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Conversion efficiency limits and bandgap designs for multi-junction solar cells with internal radiative efficiencies below unity

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Abstract

We calculated the conversion-efficiency limit ηsc and the optimized subcell bandgap energies of 1 to 5 junction solar cells without and with intermediate reflectors under 1-sun AM1.5G and 1000-sun AM1.5D irradiations, particularly including the impact of internal radiative efficiency (ηint) below unity for realistic subcell materials on the basis of an extended detailed-balance theory. We found that the conversion-efficiency limit ηsc significantly drops when the geometric mean ηint* of all subcell ηint in the stack reduces from 1 to 0.1, and that ηsc degrades linearly to logηint* for ηint* below 0.1. For ηint*<0.1 differences in ηsc due to additional intermediate reflectors became very small if all subcells are optically thick for sun light. We obtained characteristic optimized bandgap energies, which reflect both ηint* decrease and AM1.5 spectral gaps. These results provide realistic efficiency targets and design principles.

© 2016 Optical Society of America

1. Introduction

Detailed-balance theories, started by Shockley and Queisser [1], predict the conversion-efficiency limits (ηsc) and optimum bandgaps (Eg) of multi-junction solar cells [2], which are ηsc = 30% with Eg = 1.3 eV (1 junction), ηsc = 42% with Eg’s of 1.9 eV and 1.0 eV (2 junctions), and ηsc = 49% with Eg set of 2.3 eV, 1.4 eV, and 0.8 eV (3 junctions), for unconcentrated 6000K blackbody sun. Over many years, calculations have been extended to various radiation conditions (6000K blackbody, AM0, AM1.5 global and AM1.5 direct solar spectrum, etc. with 1- to 46000-fold concentrations), reflector configurations (ideal reflectors between the interfaces of subcells, with back-mirror, or without back-mirror), and electrical interconnections (series or independent connections) [2–9]. These calculations [1–9] have so far been referenced as design targets and templates. However, all the above calculations were achieved under the assumption of the radiative limit, that is, by neglecting non-radiative recombination loss. In fact, carrier recombination events in almost all semiconductor materials at room temperature are dominated by non-radiative recombination, hence it is necessary to consider the impact of non-radiative recombination losses to predict conversion efficiency limit and optimal bandgap for semiconductor solar cells.

Shockley and Queisser incorporated the effect of non-radiative recombination processes on single junction cell performance by using the external radiative efficiency (denoted hereinafter as ηext), which is defined as the ratio of the radiative recombination current due to external emission from the cell versus the total recombination current [1]. Green [10,11] surveyed state-of-the-art single junction cells under AM1.5 G spectrum and explained their conversion efficiencies assuming various ηext values. Chan [12] presented the calculations for optimal bandgaps for 1- to 3-junction solar cells while incorporating the effects of ηext by using the two-diode model for considering non-radiative Shockley-Read-Hall (SRH) recombination. Although the quantity ηext reflects cell material quality, it is affected also by cell structures, such as surface reflectivity, cell thickness, substrate material, and so on.

In contrast, internal radiative efficiency (ηint), defined as the fraction of the internal radiative recombination rate over the total recombination rate, is a suitable property that directly represents material quality independent of cell structure factors. Yablonovitch et al. [13–17] investigated conversion efficiency limits of single-junction solar cells, as a function of internal radiative efficiency to include a finite non-radiative recombination. They pointed out that a very slight deviation of ηint from 1 caused conversion efficiency ηsc to degrade significantly and sharply from the radiative-limit value.

Multi-junction solar cells consist of a series of subcells with different materials. It is unrealistic to assume that all the materials in the stack have ideally high quality. Indeed, materials with ηint close to 1 are rare, except for GaAs [18]. Moreover, under high concentration, the operating temperature of multi-junction cells would rise significantly, which further increase non-radiative recombination losses in each subcell, thereby causing the realistic subcell ηint to deviate from 1. Hence, it is important to evaluate the effect of all the subcells’ quality on ηsc and the multi-junction cell design. For this aim, we previously formulated and analyzed basic trends in conversion-efficiency limit ηsc and optimized Eg sets for the 2-junction tandem solar cells with finite subcell internal radiative efficiency ηint1 (top-cell) and ηint2 (bottom-cell) for unconcentrated 6000K blackbody sun [19]. We found that ηsc drops sharply when ηint1 or ηint2 slightly reduces from 1 to 0.9, that the optimized Eg set increases as ηsc decreases, and that the geometric mean ηint* = (ηint1ηint2)1/2 is a very useful parameter to represent the whole subcell quality. However, major attention in research and development is presently directed toward ηsc > 40% or 3-, 4-, and 5-junction structures for satellite or terrestrial concentrator uses. Thus, our formalism needs to be applied urgently to multi-junction cells and concentrator solar cells.

