The present invention relates to solar cells and more particularly, relates to a solar cell utilizing a graded buffer.
There is considerable interest in the design and fabrication of tandem multi-junction solar cells for high efficiency photovoltaics for space-based and terrestrial applications. Multi-junction solar cells comprise two or more p-n junction subcells with band gaps engineered to enable efficient collection of the broad solar spectrum. The subcell band gaps are controlled such that as the incident solar spectrum passes down through the multi-junction solar cell it passes through subcells of sequentially decreasing band gap energy. Thus, the efficiency losses associated with single junction cells—inefficient collection of high-energy photons and failure to collect low-energy photons—are minimized.
The present invention is a device, system, and method for multi-junction solar cell structure utilizing a graded buffer. An exemplary silicon germanium solar cell structure can have a substrate with a graded buffer layer grown on the substrate. A base layer and emitter layer for a first solar subcell is grown in or on the graded buffer layer. A first junction can be provided between the emitter layer and the base layer. A second solar subcell can be grown on top of the first solar subcell.
The present invention is not intended to be limited to a system or method that must satisfy one or more of any stated objects or features of the invention. It is also important to note that the present invention is not limited to the exemplary or primary embodiments described herein. Modifications and substitutions by one of ordinary skill in the art are considered to be within the scope of the present invention, which is not to be limited except by the following claims.
These and other features and advantages of the present invention will be better understood by reading the following detailed description, taken together with the drawings wherein:
a-d) are profile diagrams of a device being constructed in accordance with an exemplary multi-junction cell embodiment of the invention.
a-h) are profile diagrams of a device being constructed in accordance with an exemplary multi-junction cell on a transparent substrate embodiment of the invention.
Solar modules using 16% efficient solar cells dominate the present photovoltaic market, but even at today's very low price per watt, they cannot be profitably installed without significant subsidies, in most parts of the world. This is in part because the non-module cost or balance of systems (BOS) cost dominates total installation cost. Most of these BOS costs are area dependent and scale linearly with area. Therefore, higher efficiency solar cells reduce BOS costs, by reducing the amount of solar installation area for a given power output. For example, for residential-based rooftop installations, a doubling of efficiency can be estimated to lead to about a 20-30% decrease in total system installation cost per watt.
According to one embodiment of the invention, a tandem cell on silicon has the potential for at least 33% cell efficiency, or about double that of today's market-dominating low-cost silicon-based solar cells. Embodiments may make use of the SiGe graded buffer to allow the growth of low-dislocation density SiGe with Ge content of, for example, about 80% on a silicon wafer. The top subcell can be GaAsP lattice matched to the SiGe below it. The GaAsP can have a bandgap of about 1.6 eV. The bottom subcell can be SiGe, above the SiGe graded buffer. The SiGe of the bottom subcell can have a bandgap of about 0.9 eV.
Embodiments offer additional benefits for high efficiency multi-junction solar cells based on III-V epitaxial subcells grown on silicon germanium subcells grown on graded buffers of silicon germanium on silicon substrates. Currently, the monocrystalline germanium substrate used for almost all commercial multi-junction III-V solar cells accounts for the majority of the cost of such solar cells, even though only the top portion of this substrate contributes to solar cell operation.
Referring to
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The graded buffer layer 104 can be hetero-epitaxially grown on the substrate 102. A CVD reactor such as an ASM Epsilon 2000 can be used to produce the relaxed graded buffer layer on substrate 102; alternately, a batch epitaxy reactor can be used. The various doping levels described in the graded buffer structure and SiGe subcell layers can be incorporated in-situ during epitaxial growth, by means well known in the art. The composition of the graded buffer layer 104 can be initiated with a 0% or relatively low germanium composition. A germanium content, x, of the Si1-xGex layer is controlled by the relative concentration of the silicon and germanium precursors. By increasing the germanium content gradually, the strain due to lattice mismatch between silicon and germanium is gradually relieved, thereby minimizing threading dislocation density in the deposited relaxed SiGe layer. Typically, the germanium content of the graded Si1-xGex layer is increased at a rate of about 10%-25% germanium per micron; however, embodiments need not be limited to that range. A final graded Si1-xGex layer can comprise a 50-90% germanium composition, or for example 70-85% germanium composition. However, embodiments are not limited to that composition and various grading layers may be incorporated or may form a portion of the SiGe subcell 106. An exemplary process of growing the graded buffer layer 104 is described in greater detail and incorporated herein in U.S. Pat. No. 5,221,413 of Jun. 22, 1993 entitled: “Method for making low defect density semiconductor heterostructure and devices made thereby”. Graded buffer layer 104 may be doped n-type, with for example arsenic or phosphorous, for example in the range 1×1016 cm−3 to 1×1019 cm−3.
