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Large-mode-area Nd-doped single-transverse-mode dual-wavelength microstructure fiber laser

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Abstract

A novel design for a microstructure fiber (MSF) laser consisting of a large core and a single annulus of 5 air holes is described. The fiber design incorporates a silica core that was doped in the liquid phase with 1300 ppm Nd2O3. The light guiding losses in the structurally very simple MSF are ≈0.7 dB/m. Single transverse mode emission is demonstrated with a mode field area larger than 200 μm2. The laser simultaneously emits at two groups of wavelengths centered at 1060 nm and 1090 nm. Pumped by a cw Ti:sapphire laser, the fiber laser yields a maximum output power of 280 mW (pump power limited) at a slope efficiency of 52%. Our results indicate how the advanced possibilities of MSF’s can be used for optimized fiber laser designs.

©2005 Optical Society of America

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Figures (8)

Fig. 1.
Fig. 1. (a) Scanning electron microscope image of the end face of the penta fiber. (b) calculated near field of the fundamental HE11 mode.
Fig. 2.
Fig. 2. Experimental set up for optical pumping of the Nd3+ doped microstructure fiber.
Fig. 3.
Fig. 3. (a) Linear cut through the near field intensity distribution at threshold. (b) Cut through the near field intensity distribution about 4 times above threshold. The blue line shows a Gaussian fit indicating a 1/e2-width of w fit = 10 μm.
Fig. 4.
Fig. 4. Input/output characteristics of the penta fiber laser for linearly polarized pump. The red line and hollow symbols show the output for a bent fiber with bend radius of 1.5 cm.
Fig. 5.
Fig. 5. Angular plot of the output of the fiber laser for different orientations a polarizer behind the output of the fiber laser.
Fig. 6.(a)
Fig. 6.(a) Spectrum of the fiber laser just above threshold and (b) 4 times above threshold.
Fig. 7.
Fig. 7. Spatially dispersed output power for both emission wavelengths. The sum of both emissions does not yield the values of Fig. 4, as no correction for grating efficiencies was attempted.
Fig. 8.
Fig. 8. Temporal fluctuations on top of the cw background for the emitted wavelengths at 1060 nm and 1090 nm.
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