Considering that conversion efficiency (ηsc) is also affected by the structure and geometry of solar cells inevitably, in this work, we investigate ηsc and optimized subcell bandgap energies in three well-known versions of current-constrained 1- to 5-junction solar cells with no, air-gap and perfect intermediate reflectors for various ηint’s for all subcells and their geometric mean ηint* under the 1-sun AM1.5G and 1000-sun AM1.5D conditions. The results show that ηsc of the three versions of multi-junction solar cells drop significantly as ηint* decreases from 1 to 0.1 and then logarithmically as ηint* are reduced below 0.1. Differently from the well-investigated ideal multi-junction solar cells with ηint* = 1, the intermediate reflectors no longer boost ηsc in thick multi-junction solar cells, if ηint* is less than 0.1. Moreover, optimized bandgap energies in multi-junction solar cells made of low ηint values turned out to be much larger than those optimized for the familiar ideal cases with ηint = 1. The results provide realistic targets of efficiency limits and improved design principles of practical multi-junction solar cells.

2. Model

Figure 1 shows three versions of two-terminal multi-junction solar-cell structures studied in this work: (a) without intermediate reflectors, (b) with prefect selective intermediate reflectors that only reflect photons with energy greater than the subcell bandgap energy, and (c) with air-gap intermediate reflectors sandwiched by antireflection (AR) coatings. The structures (b) and (c) are designed for reducing external emission losses from subcell back surface to improve subcell voltage. We also assume that the three versions of multi-junction solar cells with parallel planar surfaces are all covered by AR coatings on topmost subcells and have prefect rear mirrors at bottommost subcells, thus, the reflectivity of AR coating is 0 and that of the rear mirrors is 1. Especially for single junction solar cells, the three cases are exactly the same. The solar cells consist of a stack of the materials with band gap Egi and an internal radiative efficiency ηint i. Subscript i represents a certain subcell. Subscripts 1 and n represent the uppermost- and bottommost-subcells, respectively. In typical multi-junction solar cells made of III-V compound semiconductors, refractive indices of subcells in the stack are close. Thus, each subcell refractive index (ni) can be reasonably and simply assumed to be equal to 3.5.

 figure: Fig. 1

Fig. 1 Structures of the multi-junction solar cells considered in this work (a) no intermediate reflectors, (b) with perfect intermediate reflectors (PIR) and (c) with air-gap intermediate reflectors. All of three versions of solar cells have planar surfaces, perfect front-surface AR coating on topmost cell and perfect rear mirror in bottommost cell.

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We define αsuni¯ as the energy-averaged absorption coefficient for sun-light absorption between this subcell Egi and the above subcell Egi-1 or , and separately define αlumii¯ as the energy-averaged absorption coefficient at luminescence energy of this subcell, respectively given as

αsuni¯=EgiEgi1orα(E)ϕsun(E)dEEgiEgi1orϕsun(E)dEandαlumii¯=Egiα(E)ϕlumi(E)dEEgiϕlumi(E)dE, (1, 2)
where α(E) is the subcell materials absorption coefficient that is a function as photon energy (E). In a similar way, we define energy- and angle-averaged absorptivity for sunlight (asuni¯) and for subcell luminescence (alumii¯). Note that the subcell luminescence spectrum (ϕlumi) has a different shape from the solar spectrum (ϕsun). Luminescence occurs near the band edge Egi, where the absorption coefficient sharply drops to zero. Thus, αlumii¯ is typically much smaller than αsuni¯ in practical materials. From the measured ϕlumi and photo-current external-quantum-efficiency (EQE) spectra in a standard InGaP/GaAs/Ge solar cell [20], we evaluated the ratios αlumii¯/αsuni¯ of 0.5, 0.6, and 0.15 in the respective subcells.

As for subcell thickness (li), it is firstly important for high efficiency that the absorption of solar photons is strong. Thus, we choose αsun¯l = 5 or exp(αsun¯l) = 0.007, in most calculations here, and αsun¯l = 2 or exp(αsun¯l) = 0.14, for comparison as a thinner case. In accordance with the above evaluated ratio αlumii¯/αsuni¯, we choose alumi¯l = 1 and 2 in most calculations, and analyzed effects of αlumi¯l later in some cases. We also assume infinite carrier mobility in all subcells, which means that minority carrier diffusion lengths are much larger than subcell thicknesses.