The SiGe subcell 106 can include a back surface field layer interfacing graded buffer layer 104, with Ge composition anywhere between 50-90%, approximately matched to the terminal germanium composition of graded buffer layer 104. The back surface field layer can have a thickness of e.g. 50-500 nm with n type doping levels of about 1e17-1e19 cm−3, or for example 3e17-3e18 cm−3. In an alternative embodiment, the back surface field layer may be tensile, with a germanium content lower than that of the terminal composition of graded buffer layer 104, for example about 25% lower Ge; in this case, the thickness of the back surface field layer may be thinner, for example about 20-100 nm. Due to the energy band offsets introduced by tension, a tensile back surface field layer may be more effective than a lattice-matched one. SiGe subcell 106 can include a base layer, with a Ge composition anywhere between 50-90%, approximately matched to the terminal germanium composition of graded buffer layer 104. The base layer can have a thickness of between 0.5-5.0 um with n type doping levels of about 1e15-5e17 cm−3, or for example levels of about 5e15-5e16 cm−3. If the back surface field layer is included, it can be below and in contact with the base layer.
An emitter layer can be grown on top of the base layer having a similar germanium composition or matched to the surface of the base layer. The emitter layer can have a p type doping level of 5e17-5e19 cm−3, or for example levels of about 1e18-5e18 cm−3.
The emitter layer can have a thickness of about 100-2000 nm, or for example about 200-500 nm. An exemplary process of growing a SiGe solar cell is described in greater detail and incorporated herein in U.S patent application publication 2011/0120538 published May 26, 2011 entitled: “Silicon Germanium Solar Cell”.
The tunnel junction 108 can be provided between the SiGe subcell 106 and GaAsP subcell 110. The tunnel junction 108 can comprise a bottom tunnel junction portion comprised of SiGe interfacing SiGe subcell 106, with p-type doping levels of about 7e18-1e20 cm−3 with a thickness of 5-20 nm. The percent of germanium can be approximately matched to the terminal germanium composition of graded buffer 104, or it can be richer in germanium (e.g up to about 20% higher in Ge content, and may be pure Ge) for narrower bandgap to promote more effective tunneling behavior. A top SiGe tunnel junction portion can be provided having n type doping levels of about 7e18-1e20 cm−3 with a thickness of 5-20 nm. Again, the percent of germanium can be approximately matched to the terminal germanium composition of graded buffer 104, or it can be richer in germanium (e.g up to about 20% higher in Ge content, and may be pure Ge) for narrower bandgap to promote more effective tunneling behavior. The tunneling interface is between the p-type bottom tunnel junction portion and the n-type top tunnel junction portion.
Transition layers 109 can be provided between the tunnel junction layers 108 and the GaAsP subcell 110. The transition layers may include a bottom transition layer interfacing tunnel junction 108 and comprising for example pure germanium, having n type doping levels of about 1e18-1e20 cm−3, or for example levels of about 5e18-5e19 cm−3, with a thickness of 5-30 nm. The transition layers may also include a top transition layer interfacing GaAsP subcell 110 comprised of a III-V semiconductor approximately lattice matched to the terminal portion of graded buffer 104, for example an InGaP layer with a thickness of about 10-100 nm and n-type doping of 1e18-1e19 cm−3 can be provided. The purpose of the top transition layer is to allow for the initiation of quality III-V semiconductor growth on top of the group IV semiconductor layers below. This and subsequently described III-V layers can be grown in an MOCVD (Metal Oxide Chemical Vapor Deposition) system such as a Veeco TurboDisc As/P (Arsenide/Phosphide) MOCVD System, by methods well known in the art.
