top X-ray light source[J]. High Power Laser Science and Engineering, 2018, 6(1): 01000e12 Copy Citation Text show less
    Schematic representation of the THz-driven light source with the driving laser system. SC: single-cycle; MC: multi-cycle, ICS: inverse Compton scattering.
    Fig. 1. Schematic representation of the THz-driven light source with the driving laser system. SC: single-cycle; MC: multi-cycle, ICS: inverse Compton scattering.
    Computed amplified spectral bandwidth as a function of seed energy in a Yb:YAG thin-disk regenerative amplifier ($\unicode[STIX]{x0394}\unicode[STIX]{x03BB}_{\text{Fluo}}=5$ nm).
    Fig. 2. Computed amplified spectral bandwidth as a function of seed energy in a Yb:YAG thin-disk regenerative amplifier ($\unicode[STIX]{x0394}\unicode[STIX]{x03BB}_{\text{Fluo}}=5$ nm).
    The cryogenic composite thin disk: in our approach, a thin Yb:YAG gain sheet is diffusion bonded to a thicker index-matched cap on one face while the other face is HR coated and soldered to a backplane high-performance cooler. See text for details.
    Fig. 3. The cryogenic composite thin disk: in our approach, a thin Yb:YAG gain sheet is diffusion bonded to a thicker index-matched cap on one face while the other face is HR coated and soldered to a backplane high-performance cooler. See text for details.
    Photographs of the (a) 100 mJ and (b) 1 J Yb:YAG amplifier.
    Fig. 4. Photographs of the (a) 100 mJ and (b) 1 J Yb:YAG amplifier.
    (a) Measured output spectrum (black line) at the 10 mJ energy level along with seed spectrum (grey shaded region). (b) Measured output energy versus pump input fluence characteristics showing an output energy ${\sim}$90 mJ at full pump power.
    Fig. 5. (a) Measured output spectrum (black line) at the 10 mJ energy level along with seed spectrum (grey shaded region). (b) Measured output energy versus pump input fluence characteristics showing an output energy ${\sim}$90 mJ at full pump power.
    CAD modeling of (a) the grating compressor currently in use after a Yb:YAG high-energy amplifier and (b) the holder of the large grating in the first compressor built in our lab after the Yb:KYW regenerative amplifier[47]. (c) A newer version of the grating holder, implemented for the Yb:YLF laser system.
    Fig. 6. CAD modeling of (a) the grating compressor currently in use after a Yb:YAG high-energy amplifier and (b) the holder of the large grating in the first compressor built in our lab after the Yb:KYW regenerative amplifier[47]. (c) A newer version of the grating holder, implemented for the Yb:YLF laser system.
    Schematic of the two-stage OPA system to drive the UV generation setup. In the prism compressor located between the two OPA stages, a pulse shaper is implemented: knifes block the highest and lowest spectral components. WL: white-light generation, SHG: second harmonic generation, Comp: compressor.
    Fig. 7. Schematic of the two-stage OPA system to drive the UV generation setup. In the prism compressor located between the two OPA stages, a pulse shaper is implemented: knifes block the highest and lowest spectral components. WL: white-light generation, SHG: second harmonic generation, Comp: compressor.
    (a) Spectra of the first and second OPA stages (OPA1 and OPA2). (b) Autocorrelation trace of the second OPA stage after the prism compressor and the corresponding Gaussian fit.
    Fig. 8. (a) Spectra of the first and second OPA stages (OPA1 and OPA2). (b) Autocorrelation trace of the second OPA stage after the prism compressor and the corresponding Gaussian fit.
    (a) Simultaneous measurement of the energy at the output of the Yb:KYW regenerative amplifier, pointing measured after the regenerative amplifier, and stretched spectrum. Only a fraction of the energy of the regenerative amplifier is measured without rescaling to the total energy. An rms value for the relative energy fluctuations of 0.8% is measured. The stretched spectrum was measured with a 12.5 GHz photodiode and a 4 GHz oscilloscope. (b) Long term measurement of the Yb:KYW regenerative amplifier output.
    Fig. 9. (a) Simultaneous measurement of the energy at the output of the Yb:KYW regenerative amplifier, pointing measured after the regenerative amplifier, and stretched spectrum. Only a fraction of the energy of the regenerative amplifier is measured without rescaling to the total energy. An rms value for the relative energy fluctuations of 0.8% is measured. The stretched spectrum was measured with a 12.5 GHz photodiode and a 4 GHz oscilloscope. (b) Long term measurement of the Yb:KYW regenerative amplifier output.