All subcells are connected in series, and the outflow currents (J) of all subcells are equal. According to carrier balance in each subcell, the current flux flowing out from each individual subcell would be equal to the difference between the carrier generation flux and carrier recombination flux. Thus, all of the subcell I-V characteristics in n-junction solar cells (n = 1, 2, 3, 4, and 5) are given by the following equations, for the case without intermediate reflectors:

{J/q=Rsun(Eg1,)Rext1(Eg1,,V1)[(1ηint11)4αlumi1¯l1n12alumi1¯+(1+ni2)],(a)J/q=Rsun(Egi,Egi1)+ni12Rexti1(Egi1,,Vi1)Rexti(Egi,,Vi)[(1ηinti1)4αlumii¯lini2alumii¯+(1+ni2)](i=2,3,..n1),(b)J/q=Rsun(Egn,Egn1)+nn12Rextn1(Egn1,,Vn1)Rextn(Egn,,Vn)[(1ηintn1)4αlumin¯lnnn2alumin¯+1],(c)
where Rsun(Elow,Ehigh)=πasun¯ElowEhighϕsun(E)dE is the carrier generation rates, Rexti(Egi,,Vi) = πalumii¯Egiϕlumii(E)dEexp(Viq/kTc) is the external radiative emission rate from the front surface of subcell i, Vi and kTc/q are the subcell voltages and the thermal voltage. The right-hand side of Eq. (3) are the net of carrier generation rates by absorption from sunlight (1st term) and by luminescence coupling from the adjacent upper subcell in subcell i1 (2nd term), carrier loss rates by NR recombination (3rd term), and by external emissions via the upper and bottom surfaces (4th term). The terms in square brackets after Rexti came from the general expression of 1/ηexti=(1ηintiPabsi¯)/ηintiPesci¯ [21, 22] deduced by including the probability of phonon re-absorption within subcells and Pesci¯=alumii¯/4αlumii¯lini2. In the thin limit, Pesci¯ approaches to the well-known values of 1/4ni2 and 1/2ni2 according to the bottom reflectivity of 0 and 1, respectively [22]. Equation (3) is equivalent to
{J/q=Rsun(Eg1,)Rint1(Eg1,,V1)[(1ηint11)+alumi1¯4αlumi1¯l1n12(1+n12)],(a)J/q=Rsun(Egi,Egi1)+ni12Rexti1(Egi1,,Vi1)Rinti(Egi,,Vi)[(1ηinti1)+alumii¯4αlumii¯lini2(1+ni2)](i=2,3,..n1),(b)J/q=Rsun(Egn,Egn1)+nn12Rextn1(Egn1,,Vn1)Rintn(Egn,,Vn)[(1ηintn1)+alumin¯4αlumin¯lnnn2],(c)
where Rinti is the internal luminescence rate inside subcell i.

For the cases with the air-gap and perfect intermediate reflectors, Eq. (3)b) should be modified to

J/q=Rsun(Egi,Egi1)+Rexti1(Egi1,,Vi1)Rexti(Egi,,Vi)[(1ηinti1)4αlumii¯lini2alumii¯+2],
andJ/q=Rsun(Egi,Egi1)Rexti(Egi,,Vi)[(1ηinti1)4αlumii¯lini2alumii¯+1],respectively.

In this study, we use solar illuminations of incident power per unit area Pin = 100 mW/cm2 or Pin = 90 W/cm2 intensity conditions with the spectrum of AM1.5G (1-sun) and AM1.5D (1000-sun). For Pin on the front surface of the cell, we calculated the highest value of ηsc (the conversion-efficiency limit ηsc) by optimizing Egi set in the stack, for respective values of ηint1, ηint2, …, ηintn, as,

ηsc(ηint1,ηint2,,ηintn)=MaxEg1,Eg2Egni=1nIViPin.
We used Wolfram Mathematica’s maximization toolbox to maximize ηsc with respect Eg1, Eg2, …, Egn for a given set of (ηint1, ηint2, …, ηintn).