The GaAsP subcell 110 can include a back surface field layer which may have a lattice constant approximately matching the terminal composition of graded buffer 104, and thickness of between e,g. 50-200 nm, with n type doping levels of about 1e17-1e19 cm−3, or for example between 3e17-3e18 cm−3. This layer may be comprised of GaAsP, or of a wider-bandgap semiconductor layer such as InGaP. GaAsP subcell 110 can include a GaAsP base layer above the back surface field layer, which may have lattice constant approximately matching the terminal composition of graded buffer 104, and a thickness of between 0.2-2.0 um, with n type doping levels of about 1e16-1e18 cm−3, or for example about 1e17-2e17 cm−3. Alternately, the GaAsP base layer can be slightly tensile, with for example about 0.05-0.15% strain. A GaAsP emitter layer may be grown above the GaAsP base layer with p type doping of e.g. 1e17-1e19 cm−3, or about 1e18-3e18 cm−3, and with a lattice constant similar to the GaAsP base layer. The GaAsP emitter layer can have a thickness of about 50-200 nm, or about 100 nm. Additional layers can include a window layer of AlInP or InGaP, for example with a lattice constant similar to the underlying GaAsP base and emitter layers, and thickness of between 10-50 nm, with p type doping levels of for example about 2e17-2e18 cm−3. Alternately, the window layers may be somewhat tensile, with up to e.g. 2% tensile strain, allowing a wider bandgap for less ultraviolet absorption. A GaAsP or GaAs contact layer can also be provided with a lattice constant similar to the terminal portion of graded buffer 104, and a thickness of between 100-500 nm with p type doping levels of about 5e18-1e20 cm−3. The contact layer may be removed via wet etching after subsequent top contact grid formation, and thus only remain under the top contact grid in the final structure, an approach which is well known in the art of making III-V-based multi-junction solar cells. An exemplary process of creating a GaAsP cell is known in the art. For example, see Vernon et al., “Development of high-efficiency GaAsP solar cells on compositionally graded buffer layers”, page 108-112, IEEE Photovoltaic Specialists Conference, 19th, New Orleans, La., May 4-8, 1987, Proceedings.
Top contacts 112 can be provided on the exposed surface of the GaAsP subcell 110. The top contacts 112 can be provided by known methods in the art. For example, a grid structure of CrAu with a thickness of e.g. 1 um-5 um may be provided. Anti-reflection coating (ARC) of silicon nitride with a thickness of about 10-500 nm can also be provided to improve the solar cell efficiency. Methods and materials for providing top contacts and top ARC for III-V-based multi-junction solar cells is well known in the art.
The bottom contact surface of the substrate 102 can be textured with KOH (potassium hydroxide) or TMAH, as is known in the art, to provide a pyramidally textured surface. Such a surface will cause light redirection upon reflection from the rear surface. Re-direction of the light away from a direction substantially normal to the top solar cell surface promotes total internal reflection. A thin (e.g. 10-1000 nm, or for example about 100 nm) dielectric layer of e.g. SiNx or SiO2 can be deposited on the bottom of substrate 102, after optional texturing takes place. This layer, not shown, can be between layers 102 and 114 in
Referring to
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A porous silicon layer 402a may be used to construct a base portion of a solar cell 400. The donor substrate 402 may be p-type and have resistivity below about 1 ohm-cm. Dual porous layers 402a may be formed on the surface of the donor substrate 402. The top porous layer may have a lower porosity, to serve as a template for subsequent epitaxial growth. The bottom porous layer may have a higher porosity, to allow subsequent splitting. An exemplary approach to creating a splitting plane is known in the art and is described in, for example, Yonehara & Sakaguchi, JSAP Int. July 2001, No. 4, pp. 10-16. The porous layers 402a may also be stabilized via brief thermal oxidation and may also be sealed via anneal under H2 as described in Yonehara & Sakaguchi.
