This page contains a Flash digital edition of a book.
RESEARCH REVIEW Expanding the spectral range of QCLs


Refinements to waveguides and active regions enable QCL room-temperature operation at 19 µm.


A TEAM FROM FRANCE is claiming to have set a new benchmark for the performance of quantum cascade lasers (QCLs) operating in the long infrared.


One device based on the InAs/AlSb material system delivered emission at 19 µm at temperatures up to 291 K, while a cousin at 21 µm produced lasing up to 250 K. According to the partnership between researchers at University Paris Sud and the University of Montpellier, these values represent the best performance to


explains Teisser. He and his co-workers produced two types of QCL: one design was very similar to the laser made in 2013, but employed a modified injector, plus higher doping of the active region to increase carrier dynamics; while the other had a modified active region, which replaces a diagonal intersubband transition with a vertical transition that maximises oscillator strength.


The QCL that lases via a diagonal intersubband transition (D605) has a higher threshold current density than the device that operates using a vertical transition (D686)


date for QCLs operating above 16 µm.


The team’s QCLs operate in a spectral range that corresponds to an atmospheric transparency window. This spectral range is of interest to astronomers, because it allows signals from space to reach the earth without undergoing excessive absorption.


“Since these signals are very weak, lasers can be used as local oscillators to perform heterodyne detection,” explains Raffaele Colombelli from University Paris Sud.


It is possible to construct QCLs emitting in the 19 - 24 µm range with InGaAs- based and GaAs-based devices, but lasers built with these material systems more than a decade ago did not produce encouraging results.


The pairing of InAs and AlSb is far more promising, because very low effective electron mass in the quantum wells leads to elevated optical gain. In 2013, the team at Montpellier reported QCLs emitting at around 20 µm that were based on InAs and AlSb, and device improvements are detailed in its latest


paper that is produced in collaboration with the University Paris Sud.


The latest lasers feature metal-metal waveguides. These structures produce very divergent far fields for terahertz QCLs, which are defined as emitting at 65 µm or more. However, for the French team’s lasers, undesirable diffraction effects appear to be absent. Laser structures were created in a Riber Compact 21 MBE reactor, using growth runs that could take 10 hours.


Roland Teissier from the University of Montpellier explains that one of the main difficulties associated with MBE growth is the control of the very thin AlSb layer – which has a thickness of the order of one atomic monolayer – with high interface quality. “[The second challenge is] the stability of the growth rate, in order to keep uniform layer thickness throughout the growth of the 7 µm-thick active region.”


To create the metal-metal waveguide, the researchers used wafer bonding and active region transfer. “This required the development of a specific etch stop layer and substrate removal procedure,”


76 www.compoundsemiconductor.net March 2014


These lasers have a beam divergence that is only a little larger than that of commercial QCLs operating at shorter wavelengths, such as 8 µm. “However, a larger


beam divergence can be corrected by a judicious optical system,” says Colombelli, who added that the team is also designing new laser geometries that should reduce divergence.


Compared to the QCL of 2013, the laser with higher doping had a similar threshold current, but a larger current dynamic – and the latter permitted a significantly higher operating temperature. An even higher operating temperature of 291K was possible with the QCL that featured vertical transitions in its active region. To obtain controllable side-mode emission, the team plans to use this laser design to make distributed feedback lasers capable of higher temperature operation.


“We are also planning to exploit the high optical gain of InAs in order to extend the wavelength, ideally up to 30 µm to 32 µm, where QCLs based on GaAs or InGaAs cannot operate, given the presence of photons,” says Colombelli.


D. Chastanet et. al. Appl. Phys. Lett. 104 021106 (2014)


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