We define the geometric mean ηint*=ηint1ηint2ηintnn for an arbitrary set of (ηint1, ηint2, …, ηintn). We first studied various combinations of (ηint1, ηint2, …, ηintn) and confirmed that n-junction solar cells with the same geometric mean ηint* have almost the same conversion efficiency limit ηsc and optimized Egi set, provided that all subcells have ηint <0.3. This feature was previously found in the simplest 2-junction case [19]. Taking 3-junction solar cells for instance, curves in Fig. 2(a)-(b) show ηsc and optimized Eg set against ηint* under various combinations of (ηint1, ηint2, ηint3). The three colorized curves in Fig. 2(a), representing ηsc at the case of ηint2 = ηint3 = 0.3 (red), ηint1 = ηint3 = 0.3 (blue), and ηint1 = ηint2 = 0.3 (green), almost overlap with each other, which in fact are the upper bounds of evaluated ηsc at arbitrary combination of (ηint1, ηint2, ηint3) when all subcell ηint i <0.3. The black curves are ηsc under the case of ηint1 = ηint2 = ηint3, which are close to the three color curves. We also have chosen more than 15 random sets of (ηint1, ηint2, ηint3) that independently vary from 0.3 to 10−10 (the lower bound of ηint i is around 10−17 [23]) but their geometric means ηint* are fixed as 0.1 (circles), 0.01 (triangles), 0.001 (inverted triangles), and 0.0001 (squares), respectively. It is clear that all of the symbols always sit in a narrow area between green (upper bound) and black curves (lower bound) with a deviation less than 0.2-0.3%. Thus, if ηint < 0.3 is satisfied in all subcells, ηint* can be deemed to a representative measure of all subcell material qualities for more-junction solar cells. To summarize the effects induced by various subcell qualities combinations, we only have to calculate the case of all the subcell ηint in the stack having the same values ηint1 = ηint2 = … = ηintn = ηint* to estimate the ηsc limit of n-junction solar cells for an arbitrary set of (ηint1, ηint2,…, ηintn) almost giving the same ηint*. The calculated results shown below were obtained in this way.

 figure: Fig. 2

Fig. 2 (a) The efficiency ηsc and (b) optimized Eg set of 3-junction solar cells without intermediate reflectors as function of ηint* under various combinations of (ηint1, ηint2, ηint3). Black, red, blue, and green curves in (a) respectively represent the values of ηsc at the case of ηint1 = ηint2 = ηint3, ηint2 = ηint3 = 0.3, ηint1 = ηint3 = 0.3, and ηint1 = ηint2 = 0.3. Circles, triangles, inverted triangles and squares represent more than 15 random combinations of (ηint1, ηint2, ηint3) that independently vary between 0.3 and 10−10 but their geometric means ηint* are fixed as 0.1, 0.01, 0.001, and 0.0001, which were amplified in (c)-(f).

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3. Results and discussion

Figure 3 summarizes the optimum ηsc of three versions of 1- to 5-junction solar cells, for various ηint* between 1 and 0.00001 at the four conditions: (a) αsun¯l = 5 and αlumi¯l = 1 under 1-sun irradiation, (b) αsun¯l = 5 and αlumi¯l = 1 under 1000-sun irradiation, (c) αsun¯l = 5 and αlumi¯l = 2 under 1-sun irradiation, and (d) αsun¯l = 2 and αlumi¯l = 1 under 1-sun irradiation for analyzing the effects of imperfect sunlight absorption. The dashed, solid, dotted curves in Fig. 3 show ηsc of multi-junction solar cells of without intermediate reflector, with perfect and with air-gap intermediate reflectors. The three kinds of black curves show ηsc at ηint* = 1, or in the radiative limit assuming ideal materials without non-radiative loss. These agree well with the previously reported results [1–9] except for slight dissimilarities due to differences in detailed calculation parameters. If we select αsun¯l5 and αlumi¯l5 for calculation, we will get the same ηsc limits as these pervious detailed balance limits. As mentioned in the introduction, practical materials with ηint close to 1 are very rare, and the black curves for ηint* = 1 are unrealistic to estimate ηsc for practical designs. The lower colored curves in Fig. 3 show ηsc of the three versions of multi-junction solar cells for ηint* = 0.1, 0.001, and 0.00001. Note that ηsc drops very drastically as ηint* decreases from 1 to 0.1, revealing that ηsc is very sensitive to ηint* in this region. If ηint* is below 0.1, the reduction in ηsc is almost constant, as ηint* drops by one order of magnitude. In other words, the efficiency penalty Δηsc is almost linear to log10ηint* in this low-ηint* region. Furthermore, the efficiency penalty Δηsc is increased as the junction number n increases. Taking the multi-junction cells in Fig. 3(a)-(b) with αsun¯l = 5 and αlumi¯l = 1 for instance, decrease in ηsc per decade decrease in ηint* of three versions of multi-junction solar cells for n = 2, 3, 4, and 5 in the region of ηint* close to 0.001 was around 2.49%, 2.82%, 2.85% and 2.95% under 1-sun, while that was around 2.89%, 2.99%, 3.37% and 3.44% under 1000-sun, respectively. Figure 3(a)-(b) clearly illustrate that subcell material quality affects ηsc very similarly in no and high concentration operations.