Details of an exemplary process for forming porous Si splitting layers are as follow. A p-type (100)-oriented monocrystalline Si donor substrate 402, with resistivity between 0.01-0.02 ohm-cm, may be immersed in a solution composed of one part hydrofluoric acid, one part water, and one part iso-propyl alcohol. The substrate holder is electrically insulating, forcing electrical current to pass through the substrate and not around the wafer periphery. The donor substrate 402 is in series and in-line with two silicon electrodes, one facing the front of the wafer and the other facing the back. The electrodes are equal to or greater than the diameter of the substrate and are separated from the substrate by a distance of at least 10% of the diameter of the substrate. Two different voltages are applied between the electrodes, resulting in the formation of two different porous silicon layers 402a at different current densities. The first layer, which may be etched at a current density of 2-10 mA/cm2 to a depth of 0.5-2 microns (etch time approximately 0.5-5 minutes), is low porosity (approximately 25%). The second layer, buried under the first layer and which may be etched at a current density of 40-200 mA/cm2 to a depth of 0.25-2 microns (etch time approximately 2-30 seconds), is higher porosity. The second layer defines a cleave plane after subsequent cleaning, epitaxy, and bonding, described in further detail below. After etching, the wafers may be immersed in a mixture of sulfuric acid and hydrogen peroxide, self-heating to approximately 80-140° C., for 10 minutes. Other standard semiconductor cleaning solutions, such as SC-1, SC-2, hydrofluoric acid, hydrochloric acid, or iso-propyl alcohol, may also be used. Wafers may then be loaded into the silicon growth system.
The graded buffer layer 404 can be hetero-epitaxially grown on the porous silicon layer 402a as is described in greater detail later herein. A CVD reactor such as an ASM Epsilon 2000 can be used to produce the relaxed grade buffer layer on porous layer 402a; the various doping levels described in the graded buffer structure and SiGe subcell layers can be incorporated in-situ during epitaxial growth, by means well known in the art. The composition of the graded buffer layer 404 can be initiated with a 0% or relatively low germanium composition. A germanium content, x, of the Si1-xGex layer is controlled by the relative concentration of the silicon and germanium precursors. By increasing the germanium content gradually, the strain due to lattice mismatch between silicon and germanium is gradually relieved, thereby minimizing threading dislocation density in the deposited relaxed SiGe layer. Typically, the germanium content of the graded Si1-xGex layer is increased at a rate of about 10%-25% Ge per micron; however, embodiments need not be limited to that range. A final graded Si1-xGex layer can comprise a 50-90% germanium composition or for example 70-85% germanium composition. However, embodiments are not limited to that composition and various grading layers may be incorporated or may form a portion of the SiGe subcell 406. Alternately, a batch epitaxy reactor can be used in place of the CVD reactor.
The SiGe subcell 406 can include a back surface field layer interfacing graded buffer layer 404, with Ge composition anywhere between 50-90%, approximately matched to the terminal germanium composition of graded buffer layer 404. The back surface field layer can have a thickness of e.g. 50-500 nm with p type doping levels of about 1e17-1e19 cm−3, or for example 3e17-3e18 cm−3. In an alternative embodiment, the back surface field layer may be tensile, with a germanium content lower than that of the terminal composition of graded buffer layer 404, for example about 25% lower Ge; in this case, the thickness of the back surface field layer may be thinner, for example about 20-100 nm. Due to the energy band offsets introduced by tension, a tensile back surface field layer may be more effective than a lattice-matched one. SiGe subcell 406 can include a base layer, with a Ge composition anywhere between 50-90%, approximately matched to the terminal germanium composition of graded buffer layer 404. The base layer can have a thickness of between 0.5-5.0 um with p type doping levels of about 1e15-1e17 cm−3. If the back surface field layer is included it can be below and in contact with the base layer.
An emitter layer can be grown on top of the base layer having a similar germanium composition or matched to the surface of the base layer. The emitter layer can have a n type doping level of 5e17-5e19 cm−3, or for example levels of about 1e18-5e18 cm−3.
