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Ž .

Optics Communications 171 1999 271–277

www.elsevier.comrlocateroptcom

Broadly tunable semiconductor lasers using asymmetric dual

quantum wells

Ching-Fuh Lin

a,b,)

, Bor-Lin Lee

a,b

, Miin-Jang Chen

a,b

a

Institute of Electro-Optical Engineering, National Taiwan UniÕersity, Taipei, Taiwan

b

Department of Electrical Engineering, National Taiwan UniÕersity, Taipei, Taiwan

Received 11 May 1999; received in revised form 2 September 1999; accepted 3 September 1999

Abstract

Semiconductor laser with extremely broadband tunability is achieved by engineering gain spectra of the laser material. Using asymmetric dual quantum wells, the gain bandwidth is broadened to about three times wider than that of conventional semiconductor lasers. With such laser material, the single-wavelength operation of the laser is tunable with 90 nm of tuning range. For dual-wavelength operation, the wavelength separation could be tuned from a few nm to about 55 nm. The two oscillation wavelengths could be almost randomly selected within a spectral range of more than 30 nm. Actively mode-locked operation is also achieved with 10–15 ps pulse widths and a tuning range of 62 nm. q 1999 Published by Elsevier Science B.V. All rights reserved.

PACS: 42.60.Fc; 42.55.Px; 78.66.Fd

Keywords: Semiconductor lasers; Broadband tunable; Single-wavelength oscillation; Dual-wavelength oscillation; Active mode-locking

1. Introduction

Semiconductor lasers have potential applications in many areas due to their compact size, low cost, integration possibility with electronics, and so on. For many applications such as optical communica-tion and spectroscopy, wide-range tunability is im-portant. Conventional semiconductor-laser materials have a gain bandwidth around 50 meV, which is the major limitation for tunability. Fortunately, it is pos-sible to engineer the gain spectra of semiconductor lasers. The methods that had been attempted include

)

Corresponding author. Tel.: q886-2-2363-5251 ext. 339; fax:

q886-2-2363-8247; e-mail: cflin@cc.ee.ntu.edu.tw

stacking twin active layers with different bandgaps

w x1 , using n s 1 and n s 2 transitions in the same w x

quantum well simultaneously 2 , and using multiple

w x

quantum wells of different widths 3 . The first method needs a good control on the material gradient during growth, which is not as easy as the thickness control. In the second method the wide spectrum is only obtained for certain device length. The conve-nience of thickness control for gain-spectrum engi-neering has thus interested several groups on such

w x

exploration recently 4–7 . In this work, we report

Ž .

the use of asymmetric dual quantum wells ADQWs to significantly broaden the gain bandwidth. Broad-band tunability is achieved for single-wavelength, dual-wavelength operations and active mode-locking. 0030-4018r99r$ - see front matter q 1999 Published by Elsevier Science B.V. All rights reserved.

Ž .

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tional semiconductor laser materials. Fig. 1 shows the calculated transition energy vs. well width for GaAs QW bounded by Al0.18Ga0.82As barrier. This figure shows that the n s 1 transition energies in 40

˚

˚

A and 75 A well separate for about 50 meV. Also,

˚

the n s 2 transition energy in 75 A well separates

˚

from the n s 1 transition energy in 40 A well for 75 meV. The experiments using slight different spacing

˚

of the n s 2 transition energy in 75 A and the n s 1

˚

transition energy in 40 A had shown no significant influences. Thus, the overall gain bandwidth could be almost three times wider than conventional ones.

˚

The width of the Al0.18Ga0.82As barrier is 150 A, which is wide enough to ensure no coupling between the two QWs, so the transitions occur at the desired energy levels.

