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Supercontinuum generation in a photonic crystal fiber with two zero-dispersion wavelengths tapered to normal dispersion at all wavelengths

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Abstract

We numerically study supercontinuum generation in photonic crystal fibers with two zero-dispersion wavelengths, weakly tapered to have normal dispersion at all wavelengths after a certain distance. We pump with 15 fs pulses with milliwatt average power and show that two distinct smooth spectral parts are generated, with improved stability due to the normal dispersion. We characterize the two spectral parts and show how the 3 dB bandwidth, the center wavelength, and the power of the two parts depend on the taper parameters and the pump power.

©2005 Optical Society of America

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Figures (3)

Fig. 1.
Fig. 1. (a) Dimensions and (b) dispersion profiles for the tapered triangular PCF with relative hole diameter d/Λ = 0.57 and pitch Λ = Λ0 = 1.0 μm (untapered) to Λ = ΛT = 0.9 μm, in steps of 0.01 μm. The dispersion is normal for all wavelengths for Λ < 0.96 μm. (c) Dispersion coefficients β 2 [10-27 s2/m] (red, 엯), β 3 [10-41 s3/m] (green, ◻), β 4 [10-55 s4/m] (black, ▵), and β 5 [10-70 s5/m] (blue, ◁), versus pitch Λ.
Fig. 2.
Fig. 2. Color coded power spectrum plot of the spectral evolution in a z T = 15 mm long taper with final pitch (a) ΛT = 0.98 μm and (b) ΛT = 0.93 μm. The white line represents the ZDWs with the dispersion being anomalous inside this curve.
Fig. 3.
Fig. 3. (a, i) Power spectrum for an untapered PCF with Λ T = 1.0 μm at z = 0 mm (dotted, red), 8 mm (dashed, green), and 15 mm (solid, blue). (b, i) Power spectrum at taper end z = z T = 15 mm for ΛT = 0.9 μm (dotted, red), 0.95 μm (dashed, green), and 1.0 μm (solid, blue). (c, i) Power spectrum for ΛT = 0.9 μm at taper end z = z T = 15 mm (dotted, red), 25 mm (dashed, green), and 50 mm (solid, blue). (d, i) Power spectrum at taper end z = z T = 15 mm for ΛT = 0.9 μm and average pump power 6 μW (dotted, red), 6 mW (dashed, green), and 12 mW (solid, blue). (a-d,ii) center wavelength, (a-d, iii) FWHM, and (a-d, iv) average power within the FWHM versus respective parameters, NIR (엯) and VIS spectral parts (◁).

Equations (1)

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Λ ( z ) = Λ T ( 1 + Λ 0 2 Λ T 2 Λ T 2 ( z z T ) 2 z T 2 ) 1 2 .
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