The emitter layer can have a thickness of about 100-2000 nm, or for example about 200-500 nm. An optional transition layer (not shown) can be provided between the SiGe subcell 406 and the GaAsP subcell 410. The transition layer can be, for example, a 100% germanium layer having n type doping levels of about 1e18-1e20 cm−3, or for example levels of about 5e18-5e19 cm−3 with a thickness of 5-15 nm. On top of this transition layer, a III-V nucleation layer of InGaP (not shown) with a thickness of about 10-100 nm and doping of 1e18-1e19 cm−3 can be provided. The doping type (n or p) of the III-V nucleation layer may match that of the layer immediately beneath and in contact with the III-V nucleation layer, to avoid forming a junction. The purpose of the nucleation layer is to allow for the initiation of quality III-V semiconductor growth on top of the group IV semiconductor layers (SiGe) below. This and subsequently described III-V layers can be grown in an MOCVD (Metal Oxide Chemical Vapor Deposition) system such as a Veeco TurboDisc As/P (Arsenide/Phosphide) MOCVD System, by methods well known in the art.
The tunnel junction 408 can be provided between the SiGe subcell 406 and GaAsP subcell 410. The tunnel junction 408 can comprise a bottom tunnel junction portion comprised of SiGe interfacing SiGe subcell 406, with n-type doping levels of about 7e18-1e20 cm−3 with a thickness of 5-20 nm. The percent of germanium can be approximately matched to the terminal germanium composition of graded buffer 404, or it can be richer in germanium (e.g up to about 20% higher in Ge content, and may be pure Ge) for narrower bandgap to promote more effective tunneling behavior. A top SiGe tunnel junction portion can be provided having p type doping levels of about 7e18-1e20 cm−3 with a thickness of 5-20 nm. Again, the percent of germanium can be approximately matched to the terminal germanium composition of graded buffer 404, or it can be richer in germanium (e.g up to about 20% higher in Ge content, and may be pure Ge) for narrower bandgap to promote more effective tunneling behavior. The tunneling interface is between the n-type bottom tunnel junction portion and the p-type top tunnel junction portion.
Transition layers 409 can be provided between the tunnel junction layers 408 and the GaAsP subcell 410. The transition layers may include a bottom transition layer interfacing tunnel junction 408 and comprising for example pure germanium, having p type doping levels of about 1e18-1e20 cm−3, or for example levels of about 5e18-5e19 cm−3, with a thickness of 5-30 nm. The transition layers may also include a top transition layer interfacing GaAsP subcell 410 comprised of a III-V semiconductor approximately lattice matched to the terminal portion of graded buffer 404, for example an InGaP layer with a thickness of about 10-100 nm and p-type doping of 1e18-1e19 cm−3 can be provided. The purpose of the top transition layer is to allow for the initiation of quality III-V semiconductor growth on top of the group IV semiconductor layers below. This and subsequently described III-V layers can be grown in an MOCVD (Metal Oxide Chemical Vapor Deposition) system such as a Veeco TurboDisc As/P (Arsenide/Phosphide) MOCVD System, by methods well known in the art.
