Stack-type multi-junction solar cell
US-2018351020-A1 · Dec 6, 2018 · US
US11916159B2 · US · B2
| Field | Value |
|---|---|
| Publication number | US-11916159-B2 |
| Application number | US-202217986663-A |
| Country | US |
| Kind code | B2 |
| Filing date | Nov 14, 2022 |
| Priority date | Jan 28, 2021 |
| Publication date | Feb 27, 2024 |
| Grant date | Feb 27, 2024 |
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A multijunction solar cell including an upper first solar subcell having a first band gap and positioned for receiving an incoming light beam; and a second solar subcell disposed below and adjacent to and lattice matched with said upper first solar subcell, and having a second band gap smaller than said first band gap; wherein at least one of the solar subcells has a graded band gap throughout the thickness of at least a portion of its emitter layer and base layer.
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The invention claimed is: 1. A method of fabricating a multijunction solar cell comprising: forming a first solar subcell, having an emitter layer and a base layer which form a photoelectric junction; and forming a second solar subcell disposed below and adjacent to said first solar subcell, having an emitter layer and a base layer which form a photoelectric junction; and wherein the base layer and the emitter layer of at least a particular solar subcell from among the first solar subcell and the second solar subcell has a graded band gap throughout at least a portion of a thickness of the emitter layer or the base layer in a first region in the emitter layer adjacent to the photoelectric junction, and throughout at least a portion of a thickness of its base layer in a second region spaced apart from the first region and adjacent to the junction, with the band gap in the first region and the band gap in the second region being in the range of 20 to 300 meV greater than the band gap away from the photoelectric junction in the emitter layer or the base layer in the at least the particular subcell. 2. A method as defined in claim 1 , wherein the thickness of the first region is equal to the thickness of the second region. 3. A method as defined in claim 1 , wherein the band gap in the emitter layer in the first region in the particular one of the first solar subcell and the second solar subcell increases to a first level, and then decreases to a second level in the base layer that is lower in band gap than the first level in the emitter layer of at least one solar subcell. 4. A method as defined in claim 1 , further comprising a third region in the emitter layer in the particular one of the first solar subcell and the second solar subcell that lies directly adjacent to and space apart from the first region, wherein the band gap in the third region is constant. 5. A method as defined in claim 2 , further comprising a fourth region in the base layer in the particular one of the first solar subcell and the second solar subcell that lies directly adjacent to and spaced apart from the second region, where the band gap in the fourth region is constant. 6. A method as defined in claim 3 , wherein the first level of the band gap is substantially located at the photoelectric junction of the particular one of the first solar subcell and the second solar subcell. 7. A method as defined in claim 3 , wherein the second level of the band gap is substantially located in the depletion region in the base layer of the particular one of the first solar subcell and the second solar subcell. 8. A method as defmed in claim 5 , wherein the band gap in the third region of the particular one of the first solar subcell and the second solar subcell equals the band gap in the fourth region of the at least one subcell. 9. A method as defined in claim 1 , wherein thea depletion region of the particular one of the first solar subcell and the second solar subcell is asymmetric around the photoelectric junction of the at least one subcell. 10. A method as defined in claim 1 , wherein thea width of the graded band gap region in the particular one of the first solar subcell and the second solar subcell is equal to the width of a depletion region in the at least one of the first solar subcell and the second solar subcell. 11. A method as defmed in claim 1 , wherein the band gap has a peak that is centered approximately where the Fermi level of the particular one of the first solar subcell and the second solar subcell crosses mid-band. 12. A method as defined in claim 1 , wherein the first and second regions of the graded band gap of the particular one of the first solar subcell and the second solar subcell is asymmetric around thea depletion region of the at least one of the first solar subcell and the second solar subcell. 13. A method as defined in claim 1 , wherein the first and second regions of the graded band gap of the particular one of the first solar subcell and the second solar subcell is (i) symmetric around the photoelectric junction. 14. A method as defined in claim 1 , and the first solar subcell is composed of indium gallium aluminum phosphide and has a first band gap in the range of 2.0 to 2.2 eV, wherein the emitter layer of the second solar subcell is composed of indium gallium phosphide or aluminum indium gallium arsenide, and the base layer of the second solar subcell is composed of aluminum indium gallium arsenide, the second solar subcell having a second band gap in the range of approximately 1.55 to 1.8 eV and being lattice matched with the first solar subcell and further comprising a third solar subcell disposed adjacent to said second solar subcell and composed of indium gallium arsenide and has a third band gap less than the second band gap of the second solar subcell and is lattice matched with the second solar subcell. 15. A method as defined in claim 14 , wherein the solar cell is configured for optimum operation in (i) a LEO earth orbit; (ii) a GEO earth orbit; (iii) a Mars environment; or (iv) a Jupiter environment. 16. A method as defined in claim 1 , further comprising a third solar subcell disposed below and adjacent to the second solar subcell wherein the first solar subcell, the second solar subcell, and the third solar subcell each have a graded band gap throughout at least a portion of the thickness of its respective emitter layer and base layer. 17. A method as defined in claim 1 , further comprising an intermediate graded layer disposed between one of the first solar subcell and the second solar subcell and the adjacent solar subcell disposed directly below the one solar subcell, wherein the intermediate layer is compositionally graded to lattice match the one of the first solar subcell and the second solar subcell on one side and the adjacent solar subcell on the other side and is composed of any of the As, P, N, Sb based III-V compound semiconductors subject to the constraints of having the in-plane lattice parameter greater than or equal to that of the one solar subcell and less than or equal to that of the adjacent solar subcell, and having a band gap greater than that of the one of the first solar subcell and the second solar subcell. 18. A method as defined in claim 1 , further comprising forming a bottom solar subcell disposed below the second solar subcell, and an intermediate graded layer disposed between the second solar subcell and the bottom solar subcell, wherein the intermediate layer is compositionally step-graded with between one and four steps to lattice match the second solar subcell on one side and the bottom solar subcell on the other side and composed of InGaAs or (In x Ga 1-x ) y Al 1-y As with 0<x<1, 0<y<1, and x and y selected such that the band gap remains at a constant value. 19. A method as defined in claim 14 , further comprising: a distributed Bragg reflector (DBR) layer disposed adjacent to and beneath the third solar subcell and arranged so that light can enter and pass through the third solar subcell and at least a portion of which can be reflected back into the third solar subcell by the DBR layer, wherein the distributed Bragg reflector layer is composed of a plurality of alternating layers of lattice matched materials with discontinuities in their respective indices of refraction, wherein the difference in refractive indices between alternating layers is maximized in order to minimize the number of periods required to achieve a given reflectivity, and the thickness and refractive index of each period determines the stop
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