The present invention relates generally to diode laser sources, and particularly to high power, diode laser sources.
High power, continuous wave optical signal sources are known to be desirable. It is also known to be desirable to provide high power, continuous wave optical signal sources that exhibit high power to weight ratios and manageable thermal loads. Possible uses for such sources include solid state laser (SSL) weaponry.
A high power laser system including: a plurality of emitters each including a large area waveguide and a plurality of quantum well regions optically coupled to the large area waveguide, wherein each of the quantum well regions exhibits a low modal overlap with the large area waveguide; a collimator optically coupled to the emitters; a diffraction grating optically coupled through the collimator to the emitters; and, an output coupler optically coupled through the diffraction grating to the emitters.
A “large area waveguide”, as used herein, generally refers to a waveguide of large modal width in the transverse direction. According to an aspect of the present invention, the quantum well regions may take the form of at least one, at least partially perforated single quantum well layer. For example, where a single quantum well layer is used, it may be perforated to permit electrical contact to the side of the quantum well opposite to the top of an epitaxially grown wafer.
Understanding of the present invention will be facilitated by consideration of the following detailed description of the preferred embodiments taken in conjunction with the accompanying drawings, wherein like numerals refer to like parts and:
It is to be understood that the figures and descriptions of the present invention have been simplified to illustrate elements that are relevant for a clear understanding of the present invention, while eliminating, for purposes of clarity, many other elements found in typical optical systems and methods of making and using the same. Those of ordinary skill in the art will recognize that other elements are desirable and/or required in order to implement the present invention. However, because such elements are well known in the art, and because they do not facilitate a better understanding of the present invention, a discussion of such elements is not provided herein.
Referring now to
Generally, CAH 1100 generates and amplifies optical emissions. Collimator 1200 aligns CAH 1100 emissions at the diffraction grating 1300. Grating 1300 angularly combines spatially separated components of the CAH 1100 emissions into a single, uniform propagation direction upon the output coupler 1400. And, output coupler 1400 provides optical cavity feedback and system output.
System 1000 may be well suited for being incorporated into a compact, highly efficient Architecture for Diode High Energy Laser System (ADHELS) using direct spectral beam-combining of individual element outputs. For example, a 1040 nm Coherent High Element Power (CHEP) ADHELS according to an aspect of the present invention may include many continuous wave (cw) emitting VErtical Cavity Large Area Emitter (VECLAE) modules (CVMs) to provide high, single-spatial mode powers (such as around 1000 W per CVM), at an efficiency (ηD) of around 50% or more. As will be understood by those possessing an ordinary skill in the pertinent arts, using VECLAE based emitters allows for a substantial reduction in the number of individual beams to be combined. Accordingly, a single high power density, multi-layer dielectric grating 1300 and output coupler 1400 may provide the necessary feedback to combine 100 or more beamlets. The relative simplicity of such an optical system facilitates a high beam combining efficiency (ηBC) of around 70% or more, and a beam propagation factor (BPF) around 96% or more. Consistently, a laser performance metric (LPM) of such a system is estimated at around 33% or more.
Referring now to
By way of non-limiting example, each CVM 1110 may emit around 100 to around 1000 watts, or more, in a single fundamental spatial mode 1117 via waveguide layer 1120, responsively to activation of the ridges 1115. Each CVM 1110 uses an undoped, low-loss (α˜0.1 cm−1), thick (t˜4 to 10 μm) broad area waveguide layer 1120 having a low overlap (Γ˜0.1%) to a corresponding quantum-well gain region. The quantum-well gain region may take the form of a single-quantum well gain layer. The Multiple ridges may be defined to provide p- and n-contacts (e.g., 1160) on an epitaxial side of the CVM.
Cooler 1130 provides for a substantially uniform temperature across the CVM VECLAE ridge 1115 array, resulting in a substantially uniform refractive index there-across. As is discussed in more detail below, a micro-channel cooler may be particularly well suited for use, although other coolers may be used.
Referring still to
Referring still to
Referring now also to
Referring still to
Region 30 serves as a primary propagation and amplification region during operation. Region 30 may be composed of one or more waveguiding materials suitable for use with other materials found in the system. For example, region 30 may be composed of AlGaAs. According to an aspect of the present invention, region 30 may be undoped. According to an aspect of the present invention, region 30 may be composed of undoped AlGaAs. According to an aspect of the present invention, the cross-sectional area of region 30 may be large compared to the active layer of region 40. Region 30 is vertically, optically coupled to region 40, such that activation of region 40 serves to generate and amplify optical signals in region 30.