The GaAsP subcell 410 can include a back surface field layer which may have a lattice constant approximately matching the terminal composition of graded buffer 404, and thickness of between e,g. 50-200 nm, with p type doping levels of about 1e17-1e19 cm−3, or for example between 3e17-3e18 cm−3. This layer may be comprised of GaAsP, or of a wider-bandgap semiconductor layer such as InGaP. GaAsP subcell 410 can include a GaAsP base layer above the back surface field layer, which may have lattice constant approximately matching the terminal composition of graded buffer 404, and a thickness of between 0.2-2.0 um, with p type doping levels of about 1e16-1e18 cm−3, or for example about 1e17-2e17 cm−3. Alternately, the GaAsP base layer can be slightly tensile, with for example about 0.05-0.15% strain. A GaAsP emitter layer may be grown above the GaAsP base layer with n type doping of e.g. 1e17-1e19 cm−3, or about 1e18-3e18 cm−3, and with a lattice constant similar to the GaAsP base layer. The GaAsP emitter layer can have a thickness of about 50-200 nm, or about 100 nm. Additional layers can include a window layer of AlInP or InGaP, for example with a lattice constant similar to the underlying GaAsP base and emitter layers, and thickness of between 10-50 nm, with n type doping levels of for example about 2e17-2e18 cm−3. Alternately, the window layers may be somewhat tensile, with up to e.g. 2% tensile strain, allowing a wider bandgap for less ultraviolet absorption. A GaAsP or GaAs contact layer can also be provided with a lattice constant similar to the terminal portion of graded buffer 404, and a thickness of between 100-500 nm with n type doping levels of about 5e18-1e20 cm−3. The contact layer may be removed via wet etching after subsequent top contact grid formation, and thus only remain under the top contact grid in the final structure, an approach which is well known in the art of making III-V-based multi-junction solar cells. An exemplary process of creating a GaAsP cell is known in the art. For example, see Vernon et al., “Development of high-efficiency GaAsP solar cells on compositionally graded buffer layers”, page 108-112, IEEE Photovoltaic Specialists Conference, 19th, New Orleans, La., May 4-8, 1987, Proceedings.
Top contacts 412 can be provided on the exposed surface of the GaAsP subcell 410. The top contacts 412 can be provided by known methods in the art. For example, a grid structure of AuGe with a thickness of e.g. 1 um-5 um may be provided. It should be noted that a CrAu grid structure can be used for a P-type surface. Anti-reflection coating (ARC) of silicon nitride with a thickness of about 10-500 nm can also be provided to improve the solar cell efficiency. Methods and materials for providing top contacts and top ARC for III-V based multi-junction solar cells are well known in the art. A transparent substrate 416 can be bonded to the top surface of the multi-junction solar cell to provide support and protection. The transparent substrate 416 can be, for example, a sheet of module glass. The transparent substrate 416 can be bonded to the top surface by epoxy 418 or other methods of bonding.
The donor substrate 402 may be removed from the first portion of a solar cell bonded to the transparent substrate 416 by cleaving the donor substrate 402 within the porous layers 402a. Separation may be via mechanical force alone, or enhanced with various other methods. For example, a wedged device (not shown) may be applied to induce separation at the exposed external edges of the porous region 402a. In another example, separation may be enhanced via application of a high pressure water jet directed at the edge of the porous silicon layers 402a, as described in Yonehara & Sakaguchi. In yet another example, a wet acid solution, such as HF/H202, may also be exposed to the porous region 402a to erode the porous region 402a from the edge and enhance separation. It should be understood that the above examples of separation may be used individually or in various combinations.
The bottom contact surface of the substrate 402 can be textured with NaOH, KOH (potassium hydroxide) or TMAH, or by other means such as plasma etching, or sand blasting as is known in the art, to provide a pyramidally textured surface. Such a surface will cause light redirection upon reflection from the rear surface. Re-direction of the light away from a direction substantially normal to the top solar cell surface promotes total internal reflection. A thin (e.g. 10-1000 nm, or for example about 100 nm) dielectric layer of e.g. SiNx or SiO2 can be deposited on the bottom of substrate 402, after optional texturing takes place. This layer, not shown, can be between layers 402 and 414 in
Referring to
In an alternative embodiment, the solar cell can be grown on a p-type silicon substrate instead of n-type. In this case, the doping type of each layer of graded buffer 104, SiGe subcell 106, tunnel junction 108, transition layers 109, and GaAsP subcell 110 will be reversed, n-type instead of p-type and vice versa. In this embodiment, to increase current in the SiGe subcell 106, a SiGe superlattice may be employed. In this case the SiGe base region may include thin layers of high and low Ge content. For example, the SiGe base region may include e.g. 10 compressively strained layers of SiGe e.g. 30 nm thick, with Ge content e.g. 10% higher than the terminal germanium composition of graded buffer layer 104. These layers could be interleaved with e.g. 10 tensiley strained layers of SiGe e.g. 30 nm thick, with Ge content e.g. 10% lower than the terminal germanium composition of graded buffer layer 10. Such a superlattice of alternating compressive and tensile layers is said to be ‘strained balanced’, and can include an arbitrary number of alternating strained layers without relaxing. A benefit of this approach is that the high-Ge-content layers capture low energy photons that would otherwise pass through the solar cell. The energy band alignments of compressively versus tensily strained SiGe layers are such that the conduction band offsets between such alternating regions are minimal, allowing relatively free flow of photogenerated minority carrier holes.