 figure: Fig. 3

Fig. 3 The optimized efficiency ηsc [%] of multi-junction solar cells with no (dashed curves), air-gap (dotted curves) and perfect intermedium reflectors (solid curves) as function of junction number at various values of ηint* = 10−5, 10−3, 0.1, and 1 for (a) αsun¯l = 5 and αlumi¯l = 1 (1-sun), (b) αsun¯l = 5 and αlumi¯l = 1 (1000-sun), (c) αsun¯l = 5 and αlumi¯l = 2 (1-sun) and (d) αsun¯l = 2 and αlumi¯l = 1 (1-sun).

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We compared ηsc for the three versions of solar cells in Fig. 3(a)-(d) and found clear increase in ηsc for 2- to 5-junctinon solar cells with ηint* = 1, by adding air-gap or perfect intermediate reflectors. These results are consistent with the previous researches showing the boosts of ηsc caused by the air-gap or perfect reflectors [9]. However, it turned out in Fig. 3(a)-(c) that ηsc with different reflectors are very close to each other when ηint* are less than 0.1. For a thin cell with insufficient sunlight absorption with αsun¯l = 2, Fig. 3(d) shows that ηsc with perfect reflection is obviously higher than that with no reflection even for ηint*<0.1, but is still similar to that in Fig. 3(a). Such improvement in ηsc stem from simple improvement in the sunlight absorptivity from asuni¯ = 85% for single pass without reflection to asuni¯ = 98% for double pass with perfect reflection. Therefore, we may summarize that intermediate reflectors no longer cause large ηsc boost for ηint*<0.1, in stark contrast to the ideal case with ηint* = 1, except for trivial compensation effect for insufficient sunlight absorption in thin solar cells. When solar cells are thick enough for single pass sunlight absorption, as is the case with typical practical cells, the advantage of intermediate reflectors is washed away by low ηint*<0.1. The reason is clear: for the solar cells with extremely high materials quality, the intermediate reflectors assist in photon recycling in the subcells that leads to higher internal voltage; however, for the cells with moderate or low quality, carrier recombination losses are dominated by non-radiative recombination (the 3rd term in Eq. (3)), and the external emission from the subcells (the 4th term in Eq. (3)) becomes very small. Thus, the intermediate reflectors in practical multi-junction solar cells become ineffective.

These results in Fig. 3 indicate that the impact of ηint* on efficiency ηsc is significant and must be included in the assessment or design of high-efficiency multi-junction solar cells. Our recent experimental study [20] on commercially available satellite-use InGaP/GaAs/Ge 3-junction solar cells indicated that ηint* was as low as 0.01 at the maximum-power operation condition under a 1-sun condition. Note that ηint*’s in this paper mean those at the maximum-power operation condition. Note also that ηint* is strongly bias-voltage (bias-current) dependent, and that ηint* of the present sample was about 0.1 at the open-circuit condition under a 1-sun condition. We may regard subcell materials with ηint* = 0.1 and 0.001 at the maximum-power operation condition, for example, as “good” and “moderate” materials respectively. ηsc limit of “good” and “moderate” multi-junction solar cells are clearly lower than that in the radiative limit (ηint* = 1) by several to 10% absolute, which reasonably explain why ηsc’s of realistic multi-junction solar cells [24] empirically deviate from the detailed-balance-theory predictions. Therefore, the colored curves for ηint* below 0.1 in Fig. 3(a-b) provide more realistic targets of ηsc than the prevailing data calculated for ηint* = 1.

Note that Fig. 3(c) for αlumi¯l = 2 with stronger self-absorption of luminescence showed slightly lower ηsc than that in Fig. 3(a) for αlumi¯l = 1. According to the results in Fig. 3, it is necessary to discuss the effects of material absorptivity for sunlight and subcell self-luminescence on ηsc limit.

