LBO crystal is a useful nonlinear crystal for frequency conversions of ultrafast lasers. One of the main considerations for such an application is the pulse broadening induced by the group velocity (Vg) mismatch between the input pulses and the generated pulse due to the dispersion in the crystal. In order to avoid pulse broadening, the thickness of the crystal should not exceed the maximum length (Lmax) as defined by the pulsewidth divided by the inversed group velocity mismatch (IGVM = ΔVg-1). The table below lists the Lmax for second harmonic generation (SHG) and sum frequency generation (SFG) of 10 fs pulses at the wavelength range of a Ti:Sapphire laser, one of the most common ultrafast lasers,
Type I PM on XY plane |
SHG @ |
SHG @ |
SHG @ |
SHG @ 1064 nm |
SFG @ |
IGVM (ps/cm) |
1.73 |
1.20 |
0.87 |
0.43 |
4.47 |
Lmax@10 fs (µm) |
60 |
85 |
115 |
232 |
22 |
A thickness of ~ 100 µm (0.1 mm) is apparently desired for most frequency conversion processes of 10 fs pulses.
Newlight Photonics offers on this page ultrathin/thin LBO crystals 100 µm (0.1 mm) - 3.0 mm thick developed for frequency conversions of short pulses. The typical apertures are 5x5 mm and 10x10 mm.
For thicker LBO crystals (T>3 mm) for longer pulses (ns, ps), please visit Thick LBO Crystals.
Part No. | Description | Application | Thickness | Price | Availability | Add to Cart |
Structural and Physical Properties:
Crystal Structure | Orthorhombic, Space group Pna21, Point group mm2 |
Cell Parameters | a=8.4473 Å, b=7.3788 Å, c=5.1395 Å, Z=2 |
Melting Point | ~834 °C |
Mohs Hardness | 6 |
Density | 2.47 g/cm3 |
Hygroscopic Susceptibility | Low |
Thermal Expansion Coefficients | αx=10.8x10-5 /K,αy= -8.8x10-5 /K,αz=3.4x10-5 /K |
Thermal Conductivity | 3.5 W/M/K |
Linear Optical Properties:
Transparency Range | 160 - 2600 nm |
Thermo-optic Coefficient (1/°C, λ in µm) |
dnx/dT = (-3.76λ+2.30) x 10-6 dny/dT = (6.01λ-19.40) x 10-6 dnz/dT = (1.50λ-9.70) x 10-6 |
Optical Homogeneity | δn ~10-6 /cm |
Bulk Absorption Coefficient | < 100 ppm/cm at 1064 nm, < 150 ppm/cm at 532 nm |
Sellmeier Equations (λ in µm) |
nx2=2.454140+0.011249/(λ2-0.011350)-0.014591λ2-6.60x10-5λ4 ny2=2.539070+0.012711/(λ2-0.012523)-0.018540λ2+2.00x10-4λ4 nz2=2.586179+0.013099/(λ2-0.011893)-0.017968λ2-2.26x10-4λ4 |
Refractive Indices: @ 1064 nm @ 532 nm @ 266 nm |
nx = 1.5656, ny = 1.5905, nz=1.6055 nx = 1.5785, ny = 1.6065, nz=1.6212 nx = 1.5973, ny = 1.6286, nz=1.6444 |
Nonlinear Optical Properties:
SHG Phase Matchable Range | 551 ~ 2600 nm (Type I); 790-2150 nm (Type II) |
NLO Coefficients | d31=1.05 ± 0.09 pm/V d32= -0.98 ± 0.09 pm/V d33=0.05 ± 0.006 pm/V |
Effective Nonlinearity Coefficients | dooe=d32cosφ (in XY plane) deeo=d31cos2θ+d32sin2θ (in XZ plane) doeo=d31cosθ (in YZ plane) deoe=d31cos2θ+d32sin2θ (in XZ plane) |
Damage Threshold (Bulk) @ 1064 nm @ 532 nm |
9 GW/cm2 (9 ns); 19 GW/cm2 (1.3 ns) 2.2 GW/cm2 (10 ns); 45 GW/cm2 (100 ps) |
NCPM Temperature | 148 oC for SHG @ 1064 nm, 162 oC for SHG @ 1053 nm 172 oC for SHG @ 1047nm |
Damage Threshold:
LBO has the highest bulk damage threshold among all known nonlinear optical crystals and is the crystal of choice for high power second and third harmonic generations of Nd:YAG, Nd:YLF, and Nd:YVO4 lasers,
Comparison of bulk damage threshold (@1064 nm, 1.3 ns):
Crystal | Energy Fluence (J/cm2) | Power Density (GW/cm2) |
KTP | 6.0 | 4.6 |
KDP | 10.9 | 8.4 |
BBO | 12.9 | 9.9 |
LBO | 24.6 | 18.9 |
Specifications of Thin LBO Components:
Wavefront distortion: | less than λ/8 @ 633 nm |
Clear aperture: | > 90% central area |
Flatness: | λ/8 @ 633 nm |
Scratch/Dig: | 10/5 to MIL-O-13830A |
Parallelism: | better than 20 arc seconds |
Angle tolerance: | Δθ < +/-0.25o, Δφ < +/-0.25o |
Coatings:
Thin LBO crystals are typically offered uncoated.
Anti-reflective coatings (AR-coatings): Multi-layer dielectric single-band, dual-band and broad-band AR coatings on LBO surfaces are available upon request.
Mounts:
For customer convenience and protection of thin crystals, all thin crystals are pre-mounted in a standard 1" (25.4 mm ) anodized aluminum (Al) holder. Customer holders ( e.g. holders with openings to steer a probe beam past the edge of the crystal) are also available at a small cost. The mounted crystals may be further mounted in a conventional 1" mirror mount to be angle tuned for phase matching (as shown to the right, mirror mounts and posts are not included).
If you do not find the suitable products above, you may let us know your requirements or applications in the form below. Our sales or technical staff will get back to you as soon as possible.
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