In another alternative embodiment, for the case of an n-type substrate, n-type base regions and p-type emitter regions as originally described above, the bottom transition layer of e.g. pure Ge can be omitted from transition layers 109, and the top transition layer (a III-V semiconductor) interfaces directly with tunnel junction 108. In this case, the well known autodoping effect may be used to produce or to increase the n-type doping in top portion of tunnel junction 108. The autodoping effect is where, where under proper growth conditions, the growth of a III-V semiconductor containing P or As causes n-type doping of an immediately underlying group IV semiconductor surface, through diffusion of P or As into the group IV semiconductor. The conditions employed to create the autodoping effect is well known in the art, yet as an example, the P or As diffusion is commonly employed during the heat-up and bake of the substrate while having an overpressure of the Group V source. The depth and amount of P or As diffusion is controlled by the temperature and time of baking before the initiation of the Group III source, which initiates the growth of the III-V semiconductor. It is because our solar cell design optionally allows the n-type portion of tunnel junction 108 to directly interface a III-V semiconductor layer (the above-described top transition layer, for the case where the bottom transition layer is omitted) that we can take advantage of the autodoping effect to increase or even to create the n-type doping in the top portion of tunnel junction 108.
In an alternative embodiment, for the case of an n-type substrate, n-type base regions and p-type emitter regions as originally described above, the bottom transition layer of e.g. pure Ge can be omitted from transition layers 109, and additionally the n-type SiGe portion of tunnel junction 108 may be omitted. In this case, the tunneling interface is directly between a p-type SiGe tunnel junction region and an n-type III-V transition layer such as InGaP.
In an alternative embodiment, a porous Si Bragg reflector can be included below the SiGe subcell, to improve reflectance of light that has passed through the SiGe subcell. The means to produce a porous Si Bragg reflector, and to subsequently grow quality epitaxy on top, are described for example in Niewenhuysen et al. “Epitaxial thin film silicon solar cells with CVD grown emitters exceeding 16% efficiency”, 34th IEEE PVSC, (2009). This reflector can be either instead of, or in addition to, a reflector on the rear surface of the silicon handle wafer as described above.
In an alternative embodiment, a supplemental top contact layer may be provided to allow more flexibility in top contact metallurgy. While III-V layers are typically contacted with stacks of multiple metals often including expensive Au, silicon can be contacted by single low-cost metals such as Aluminum. Therefore, one may deposit on top of GaAsP subcell 110, via e.g. PECVD, a thin in-situ doped amorphous or microcrystalline Si layer, with doping type the same as the top of GaAsP subcell 110. The means of depositing such via PECVD are well known in the art. This layer may be deposited directly on top of and in contact with a III-V contact layer such as GaAs or GaAsP on top of GaAsP subcell 110. Alternately, the III-V contact layer may be omitted, and the amorphous Si may be deposited directly on top of the window layer of GaAsP subcell 110.
Other modifications and substitutions by one of ordinary skill in the art are considered to be within the scope of the present invention, which is not to be limited except by the following claims.
This application claims the benefit of and priority to U.S. Provisional Application Ser. No. 61/530,680 filed Sep. 2, 2011, U.S. Provisional Application Ser. No. 61/650,133 filed May 22, 2012, and U.S. Provisional Application Ser. No. 61/657,698 filed Jun. 8, 2012, the disclosures of which are hereby incorporated by reference in their entirety.
Portions of the present invention may have been made in conjunction with Government funding under contract number HR0011-07-9-0005, and there may be certain rights to the Government.
| Number | Date | Country | |
|---|---|---|---|
| 61530680 | Sep 2011 | US | |
| 61650133 | May 2012 | US | |
| 61657698 | Jun 2012 | US |