    (a) Measured 1-h stability of the regenerative amplifier output at the 10 mJ energy level. The computed shot-to-shot instabilities are less than $\pm 0.75\%$ rms over 1-h. In inset, the measured spatial intensity profile at 10 mJ output energy. (b) Measured output energy stability recorded over 3.5 h at ${\sim}$75 mJ output energy. The observable slow drift is attributed to a minor drift in seed energy of the current frontend. Energy instabilities less than $\pm 0.7\%$ over 3.2 h are routinely achieved.
    Fig. 10. (a) Measured 1-h stability of the regenerative amplifier output at the 10 mJ energy level. The computed shot-to-shot instabilities are less than $\pm 0.75\%$ rms over 1-h. In inset, the measured spatial intensity profile at 10 mJ output energy. (b) Measured output energy stability recorded over 3.5 h at ${\sim}$75 mJ output energy. The observable slow drift is attributed to a minor drift in seed energy of the current frontend. Energy instabilities less than $\pm 0.7\%$ over 3.2 h are routinely achieved.
    Pulse energy measurement of the compressed OPA output over 15 h.
    Fig. 11. Pulse energy measurement of the compressed OPA output over 15 h.
    Schematic representation of the laser system based on cryo-Yb:YAG laser systems.
    Fig. 12. Schematic representation of the laser system based on cryo-Yb:YAG laser systems.
    Schematic representation of the laser system based on cryo-Yb:YLF and cryo-Yb:YAG laser systems.
    Fig. 13. Schematic representation of the laser system based on cryo-Yb:YLF and cryo-Yb:YAG laser systems.
    Schematic representation of the laser system based on RT-Yb:YAG laser systems.
    Fig. 14. Schematic representation of the laser system based on RT-Yb:YAG laser systems.
    Layout of two Yb:YAG laser chains on one optical table. The seed pulses are fiber delivered. The delay stage (dt) is followed by the Yb:KYW regenerative amplifier (REG), followed by the two CTD amplifiers with a relay imaging telescope (R.Tel) in between. After the regenerative amplifier and the first CTD amplifier, there is a pointing stabilizer. The spatial profile of the beam is measured after each stage. The alignment laser for first alignment of the 100 mJ CTD is represented.
    Fig. 15. Layout of two Yb:YAG laser chains on one optical table. The seed pulses are fiber delivered. The delay stage (dt) is followed by the Yb:KYW regenerative amplifier (REG), followed by the two CTD amplifiers with a relay imaging telescope (R.Tel) in between. After the regenerative amplifier and the first CTD amplifier, there is a pointing stabilizer. The spatial profile of the beam is measured after each stage. The alignment laser for first alignment of the 100 mJ CTD is represented.
    Photocathode laserGun lasersLINAC laserICS laser
    THz energy [mJ]130
    IR/UV energy [J]$100\times 10^{-9}$$200\times 10^{-9}$0.1–110.1–1
    Conversion efficiency needed215
    THz pulse structureSCMC
    THz duration [ps]${<}$10200
    IR/UV duration [ps]0.04–0.10.8–52000.8–5
    Central wavelength [nm]2531020–1030
    Repetition rate [Hz]100–1000
    IR beam qualityGaussianSuper-GaussianSuper-GaussianSuper-Gaussian
    Energy stability${<}$0.1%
    Pointing stability${<}$3% of DL
    Table 1. Summary of the requirements of each laser chain. The THz energy takes into account the transport losses (for single-cycle THz pulses, twice the required energy within the gun is accounted for, and ${\sim}1.5$ for multi-cycle THz pulses).
    ParameterYb:YAGYb:YAGYb:YLF
    @ RT@ CT@ CT
    Lifetime [ms]0.9512
    Absorption wavelength [nm]940938
    Emission wavelength [nm]10301029.51020
    Emission bandwidth [nm]${\sim}9$${<}$1.310
    Absorption cross-section [$10^{-20}~\text{cm}^{-2}$]0.81.61
    Emission cross-section [$10^{-20}~\text{cm}^{-2}$]2.2${\sim}10$1.8
    Saturation fluence [$\text{J}\cdot \text{cm}^{-2}$]101.620
    Thermal conductivity [$\text{W}\cdot \text{m}^{-1}\cdot \text{K}^{-1}$]124724
    Nonlinear refractive index coefficient [$10^{-16}~\text{cm}^{2}\cdot \text{W}^{-1}$]6.26.21.7
    $\text{d}n/\text{d}T$ [$10^{-6~}~\text{K}^{-1}$]7.80.91.2
    Table 2. Summary of the spectroscopic and thermo-optic properties of Yb:YAG at RT and CT and Yb:YLF at cryogenic temperature.