Figure 4 plots ηsc as function of αlumi¯l for the three versions of 3-junction solar cells with ηint* = 1 (“ideal”), 0.1 (“good”), and 0.001 (“moderate”) having (a) strong sunlight absorption αsun¯l = 5 and (b) incomplete sunlight absorption αsun¯l = 2. Note that ηsc decreases gently as luminescence absorptivity (αlumi¯l) increases, for fixed αsun¯l. The reason is clear in Eqs. (3)-(4): as αlumi¯l increases, alumii¯, 4αlumii¯lini2/alumii¯, and dark current density J0i = qRext(Egi,, 0) increase, and both radiative and non-radiative recombination losses increase to lower ηsc. On the other hand, it is trivial that high values of asuni¯ can generate more photocurrents that leads to increase in ηsc. High-efficiency solar cells prefer large asuni¯ and small alumii¯, and have optimum thickness.

 figure: Fig. 4

Fig. 4 The efficiency ηsc of 3-junction solar cells with no (dashed curves), air-gap (dotted curves) and perfect intermedium reflectors (solid curves) at ηint* fixed as 1, 0.1, and 0.001 as function of alumi¯l for (a) asun¯l = 5 and (b) asun¯l = 2.

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The bar graph in Fig. 5(a)-(b) shows the optimized bandgaps combination (Eg1, Eg2, …, Egn) at ηint* = 1~0.00001, for n-junction (n = 1, 2, 3, 4, and 5) solar cell without reflectors under (a) 1-sun and (b) 1000-sun conditions. Since intermediate reflectors make negligible difference under ηint*<0.1 with αsun¯l = 5, we only show the case of no intermediate reflectors. Note that the optimized bandgaps blue-shifted as ηint* decreased. In the case of (a) 1-sun AM1.5G, blue-shifts in the optimized bandgaps are larger between ηint* = 1 and 0.1, than those occurred between an order of magnitude decrease in ηint* below 0.1, which are similar to the feature of ηsc limit against ηint* in Fig. 3(a). Note also that the bottommost bandgap Egn of n-junction solar cell tend to be pinned at around 0.70, 0.93, 1.12 and 1.38eV, corresponding to rising edge on the AM1.5 spectrum gaps due to atmospheric gas absorption. As a mixed result of the two trends of blue-shifts and the bandgap pinning, some anomalous jumps in the optimized bandgaps were found. In the case with (b) 1000-sun AM1.5D, the optimal bandgap sets are obviously smaller than those under (a) 1-sun. Since short circuit currents increase linearly with concentration ratio (C), while open circuit voltages roughly increase logarithmically with C, concentrator multi-junction cells with smaller bandgap combination materials tend to achieve higher efficiency. The two trends of blue-shifts and the bandgap pinning in the optimized Egi set with ηint i clarified in (a) were also found under concentrating operation (b), where the effect of bandgap pinning was very obvious and the larger blue shifts between ηint* = 1 and 0.1 than those below 0.1 was not significant.

 figure: Fig. 5

Fig. 5 The optimized set of bandgaps Egi [eV] as function of junction number at various values of ηint* = 0.00001~1, for αsun¯l = 5 and αlumi¯l = 1 under (a) AM1.5G (1-sun) and (b) AM1.5D (1000-sun).

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The blue-shifts of the optimized Egi set with ηint i decrease are the same with those found in our previous basic study on 2-junction solar cells under 6000K blackbody irradiation, that is a continuous spectrum without any gaps, and can be ascribed to the following reason. Subcell open circuit voltage (Voci) is determined by subcell bandgap and the term of voltage penalty due to imperfect material quality (ηint i <1) independent of bandgap, expressed as VociEgi + kTcln(ηint i)-C, where C is a constant determined by subcell structure and material properties, such as refractive index [21]. If ηint i becomes low, subcell Voci should decrease. Therefore, larger Egi should compensate for this penalty in Voci. Due to the series connection of subcells, the extracted current is limited by the least photo-generated current among all the subcells in the stack, and the optimal bandgaps must be chosen so as to satisfy the current-matching condition. It is interesting but reasonable that change in ηint i of only one subcell i causing a change in ηint*, which affects the optimization of all bandgaps in the stack.

The present work provides instructive conclusions and proposals for the practical design of high-efficiency multi-junction solar cells. The efficiency limits for 2- and 3-juntion cells without intermediate reflectors under 1-sun are high, which are respectively 38.2% and 43.5% for ηint* = 0.1, and 33.0% and 37.6% even for ηint* = 0.001 at αsun¯l = 5 and αlumi¯l = 1, provided that a properly blue-shifted optimal-bandgap set is chosen. This result reveals that 2- and 3-juntion cells still can be implemented as a potential alternative for higher-efficiency solar cells, since the efficiency of them can be further improved if we use proper bandgap sets optimized in accordance with the material quality. We additionally note that the improvements in ηsc becomes small: 2.5% and 2.1% when junctions are increased from 3- to 4-junctions and from 4- to 5-junctions, respectively, under 1-sun with ηint* = 0.001. That is to say, additional efficiency add-on is very small for a high number of junctions. Though this trend has already been proven [2, 9] for the case of ηint* = 1, here we confirmed it generally for all the cases of ηint* = 1, 0.1, and ηint*<<1.

