This page contains a Flash digital edition of a book.
research  review VCSELs retain speeds at high temperatures


A GERMAN team claims to have broken the record for data transmission from an oxide- confined 980 nm VCSEL operating at 85 °C. Their device, which is capable of 25 Gbit/s operation at that elevated temperature, is an ideal source for very short optical links in high performance computers, according to the researchers from the Technical University of Berlin and VI Systems.


“Since temperatures inside computers are as high as 85 °C, or even higher, good temperature stability is indispensable for robust, inexpensive optical links,” says Dieter Bimberg, head of the research team at the Technical University of Berlin.


Today 850 nm is the standard wavelength for short-reach optical links and local and storage-area networks, but Bimberg believes there is a strong case for 980 nm sources in all these applications.


“980 nm has the crucial advantage of transparency of the GaAs substrate, so one can easily realize bottom-emitting devices, increasing and simplifying packaging density. This is very important, for example, in the case of a large number of VCSELs for parallel optical links.”


VCSELs are fabricated via MOCVD growth


The 980 nm VCSELs produced by researchers at the Technical University of Berlin and VI Systems have bit error rates at 25 Gbit/s of less than 10-12


.


of an epistructure containing 24 pairs of Al0.12


Ga0.88 As and Al0.90 Ga0.10 As layers for the


bottom mirror, and 37 pairs for the top mirror. Sandwiched between these mirrors is an active region with five compressively strained In0.21


Ga0.79 P0.12


4.2 nm thick, which are interlaced with 6 nm thick GaAs0.88


Ga0.02 As oxide apertures positioned just


As quantum wells that are tensile strained barriers.


Selective wet etching forms two 30 nm-thick Al0.98


above the microcavity, in the field intensity nodes in the first two periods of the upper mirror.


Output from this 10 µm-diameter oxide aperture VCSEL is 4.3 mW at 20 °C, falling


to 2.6 mW at 85 °C. This relatively small reduction in power stems from an intentional red-shift detuning of 15 nm between the quantum well gain peak and the cavity resonance.


Future targets for the team are to speed the 980 nm VCSELs to 40 Gbit/s and maintain this rate at 100 °C. “We will use an optimized active region to improve the temperature stability even further, and an optimized cavity design to increase the speed beyond 25 Gbit/s,” reveals Bimberg.


A. Mutig et al. Appl. Phys Lett. 97 151101(2010)


Modeling questions Auger’s contribution to droop


CURVE fitting with the standard equation for carrier recombination in an LED shows that Auger recombination cannot, by itself, account for droop, the decline in device efficiency at high drive currents. That’s the claim of a partnership between Rensselaer Polytechnic Institute (RPI), Sandia National Laboratories and Samsung LED.


Their effort involved fabricating a range of LEDs with varying numbers of quantum wells, device areas and quantum efficiencies; measuring external quantum efficiency at a range of currents; and fitting the data with the well-known “ABC” equation for carrier recombination. This equation describes non-radiative recombination at defects by a term that is proportional to the carrier concentration, and uses quadratic and cubic variants to cater for radiative and Auger recombination, respectively.


“It is impossible for us to just use the ABC model and get a good fit,” explains team member Fred Schubert from RPI, who says that the team’s experiment indicates that there are contributions from second order, third order and fourth order terms caused by carrier leakage. “Some of the samples have significant fourth order contributions.”


Inserting additional terms in the carrier recombination model has enabled the US- Korean partnership to fit the experimental data far better. To realize a good fit at all drive currents, it began by matching the ABC model to the data at low current densities. “This part of the curve is not in question,” says Schubert. “Everybody agrees that there is Shockley-Reed-Hall recombination and radiative recombination.”


Curve fitting was then extended to higher currents, where droop plays a significant


54 www.compoundsemiconductor.net November / December 2010


role. Here they found that at current densities of 111 A/cm2


the higher-than-third


order terms contribute 13 percent or more to the total recombination rate.


Using their model, the team extracted an coefficient for third order processes of 8 x 10-29


cm6 s-1 for the LEDs, which


is comparable to values obtained by other experimentalists, but far higher than those determined by first-principle theoretical calculations for Auger recombination.


The researchers point out that this striking difference could be due to one component of carrier leakage that, like Auger recombination, is proportional to the cube of the carrier density.


