2008
DOI: 10.1063/1.2911747
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Nonlinear measurement of mid-infrared absorption in AlOx waveguides

Abstract: We report a quantitative study on the absorption of oxidized-AlAs (AlOx) integrated thin layers in the mid-infrared range (2–4μm). An AlOx absorption coefficient of 1600cm−1 is measured in a nonlinear waveguide, by investigating the phase-matching bandwidth of parametric fluorescence. Since mid-infrared optical losses of the idler mode are inferred from the corresponding signal features in the 1–2μm range, our technique takes advantage of common near-infrared sources and detectors.

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Cited by 13 publications
(14 citation statements)
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“…We can, therefore, estimate α ω to be around 1 cm −1 . These mid-IR losses are lower than those measured by Ravaro et al in a similar waveguide [20], thanks to the smaller number of AlOx layers in our sample. The low level of losses also confirms that the laser wavelength is beyond any tail of the AlOx absorption peak around 3.3 μm as observed in [20].…”
Section: Experiments and Discussioncontrasting
confidence: 66%
“…We can, therefore, estimate α ω to be around 1 cm −1 . These mid-IR losses are lower than those measured by Ravaro et al in a similar waveguide [20], thanks to the smaller number of AlOx layers in our sample. The low level of losses also confirms that the laser wavelength is beyond any tail of the AlOx absorption peak around 3.3 μm as observed in [20].…”
Section: Experiments and Discussioncontrasting
confidence: 66%
“…Around degeneracy, when the wavelength of the TM 00 pump mode is tuned from 950 to 1060 nm, the TE 00 signal wavelength ranges from 1060 to 2120 nm [22]. Accordingly, we used a set of linearly polarized CW lasers, tunable between 1280 and 1610 nm (Tunics telecom external cavity diode lasers), and around 2120 nm (Nanoplus DFB laser diode), for the Fabry-Perot fringe measurements, and between 950 and 1100 nm (Spectra-Physics Ti:sapphire laser) for the transmission measurements.…”
Section: B Experimental Resultsmentioning
confidence: 99%
“…The optical parameters of our modeling are the Bragg mode internal losses, whose value α = 35 cm −1 is extracted from the experimental results obtained by a second-harmonic generation measurement [14]; the overlap integral between the Bragg mode and the quantum well Γ = 2.45%, calculated with a commercial eigenmode solver [15]; and the facets modal reflectivity for the Bragg mode R = 0.86, calculated by Finite-Difference Time-Domain (FDTD). The radiative recombination time in the quantum well is set to τ rad = 5 × 10 −17 m 3 ·s −1 , while the Shockley-Read-Hall non-radiative recombination processes is τ SRH = 5 ns [16].…”
Section: Optoelectronic Characterizationmentioning
confidence: 99%