• High Power Laser Science and Engineering
  • Vol. 8, Issue 3, 03000e29 (2020)
Mario Galletti1、2、3、*, Hugo Pires1, Victor Hariton1, Joana Alves1, Pedro Oliveira2, Marco Galimberti2, and Gonçalo Figueira1
Author Affiliations
  • 1GoLP/Instituto de Plasmas e Fusão Nuclear, Instituto Superior Tecnico, Universidade de Lisboa, 1049-001 Lisboa, Portugal
  • 2Central Laser Facility, Science and Technology Facilities Council, Rutherford Appleton Laboratory, Harwell Science and Innovation Campus, Didcot, UK
  • 3INFN-LNF, Via Enrico Fermi 54, 00044 Frascati, Italy
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    DOI: 10.1017/hpl.2020.27 Cite this Article Set citation alerts
    Mario Galletti, Hugo Pires, Victor Hariton, Joana Alves, Pedro Oliveira, Marco Galimberti, Gonçalo Figueira. Ultra-broadband near-infrared NOPAs based on the nonlinear crystals BiBO and YCOB[J]. High Power Laser Science and Engineering, 2020, 8(3): 03000e29 Copy Citation Text show less
    Representation of noncollinear phase-matching condition. o.a. is the crystal optic axis.
    Fig. 1. Representation of noncollinear phase-matching condition. o.a. is the crystal optic axis.
    Parametric scan for the BiBO nonlinear crystal. (a) Simulated phase-matched wavelength (λsM) dependence of the amplified spectrum. The crystal thickness is 2.5 mm and the pump intensity is ~50 GW/cm2. (b) Simulated noncollinear angular dependence of the amplified spectrum over a range ~1.6. The crystal thickness is 2.5 mm and the pump intensity is ~50 GW/cm2. The box (translucent white) highlights the region of interest where the bandwidth is maximized but the central region (~0.9 μm) is not heavily depleted.
    Fig. 2. Parametric scan for the BiBO nonlinear crystal. (a) Simulated phase-matched wavelength (λsM) dependence of the amplified spectrum. The crystal thickness is 2.5 mm and the pump intensity is ~50 GW/cm2. (b) Simulated noncollinear angular dependence of the amplified spectrum over a range ~1.6. The crystal thickness is 2.5 mm and the pump intensity is ~50 GW/cm2. The box (translucent white) highlights the region of interest where the bandwidth is maximized but the central region (~0.9 μm) is not heavily depleted.
    Simulated amplification spectrum for a 5 mm YCOB crystal pumped at 515 nm with an intensity of ~50 GW/cm2.
    Fig. 3. Simulated amplification spectrum for a 5 mm YCOB crystal pumped at 515 nm with an intensity of ~50 GW/cm2.
    Simulated noncollinear angular dependence of the BiBO amplified spectrum. Crystal thickness is 2.5 mm and the pump intensity is ~50 GW/cm2.
    Fig. 4. Simulated noncollinear angular dependence of the BiBO amplified spectrum. Crystal thickness is 2.5 mm and the pump intensity is ~50 GW/cm2.
    Schematic of the OPCPA chain used for crystal comparison. SHG, second harmonic generation; WLG, white light generation.
    Fig. 5. Schematic of the OPCPA chain used for crystal comparison. SHG, second harmonic generation; WLG, white light generation.
    Noncollinear OPA stage seed: supercontinuum generation.
    Fig. 6. Noncollinear OPA stage seed: supercontinuum generation.
    Experimental results for the YCOB NOPA stage compared to theoretical analysis. Amplified spectra for (a) 5 mm, (b) 7.5 mm and (c) 15 mm crystals. The shadowed curve is the numerically calculated amplified spectrum for the following parameters: λp = 515 nm, Ip ~50 GW/cm2, deff = 5, 7.5, 15 mm YCOB crystal thicknesses, and the signal and crystal angles are those reported in Table 2.
    Fig. 7. Experimental results for the YCOB NOPA stage compared to theoretical analysis. Amplified spectra for (a) 5 mm, (b) 7.5 mm and (c) 15 mm crystals. The shadowed curve is the numerically calculated amplified spectrum for the following parameters: λp = 515 nm, Ip ~50 GW/cm2, deff = 5, 7.5, 15 mm YCOB crystal thicknesses, and the signal and crystal angles are those reported in Table 2.
    Experimental results for the BiBO NOPA stage: amplified spectrum for a 2.5 mm crystal. Different noncollinear angles are plotted to show the influence of θNC on the spectral dip around 920 nm.
    Fig. 8. Experimental results for the BiBO NOPA stage: amplified spectrum for a 2.5 mm crystal. Different noncollinear angles are plotted to show the influence of θNC on the spectral dip around 920 nm.
    Theoretical amplified spectrum for LBO and BBO crystals in a noncollinear geometry to maximize the bandwidth.
    Fig. 9. Theoretical amplified spectrum for LBO and BBO crystals in a noncollinear geometry to maximize the bandwidth.
    ABCD
    YCOB[27]
    nx2.76970.020340.017790.00643
    ny2.87410.022130.018710.01078
    nz2.91070.022320.018870.01256
    BiBO[35]
    nx3.07400.03230.03160.01337
    ny3.16850.03730.03460.01750
    nz3.65450.05110.03710.02260
    Table 1. Sellmeier equation () coefficients for YCOB and BiBO[27,35].
    NL crystalYCOBBiBO
    Axis planexzyz
    Interactionoo-eee-o
    Central λs (nm)@850@850
    θC (°)5512
    ϕ (°)6290
    deff (pm/V)1.413.02
    θNC (°)3.752.9
    LC (mm)52.5
    LC (mm)7.5/
    LC (mm)15/
    Table 2. Parameters for the nonlinear crystals BiBO and YCOB to obtain broadband amplification. θC (°) and ϕ (°) are the crystal angles for perfect phase matching, deff (pm/V) is the nonlinear efficiency, θNC (°) is the noncollinear angle and LC (mm) is the crystal length.
    Mario Galletti, Hugo Pires, Victor Hariton, Joana Alves, Pedro Oliveira, Marco Galimberti, Gonçalo Figueira. Ultra-broadband near-infrared NOPAs based on the nonlinear crystals BiBO and YCOB[J]. High Power Laser Science and Engineering, 2020, 8(3): 03000e29
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