Two types of SLDs had been fabricated on the MOCVD grown substrate with the ADQWs, one

w x

with tilted ridge waveguide 8 and the other with

w x

bent ridge waveguide 9 . The fabricated SLDs show that their emission spectra are 2 ; 3 times wider than conventional SLDs fabricated on substrate with two

w x

QWs of the same width 3 . The tilted-strip SLDs

Fig. 1. Calculated transition energy vs. well width for GaAs quantum well bounded by Al0.18Ga0.82As barrier.

3. Tuning of single-wavelength oscillation

A ring-cavity configuration schematically shown in Fig. 2 was set up for single-wavelength operation. Two mirrors and one grating were used in the setup. Because the beam emitted from the tilted ridge waveguide has a crescent shape, the triangular ring cavity shown in Fig. 2 has less coupling loss than the usual four-mirror zigzag ring cavity. The ring cavity provides two advantages over the linear cavity. First, because the cross section of the active region is very small and both facets of the SLD have a very small retro-reflectivity, the alignment of the ring cavity is easier than a linear cavity. Second, in the conven-tional linear cavity, the output beam is accompanied with significant amplified spontaneous emission

ŽASE noise. However, in the ring-cavity configura-. Ž .

tion, one arm of the output beams, beam a , has very little ASE noise because the ASE noise is first spatially dispersed by the grating and then filtered

Ž . Ž .

out by the mirror mount M1. Fig. 3 a and Fig. 3 b

Ž .

show the measured spectra emitted from beams a

Ž .

and b , respectively. The ASE suppression ratio in

Ž .

Fig. 3 a is significantly improved to 40 dB. This measurement is limited by experimental instruments. SLDs of different lengths had been used in the cavity. Tuning of wavelength was achieved by rotat-ing the gratrotat-ing angle. The tunrotat-ing characteristics are

Ž . Ž .

shown in Fig. 4 a and Fig. 4 b . The tuning ranges are 90, 70, and 48 nm for the 400-, 700-, and 1000-mm devices. In the experiment, the operation current was limited to below 400 mA. Further in-crease of injection current should inin-crease the tuning range, but not much, because the threshold current increases significantly at the two sides of the tuning

Ž .

curve. The ASE suppression ratio of beam a was measured to be 40 dB for the entire tuning range.

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Fig. 2. The experimental setup of ring cavity.

The wide tuning range of using the 400-mm SLD

˚

indicates that the n s 1 and n s 2 transitions in 75 A

Ž . Ž .

Fig. 3. The spectra measured from beams a and b , respectively, in Fig. 2.

Ž . Ž .

Fig. 4. a Threshold current vs. tuning wavelength; and b tuning range vs. device length.

˚

well and n s 1 transition in 40 A well could all contribute to the laser oscillation. The length depen-dence of tuning is caused by two reasons. First, as

Ž .

shown in Fig. 4 a , because the minimum threshold current for using SLDs of different lengths is about the same, the threshold current density for the shorter device is higher, indicating that the shorter SLD is pumped harder. Consequently, band-filling effect leads to a broader spectrum. Second, the exponential growth of amplified spontaneous emission could ef-fectively reduce the emission spectral width of the long SLD, leading to a narrower tuning range. Both factors cause the tuning range to approximately lin-early decrease with the device length, as shown in

Ž .

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SLD was also used in this experiment for the reason of reduced Fabry–Perot resonance to enhance the spectral control of the external cavity. A

reflection-w x

type grating telescope 10 was used on one side of the SLD. The grating has 1200 linesrmm. V-shaped double slits were inserted in front of the mirror for the selection of the oscillation wavelengths. An out-put coupler with RrT s 70r30 was used on the other side of the SLD to form the laser cavity. With

Ž .

the setup, the spectral spacing Dl of the two

Ž .

wavelengths is related to the slit spacing D l simply

Ž . Ž .

by the formula: D l in nm s 3.83 D l in mm . Therefore, moving the V-shaped slits vertically could change the spectral spacing of the two wavelengths. The experiment showed that simultaneous oscillation at two wavelengths could occur with their spacing as far as 55.7 nm. Within this spacing, the two modes could be adjusted to have equal powers. Beyond 55.7 nm, two-mode oscillation is still possible, but the mode of long wavelength always has a larger power. Fig. 6 shows the measured spectra at two spacings: 5 nm and 55.7 nm.