Region 40 may take the form of a ridge waveguide structure including an active layer sandwiched between cladding layers. For example, region 40 may include quantum well(s) in a layer 44 sandwiched between an upper cladding 42 and a lower cladding 46. By way of further example, quantum well(s) layer 44 may take the form of a single quantum well (SQW) structure or multi-quantum well (MQW) structure. Quantum well(s) layer 44 may be composed of any suitable material system, such as an InGaAs/GaAs material system, by way of non-limiting example only. Upper cladding 42 may take the form of a suitable cladding material for use with layer 44, such as p-AlGaAs. Lower cladding 46 may also take the form of a suitable cladding material for use with layer 44, such as n-AlGaAs. Contact 43 may be provided for upper cladding layer 42. Contacts 45 and 47 may be provided for lower cladding layer 46. In one configuration, contact 43 provides a p-contact for region 40, while contacts 45, 47 provide n-contacts for region 40, as will be understood by those possessing an ordinary skill in the pertinent arts.
The ridge waveguide structure may optionally be provided with passivation and/or cap layers. Further, lower cladding layer 46 of the ridge waveguiding structure may be coupled to an upper surface 30′ of region 30—thereby vertically, optically coupling region 30 to region 40.
Again, while
Referring now also to
A device featuring these characteristics is suitable for use with high current injection. Thus, device 10 it suitable for generating high power optical signals. Further, as may be seen in
Referring again to
For non-limiting purposes of further explanation only, the following example may be considered. Referring now to
A graded waveguide layer 140 may be provided over layer 130. Layer 140 may be about 0.3 μm thick. Graded waveguide layer 140 may have an aluminum content that is graded from about 0.25% to about 0.21%. The graded layer 140 may be graded substantially linearly and transversely with respect to the layers structure, with the lower percentage nearer the quantum well(s) layer. Graded waveguide layer 140 may be undoped. A GaAs barrier layer 150 may be provided over graded layer 140. Barrier layer 150 may be about 10 nm thick, for example. Barrier layer 150 may be undoped. An InGaAs quantum well layer 160 may be provided over barrier layer 150. The content and configuration of the quantum well layer may be selected to provide gain at a wavelength of interest. By way of non-limiting example, layer 160 may have an In content of about 0.2, and be about 7 nm thick, for example. Layer 160 may also be undoped. A GaAs barrier layer 170 may be provided over quantum well layer 160. Barrier layer 170 may be about 10 nm thick and be undoped as well. A graded waveguide layer 180 may be provided over barrier layer 170. Layer 180 may be about 0.6 μm thick. Layer 180 may be composed of AlGaAs, and have an Al content that is graded from about 0.2% to about 0.4%. The graded layer 180 may be graded substantially linearly and transversely with respect to the layers structure, with the lower percentage nearer the quantum well(s) layer. Layer 180 may be undoped. A p-cladding layer 190 may be provided over layer 180. Layer 190 may be about 1 μm thick. Layer 190 may be composed of AlGaAs, and have an Al content of about 0.4%. Layer 190 may be p-doped to about 2×1018 cm−3. An intermediate graded layer 200 may be provided over layer 190. Layer 200 may be about 350 nm thick. It may be composed of AlGaAs, and have an Al content that is graded from about 0.4% to about 0%. Layer 200 may be graded substantially linearly and transversely with respect to the layers structure. The graded layer may have the lower Al content nearer the quantum wells layer. Layer 200 may be p-doped to about 2×1018 cm−3. Finally, a contact layer 210 may be provided over layer 200. Layer 210 may be about 50 nm thick. Layer 210 may be composed of GaAs and be p-doped to about 1.5×1019 cm−3.