Under concentration conditions, basic trends are similar to the above case without concentration: even for moderate materials with ηint* = 0.001, the ηsc limits for 2- and 3-juntions under 1000-sun at are high, 40.1% and 45.6%, respectively, but with an obvious blue-shifted optimal-bandgap set. Improvements in ηsc are not large, 3.0% and 2.1%, for junctions increases from 3 to 4 and from 4 to 5, respectively, for 1000-sun and ηint* = 0.001. For practical 3-junction cells, it is empirically considered that popular InGaP/(In)GaAs/Ge or InGaP/GaAs/InGaAs cells have already reached their practical efficiency upper limits under concentrated light, limited by subcell materials and lattice mismatch [25–29]. Therefore, several research groups explore new materials [25], new design [27] and new process [29,30] for 3- or more-junction structures. Our results and calculation model presented here provide useful design targets on subcell bandgap combination and efficiency reference for high-efficiency multi-junction solar cells.

Additional improvement in ηsc may occur at increased concentrations or pumping power density, with the help of improvements in ηint of each subcell. We believe that such improvement in ηint partly contributes to improvement in ηsc of practical solar cells at high concentrations, based on the results shown in Fig. 3(b). On the other hand, we note that the temperature of the multi-junction solar cells would increase under high concentrating operations, which usually causes significant reduction in ηsc obversed in experimental studies [31–33].

We here remind the readers that all the above results were obtained for αsun¯l and αlumi¯l being some assumed values, and a refractive index of 3.5. With different input values, the values of ηsc and optimized bandgaps may change. However, within realistic input values, the resulting values of optimal bandgap set of reasonably thick solar cells usually change slightly. Moreover, the qualitative features obtained in this study remain valid. In this study, we used another assumption of infinite carrier mobility to obtain the conversion-efficiency limits. Effects of finite mobility can be incorporated into the present theory, if we introduce phenomenological parameters ti, which represent the probability that a photon absorbed in the subcell i produces an electron-hole pair available as short-circuit current, as was included in the seminal paper by Shockley and Queisser [1] for single-junction cells. In the paper, we have assumed all of the surfaces and interfaces of multi-junction solar cells are flat. Randomly textured surfaces have been proposed to increase subcell external radiative efficiency [9]. For the randomly textured multi-junction solar cells, we should change absorptivity expression mentioned in [13].

4. Conclusion

In conclusion, we studied the theoretical efficiency limit ηsc and subcell bandgap energies including their dependence on the geometric mean ηint* of all the subcells’ internal radiative efficiencies ηint in the multi-junction solar cells with no, air-gap and perfect intermediate reflectors. We confirmed that ηint* is a very useful parameter that summarizes ηint of all the subcells with ηint <0.3 and that ηsc calculated for ηint1 = ηint2 = … = ηintn represents ηsc for arbitrary combinations of (ηint1, ηint2, …, ηintn) giving the same ηint*. As ηint* decreases from 1 to 0.1, the efficiency limit ηsc of the three versions of cells decrease drastically. Semi-logarithmic relationships were found between ηsc and ηint* for ηint* below 0.1. Differently from the case with the well-investigated ideal multi-junction solar cells, the intermediate reflectors no longer boost ηsc of the practical thick multi-junction solar cells with ηint* less than 0.1. The optimized bandgap energies were obtained for finite ηint* below 1, which were significantly blue-shifted from those within the radiative limit (ηint* = 1) and affected by the edges of AM1.5 solar-spectrum gaps. We found that high ηsc are possible for 2- and 3- junction cells with realistic materials with low ηint*, if we chose the optimized designs obtained in this work. Our present results provide realistic efficiency targets and design principles for multi-junction solar cells made of realistic subcell materials.

Acknowledgments

This work was partly supported by JST-CREST, JSPS KAKENHI (No. 26610081, 26390075), the Photon Frontier Network Program of MEXT, JST-SENTAN, L.Z. was awarded a scholarship to pursue a PhD degree through a rigid academic evaluation process organized by the China Scholarship Council.