For two modes with a fixed spectral spacing, they could also be simultaneously tuned by moving the

Fig. 5. Schematic of the experimental setup for dual-wavelength operation.

Fig. 6. Measured spectra of two wavelengths at two spacings: 5 nm and 55.7 nm.

V-shaped slits horizontally. If the two modes are spectrally separated as far as 39 nm, the tuning range is 7 nm. For a narrow spectral spacing like 5.5 nm, the tuning range increases to 34.7 nm. For an even narrower spectral spacing, the tuning range should

w x

increase further 11 . Fig. 7 shows the tuning spectra of two wavelengths at fixed spacing. On the other hand, the tuning can also be achieved with one wavelength being varied, while the other is fixed. This is accomplished by using a new type of V-shaped slits. The new type has one vertical side of the V shape. Vertically moving such V-shaped slits

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Fig. 8. The tuning spectra for one wavelength varied and the other

Ž . Ž .

fixed at: a 800 nm; and b 830 nm.

could cause one wavelength fixed and the other

Ž . Ž .

varied. Fig. 8 a and Fig. 8 b show the tuning spectra for one wavelength fixed at 800 nm and 830 nm, respectively. The tuning of the varied wave-length can be over 30 nm and the fixed wavewave-length can be selected between 792 nm and 835 nm. Those experiments indicate that the two oscillation wave-lengths can be almost randomly selected within a spectral range over 30 nm.

Because of the wide tuning range, the two oscilla-tion modes can be contributed either from one QW or two QWs. We had observed in the experiment that the two modes had a strong competition if they were contributed from the same well. In contrast, the two modes had a relatively weak competition if they were contributed from different wells. The reason is because the intraband relaxation in the same well is much faster than the carrier transport between two wells. Consequently, dual-wavelength oscillation is easier to maintain when the two modes are con-tributed from different wells, respectively. From this

point of view, using MQWs of different width for multi-wavelength oscillation should be better than using various quantized levels in the same well.

5. Tuning of active mode-locking

In the mode-locking experiment, the ring cavity similar to the one shown in Fig. 2 was used for the advantages mentioned previously. In addition, the pulse train can be more easily synchronized with the RF modulation signal travelling in the ring cavity

w x

than in the linear cavity 12 . Fig. 9 shows the measured laser output power vs. the modulation frequency for RF power fixed at 16 dBm and DC bias at threshold. This frequency response should have already included the effects of the external electronics parasitic and intrinsic carrier transport in SLD. As shown in the figure, the output power is very strong when the laser is modulated at the multiple of the round-trip frequency. In the active mode-locking, modulation at a higher frequency could usually result in shorter mode-locked pulse

w x

widths 13 . However, Fig. 9 shows that the response of the laser over the third harmonic is reduced to less than half of that at the round-trip frequency. There-fore, the third harmonic, ; 886 MHz, of the cavity round-trip frequency was used for mode-locking ex-periment.

The grating was adjusted to have the laser oscil-lating near 830 nm. Without applying RF signal,

Ž .

Fig. 9. The measured average power of the laser output a in Fig. 2 vs. RF modulation frequency.

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the other hand, the measured autocorrelation shape and width are not strongly affected by the DC biased level as long as it is below the threshold and above 0.6 I . The coincidence of modulation frequencyth with the cavity round-trip characteristics suggests that the short pulses should be generated by mode-locking mechanism instead of gain-switching.