    Frontend Description
    output
    #1Seed for laser for multi-cycle terahertz generation (two laser lines)
    #2Ultra-short pulse seed for ICS laser-beam line
    #3Ultra-short pulse seed for gun lasers
    #4Ultra-short pulse for diagnostics such as electro-optical sampling
    Table 3. Description of the main outputs of the frontend.
    OscStretchRegenTel ICryo ITel IICryo IITransportCompr
    $f_{\text{rep}}$70 MHz70 MHz1 kHz1 kHz100 Hz(1 kHz)(1 kHz)(1 kHz)(1 kHz)
    100Hz100 Hz100 Hz100 Hz
    $\unicode[STIX]{x03BB}_{0}$1029.5 nm
    $\unicode[STIX]{x0394}\unicode[STIX]{x03BB}$5–10 nm${\sim}$2–3 nm2–2.5 nm2–2.5 nm0.5 nm0.5 nm0.3 nm0.3 nm0.3 nm
    E${\sim}$nJ${\sim}$nJ5 mJ5 mJ100 mJ100 mJ1.2 J1.2 J1 J
    $\unicode[STIX]{x1D70F}$${<}$200 fs1.6–2.4 ns1.6–2 ns0.4 ns0.4 ns0.4 ns0.4 ns0.4 ns4 ps
    B${<}$1.5${<}$0.0010.4850.0130.4890.148
    Table 4. Summary of the pulse parameters after each module of the CT Yb:YAG laser chain.
    OscStretchRegenCompr
    $f_{\text{rep}}$70 MHz70 MHz1 kHz(1 kHz)
    100 Hz100 Hz
    $\unicode[STIX]{x03BB}_{\text{0}}$1030 nm
    $\unicode[STIX]{x0394}\unicode[STIX]{x03BB}$5–10 nm${\sim}$5 nm2 nm2 nm
    E${\sim}$nJ${\sim}$nJ130 mJ100 mJ
    $\unicode[STIX]{x1D70F}$${<}$200 fs3.25 ns1.3 ns1–2 ps
    Table 5. Summary of the pulse parameters after each module of the RT-Yb:YAG laser chain.
    OscStretchRegenCryo ICompr
    $f_{\text{rep}}$70 MHz70 MHz100 Hz100 Hz100 Hz
    $\unicode[STIX]{x03BB}_{0}$1020 nm
    $\unicode[STIX]{x0394}\unicode[STIX]{x03BB}$5–10 nm${\sim}$2–3 nm2.1 nm2 nm2 nm
    E${\sim}$nJ${\sim}$nJ10 mJ100 mJ70 mJ
    $\unicode[STIX]{x1D70F}$${<}$200 fs${\sim}$0.7–1 ns0.7 ns0.66 ns750 fs
    Table 6. Summary of the pulse parameters after each module of the CT-Yb:YLF laser chain.
    DiagnosticSeederStretcherYb:KYWYb:YAGYb:YAGYb:YLFYb:YLFCompressorsUV
    regenCTD 100 mJCTD 1 JRegenbooster
    PowerX
    EnergyXXXXXXXXX
    ReprateXXXX
    Temporal profileXXXXXXXX
    SpectrumXX
    Beam profileXXXXXXX
    CurrentsXXXXX
    Diode and crystal temperaturesXXXXX
    Diode power before and after crystalXX
    TemperatureXXXXXXXX
    HumidityXXXXXXXX
    LN2 levelXXXX
    ChillerXXXXX
    VacuumXXXX
    Table 7. Diagnostics for the modules.
    Anne-Laure Calendron, Joachim Meier, Michael Hemmer, Luis E. Zapata, Fabian Reichert, Huseyin Cankaya, Damian N. Schimpf, Yi Hua, Guoqing Chang, Aram Kalaydzhyan, Arya Fallahi, Nicholas H. Matlis, Franz X. Kärtner. Laser system design for table-top X-ray light source[J]. High Power Laser Science and Engineering, 2018, 6(1): 01000e12
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