For non-limiting purposes of further explanation only, the following example may also be considered. Referring again
A graded waveguide layer 140 may be provided over layer 130. Layer 140 may be about 0.3 μm thick. Graded waveguide layer 140 may have an aluminum content that is graded from about 0.25% to about 0.21%. The graded layer 140 may be graded substantially linearly and transversely with respect to the layers structure, with the lower percentage nearer the quantum well(s) layer. Graded waveguide layer 140 may be undoped. A GaAs barrier layer 150 may be provided over graded layer 140. Barrier layer 150 may be about 10 nm thick, for example. Barrier layer 150 may be undoped. An InGaAs quantum well layer 160 may be provided over barrier layer 150. Layer 160 may have an In content of about 0.2, and be about 7 nm thick, for example. Layer 160 may also be undoped. A GaAs barrier layer 170 may be provided over quantum well layer 160. Barrier layer 170 may be about 10 nm thick and be undoped as well. A graded waveguide layer 180 may be provided over barrier layer 170. Layer 180 may be about 0.6 μm thick. Layer 180 may be composed of AlGaAs, and have an Al content that is graded from about 0.2% to about 0.4%. The graded layer 180 may be graded substantially linearly and transversely with respect to the layers structure, with the lower percentage nearer the quantum well(s) layer. Layer 180 may be undoped. A p-cladding layer 190 may be provided over layer 180. Layer 190 may be about 1 μm thick. Layer 190 may be composed of AlGaAs, and have an Al content of about 0.4%. Layer 190 may be p-doped to about 2×1018 cm−3. An intermediate graded layer 200 may be provided over layer 190. Layer 200 may be about 350 nm thick. It may be composed of AlGaAs, and have an Al content that is graded from about 0.4% to about 0%. Layer 200 may be graded substantially linearly and transversely with respect to the layers structure with the lower Al content nearer the quantum wells layer. Layer 200 may be p-doped to about 2×1018 cm−3. Finally, a contact layer 210 may be provided over layer 200. Layer 210 may be about 50 nm thick. Layer 210 may be composed of GaAs and be p-doped to about 1.5×1019 cm−3.
This latter material system may yield beam narrowing to a full width at half maximum (FWHM) value of around 5° to 6°. In summary, the differences: increase the large mode waveguide thickness from about 3 μm to about 6 μm; increase Al contents in the large mode waveguide; increase the lower clad thickness to about 1.5 μm; increase spoiler thickness to about 5 μm; and, increase Al contents in spoiler layer to around 25.1-25.2%
Regardless of the particulars, layers 100-210 may be provided and shaped using conventional processing methodologies suitable for use with the materials thereof, such as deposition and etching for example. Conventional processing technologies may be used to simultaneously form many VECLAE ridges over a common substrate and large area waveguide layer, for example. According to an aspect of the present invention, one may precisely control the Al content of layer 120 to provide for good waveguiding and amplification properties. For example, it may prove important to control the Al content to within about 1% of the target content. Layers 100, 110 are suitable for use as substrate 20 of
By way of further, non-limiting example only, it is expected that the second-discussed material layer structure will provide a FA FWHM of ˜6° with an Al content x=0.252 in the spoiler, 5° with x=0.251 and 6.5° with x=0.254. As will be understood by those possessing an ordinary skill in the pertinent arts, device performance may sharply depend on the composition of the spoiler layer. It is believed that the broadening FA FWHM with an increase of Al contents is due to the reduction of zero mode penetration in the spoiler layer. The decrease of Al content in the spoiler layer leads to fast increase of the zero mode leakage out of the waveguide. This leakage is equivalent to the losses of 1 cm−1 if Al content drops to 25.0% and yet negligible at x=0.251. The increase of Al content in the spoiler layer decreases the difference in the optical (“selection”) losses between zero and second transverse modes. These difference are 8 cm31 1 and 5 cm−1 for x=0.251 and 0.252, respectively. At x=0.254 difference in the losses and mode selection disappear.
Accordingly, beam width of a VECLAE ridge and array of ridges may vary as a function of growth technology. The accuracy of flow control preferably allows for growth of an Al0.25Ga0.75As spoiler layer with a tolerance of about +/−0.1 Al or better. In such a case, yield of VECLAE structures providing a FA FWHM between 5° and 6° and high-mode discrimination factor at a level better than about 5 cm−1 is expected to be about 50%.
Far fields of a VECLAE structure according to the first example discussed in connection with
As set forth, multiple VECLAE ridges may be monolithically integrated together. Referring now also to
Layers 620, 630, 640, 650 and 660 may be selectively patterned to define a plurality of VECLAE ridge regions or structures 10′. Layer 610 may be selectively patterned, such as by etching trenches 690 (one is shown), to provide VECLAE ridge 10′ electrical isolation. Individual mode profiles 35′ may result from activation of active regions 630—which mode profiles may collectively define a device super-mode profile.
In practice, several hundred VECLAE ridge systems 10′ may be integrally formed as emitters in a CVM. For example, 100 or 200 VECLAE ridges may be integrally formed on substrate 20 and use common guiding region 30. The outermost (i.e., peripheral) ridges may be laterally separated by around 10 cm or more, for example.