The autocorrelation curves show no secondary pulses resulting from the residual reflectivity of

w x

laser-diode facets 13 because the tilted waveguide effectively reduce the retroreflectivity at both facets

w x

of the SLD 8 . This autocorrelation trace can be well fitted by the single-sided exponential shape, as shown by the dotted line in Fig. 10. The mode-locking condition is similar for the tuning range from 810 nm to 857 nm. Fig. 11 shows the lasing threshold, DC bias, and RF modulation frequency vs. tuning wavelength in the experiment. The lasing threshold for 810–857 nm is approximately between 45 mA and 70 mA. The RF modulation depth was

main-Fig. 10. The autocorrelation trace of the mode-locked pulses at

Ž

different modulation frequency. The autocorrelation widths are also indicated and dotted lines are fitted by single-sided

exponen-.

tial functions .

Fig. 11. The threshold current, DC biased current, and RF modula-tion frequency vs. tuning wavelength for the actively mode-locked lasers in the experiment.

tained at ; 0.5 Ith for the entire tuning range. For the wavelength below 810 nm, the lasing threshold increases to above 70 mA. The RF modulation depth at 0.5 Ith then causes an extra gain for the tail of the pulses, leading to significant broadening of the pulses. The extra gain could be reduced by lowering the DC biased level, so the well-behaved autocorrela-tion trace was retained by decreasing the DC bias.

Fig. 12 shows the mode-locked pulse width and spectral width vs. the tuning wavelength. The pulse width is calculated by assuming the single-sided exponential pulse shape. The pulse width is 10–15 ps and in general decreases with decreasing laser wavelength. One reason for the tendency may be due

Fig. 12. The mode-locked pulse width and spectral width vs. the tuning wavelength.

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to the increasing differential gain with decreasing

w x

wavelength 14 . The corresponding spectrum from

Ž .

beam a contains almost no ASE noise, as explained in Section 3. The FWHM of the spectrum is between

˚

˚

2 A and 4.5 A. The time-bandwidth products of the mode-locked pulses are mostly between one to two. Assuming single-sided exponential pulse shape, the chirped pulses could be possibly compressed to 1–2

w x

ps. Different from the past observation, 15 there is no evidence of decreased chirp with decreasing las-ing wavelength. The reason is probably due to the broad gain bandwidth provided by the asymmetric dual quantum wells.

Although the tuning is demonstrated only for 795–857 nm, a wider tuning range for such actively mode-locked pulses could be expected with proper adjustment of DC bias and RF modulation depth. The wide tuning range is possible due to the broad gain bandwidth provided by the asymmetric dual quantum-well structure. On the other hand, the grat-ing had been replaced with a mirror to see if a broad spectrum could be actively mode-locked to generate extremely short-pulses. The spectral width was then

˚

significantly broadened to about 50 A when the modulation signal was applied. However, no matter what conditions could be possibly adjusted, the auot-correlation trace shows no well-behaved shapes. The reason is probably because the RF modulation is not strong enough to mode-lock such a broad spectrum.

6. Conclusion

In conclusion, the gain bandwidth of semiconduc-tor lasers could be broadened to about three times wider than that of conventional semiconductor lasers using ADQWs. Extremely broadband tunability is therefore possible with such laser material. 90 nm of tuning range is achieved for single-wavelength oper-ation. For dual-wavelength operation, the spectral spacing of the two modes could be tuned from a few

nm to about 55 nm. Active mode-locking of semi-conductor lasers with ADQWs is also possible to generate pulses of 10–15 ps with a tuning range of 62 nm.

Acknowledgements

This work is supported in part by National Sci-ence Council, Taipei, Taiwan, ROC, under the con-tract No. NSC88-2215-E-002-021 and No. NSC2112-M-002-038.

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數據

Fig. 1. Calculated transition energy vs. well width for GaAs quantum well bounded by Al 0.18 Ga 0.82 As barrier.
Fig. 3. The spectra measured from beams a and b , respectively, in Fig. 2.
Fig. 6 shows the measured spectra at two spacings: 5 nm and 55.7 nm.
Fig. 8. The tuning spectra for one wavelength varied and the other
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