Q. Dai et al. Appl. Phys Lett. 97 133507 (2010)


Page 1  |  Page 2  |  Page 3  |  Page 4  |  Page 5  |  Page 6  |  Page 7  |  Page 8  |  Page 9  |  Page 10  |  Page 11  |  Page 12  |  Page 13  |  Page 14  |  Page 15  |  Page 16  |  Page 17  |  Page 18  |  Page 19  |  Page 20  |  Page 21  |  Page 22  |  Page 23  |  Page 24  |  Page 25  |  Page 26  |  Page 27  |  Page 28  |  Page 29  |  Page 30  |  Page 31  |  Page 32  |  Page 33  |  Page 34  |  Page 35  |  Page 36  |  Page 37  |  Page 38  |  Page 39  |  Page 40  |  Page 41  |  Page 42  |  Page 43  |  Page 44  |  Page 45  |  Page 46  |  Page 47  |  Page 48  |  Page 49  |  Page 50  |  Page 51  |  Page 52  |  Page 53  |  Page 54  |  Page 55  |  Page 56  |  Page 57  |  Page 58  |  Page 59  |  Page 60  |  Page 61  |  Page 62  |  Page 63  |  Page 64  |  Page 65  |  Page 66  |  Page 67  |  Page 68  |  Page 69  |  Page 70  |  Page 71  |  Page 72  |  Page 73  |  Page 74  |  Page 75  |  Page 76  |  Page 77  |  Page 78  |  Page 79  |  Page 80  |  Page 81  |  Page 82  |  Page 83  |  Page 84  |  Page 85  |  Page 86  |  Page 87  |  Page 88  |  Page 89  |  Page 90  |  Page 91  |  Page 92  |  Page 93  |  Page 94  |  Page 95  |  Page 96  |  Page 97  |  Page 98  |  Page 99  |  Page 100  |  Page 101  |  Page 102  |  Page 103  |  Page 104  |  Page 105  |  Page 106  |  Page 107  |  Page 108  |  Page 109  |  Page 110  |  Page 111  |  Page 112  |  Page 113  |  Page 114  |  Page 115  |  Page 116  |  Page 117  |  Page 118  |  Page 119  |  Page 120  |  Page 121  |  Page 122  |  Page 123  |  Page 124  |  Page 125  |  Page 126  |  Page 127  |  Page 128  |  Page 129  |  Page 130  |  Page 131  |  Page 132  |  Page 133  |  Page 134  |  Page 135  |  Page 136  |  Page 137  |  Page 138  |  Page 139  |  Page 140  |  Page 141  |  Page 142  |  Page 143  |  Page 144  |  Page 145  |  Page 146  |  Page 147  |  Page 148  |  Page 149  |  Page 150  |  Page 151  |  Page 152  |  Page 153  |  Page 154  |  Page 155  |  Page 156  |  Page 157  |  Page 158  |  Page 159  |  Page 160  |  Page 161  |  Page 162  |  Page 163  |  Page 164  |  Page 165  |  Page 166  |  Page 167  |  Page 168  |  Page 169  |  Page 170  |  Page 171  |  Page 172  |  Page 173  |  Page 174  |  Page 175  |  Page 176  |  Page 177  |  Page 178  |  Page 179  |  Page 180  |  Page 181  |  Page 182  |  Page 183  |  Page 184  |  Page 185  |  Page 186  |  Page 187  |  Page 188  |  Page 189  |  Page 190  |  Page 191  |  Page 192  |  Page 193  |  Page 194  |  Page 195  |  Page 196  |  Page 197  |  Page 198  |  Page 199  |  Page 200  |  Page 201  |  Page 202  |  Page 203  |  Page 204  |  Page 205  |  Page 206  |  Page 207  |  Page 208  |  Page 209  |  Page 210  |  Page 211  |  Page 212  |  Page 213  |  Page 214  |  Page 215  |  Page 216  |  Page 217  |  Page 218  |  Page 219  |  Page 220  |  Page 221  |  Page 222  |  Page 223  |  Page 224  |  Page 225  |  Page 226  |  Page 227  |  Page 228  |  Page 229  |  Page 230  |  Page 231  |  Page 232  |  Page 233  |  Page 234  |  Page 235  |  Page 236  |  Page 237  |  Page 238  |  Page 239  |  Page 240  |  Page 241  |  Page 242  |  Page 243  |  Page 244  |  Page 245  |  Page 246  |  Page 247  |  Page 248  |  Page 249  |  Page 250  |  Page 251  |  Page 252  |  Page 253  |  Page 254  |  Page 255  |  Page 256