Referring again to
As will be understood by those possessing an ordinary skill in the pertinent arts, conventional single-mode diode lasers with output power ˜1 W are impractical for spectral-beam-combined scaling to 100 kW due to the large number of sources, which would in turn require a less-efficient scheme of phase-locking. The present invention addresses this shortcoming by using VECLAE sources, which have a transverse mode greater than about 4 μm, thereby enabling output power ranging from about 100 to 1000 W, while maintaining manageable heat fluxes of ˜1000 W/cm2. According to an aspect of the present invention, separate QW and waveguide regions enable the VECLAE to support greatly enlarged modal cross-sections in both transverse and lateral directions, with single fundamental lateral supermode operation. Further, the undoped planar waveguide beneath top p- and n-contacts permits modal propagation loss of an intrinsic semiconductor, i.e., αVECLAE≦0.1 cm−1 for >1 cm length. Further yet, the “dilute waveguide” has a QW modal overlap of ΓQW less than about 0.1%, thereby sharply reducing carrier-effect nonlinearity as compared to conventional structures of ˜1.5% overlap. This is demonstrated in the following Table—1, which illustrates non-limiting, exemplary parameters according to an aspect of the present invention.
By way of further explanation, conventional single-mode ridge lasers typically employ ˜3 μm waveguides, because wider ribs cause multimode “filamentation” even under short-pulse bias, due to refractive index dependence on power mediated by well-known carrier-effect nonlinearities. A “dilute” waveguide (one with small ΓQW) suppresses refractive index changes causing filamentation, thus permitting the VECLAE real-refractive-index guiding to control light propagation. For cw operation, the small αVECLAE sharply reduces thermal-effect nonlinearities mediated by absorption and bandgap-shrinkage-mediated index change.
Referring now also to
Referring still to
Referring still to
Referring now also to
By way of further, non-limiting explanation only,
In contrast,
For cw operation, the following dissipative heat sources may be introduced to take thermal nonlinearity into account: non-radiative recombination; voltage drop over hetero-junction barriers (voltage defect); resistive heating; and, bulk optical absorption. One may predict heat flow in the cross-section of the device and the heat-sink with a single point heat source using finite element simulation. Extracting the temperature increase horizontally around this point provides a kernel, which may be included in the BPM solver. Using such an analysis, performance of the VECLAE in
In other words, the problem affects ridges at the periphery of the VECLAE; such that for larger VECLAE arrays, such as arrays of 100 ridges or more (1 mm width), the temperature is more uniform for the vast majority of the stripes. Thus, heat stabilization across large VECLAE arrays does not appear to be critical. Nonetheless, even for a 10 element VECLAE, a flat phase front may be restored. For example, equalization of phase by preferentially pumping outer VECLAE ridges may be used. Pre-compensation of phase by slight variation of ridge widths across the ridge array may be used. Or, heat sinking, such as by using micro-channel coolers may be used. Optionally, preferentially cooling of the central waveguides may be used. Again though, heat non-uniformity is believed to become more mitigated with the larger of an array that is used (e.g., the more VECLAE ridges that are used).
The micro-channel approach may nonetheless provide additional benefits, such as facilitating operation over a wider temperature range. Referring again to
Referring now also to
Referring now to
Referring finally to
It will be apparent to those skilled in the art that various modifications and variations may be made in the apparatus and process of the present invention without departing from the spirit or scope of the invention. Thus, it is intended that the present invention cover the modification and variations of this invention provided they come within the scope of the appended claims and their equivalents.
This Application claims priority of U.S. patent application Ser. No. 60/575,048, filed May 27, 2004, entitled HIGH POWER DIODE LASER AMPLIFIER CONSISTING OF MULTIPLE STRIPES and 60/575,049, filed May 27, 2004, entitled LARGE OPTICAL CAVITY LASER WITH PRIMARILY UNDOPED OPTICAL CAVITY; and, is a continuation-in-part application of U.S. patent application Ser. No. 11/002,403, filed Dec. 2, 2004, entitled VERTICALLY COUPLED LARGE AREA AMPLIFIER, the entire disclosures of each of which are hereby incorporated by reference as if being set forth in their respective entireties herein.
This invention was made with Government support under Contract No. MDA-972-03-C-0043 awarded by DARPA. The Government has certain rights in this invention.
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Number | Date | Country | |
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20070036190 A1 | Feb 2007 | US |
Number | Date | Country | |
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60575048 | May 2004 | US | |
60575049 | May 2004 | US |
Number | Date | Country | |
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Parent | 11002403 | Dec 2004 | US |
Child | 11140602 | US |