References and links

1. lW. Shockley and H. J. Queisser, “Detailed balance limit of efficiency of p-n junction solar cells,” J. Appl. Phys. 32(3), 510–519 (1961). [CrossRef]  

2. A. D. Vos, “Detailed balance limit of the efficiency of tandem solar cells,” J. Phys. D Appl. Phys. 13(5), 839–846 (1980). [CrossRef]  

3. C. H. Henry, “Limiting efficiencies of ideal single and multiple energy gap terrestrial solar cells,” J. Appl. Phys. 51(8), 4494–4500 (1980). [CrossRef]  

4. A. S. Brown and M. A. Green, “Detailed balance limit for the series constrained two terminal tandem solar cell,” Physica E 14(1), 6–100 (2002).

5. A. Martí and G. L. Araujo, “Limiting efficiencies for photovoltaic energy conversion in multigap systems,” Sol. Energy Mater. Sol. Cells 43(2), 203–222 (1996). [CrossRef]  

6. I. Tobías and A. Luque, “Ideal efficiency of monolithic, series-connected multijunction solar cells,” Prog. Photovolt. Res. Appl. 10(5), 323–329 (2002). [CrossRef]  

7. S. Kurtz, D. Myers, W. E. McMahon, J. Geisz, and M. Steiner, “A comparison of theoretical efficiencies of multi-junction concentrator solar cells,” Prog. Photovolt. Res. Appl. 16(6), 537–546 (2008). [CrossRef]  

8. A. S. Brown and M. A. Green, “Limiting efficiency for current-constrained two-terminal tandem cell stacks,” Prog. Photovolt. Res. Appl. 10(5), 299–307 (2002). [CrossRef]  

9. V. Ganapati, C.-S. Ho, and E. Yablonovitch, “Air gaps as intermediate selective reflectors to reach theoretical efficiency limits of multibandgap solar cells,” IEEE J. Photovoltaics 5(1), 410–417 (2015). [CrossRef]  

10. M. A. Green, “Radiative efficiency of state-of-the-art photovoltaic cells,” Prog. Photovolt. Res. Appl. 20(4), 472–476 (2012). [CrossRef]  

11. M. A. Green, K. Emery, Y. Hishikawa, W. Warta, and E. D. Dunlop, “Solar cell efficiency tables (Version 45),” Prog. Photovolt. Res. Appl. 23(1), 1–9 (2015). [CrossRef]  

12. N. L. A. Chan, N. J. Ekins-Daukes, J. G. J. Adams, M. P. Lumb, M. Gonzalez, P. M. Jenkins, I. Vurgaftman, J. R. Meyer, and R. J. Walters, “Optimal bandgap combinations—does material quality matter?” IEEE J. Photovoltaics 2(2), 202–208 (2012). [CrossRef]  

13. O. D. Miller, E. Yablonovitch, and S. R. Kurtz, “Strong internal and external luminescence as solar cells approach the Shockley-Queisser limit,” IEEE J. Photovoltaics 2(3), 303–311 (2012). [CrossRef]  

14. O. D. Miller, “Photonic design: From fundamental solar cell physics to computational inverse design,” Ph.D. dissertation, Dept. Elect. Eng. Comput. Sci., Univ. Calif., Berkeley, CA, USA, (2012).

15. O. D. Miller and E. Yablonovitch, “Detailed balance solar cell efficiency limits for internal fluorescence yield slightly less than 100%,” Optics for Solar Energy (OSA, 2010).

16. E. Yablonovitch and G. D. Cody, “Intensity enhancement in textured optical sheets for solar cells,” IEEE Trans. Electron Dev. 29(2), 300–305 (1982). [CrossRef]  

17. E. Yablonovitch, “Statistical ray optics,” J. Opt. Soc. Am. 72(7), 899–907 (1982). [CrossRef]  

18. I. Schnitzer, E. Yablonovitch, C. Caneau, and T. J. Gmitter, “Ultrahigh spontaneous emission quantum efficiency, 99.7% internally and 72% externally, from AlGaAs/GaAs/AlGaAs double heterostructures,” Appl. Phys. Lett. 62(2), 131–133 (1993). [CrossRef]  

19. L. Zhu, C. Kim, M. Yoshita, S. Chen, S. Sato, T. Mochizuki, H. Akiyama, and Y. Kanemitsu, “Impact of sub-cell internal luminescence yields on energy conversion efficiencies of tandem solar cells: A design principle,” Appl. Phys. Lett. 104(3), 031118 (2014). [CrossRef]  

20. S. Chen, L. Zhu, M. Yoshita, T. Mochizuki, C. Kim, H. Akiyama, M. Imaizumi, and Y. Kanemitsu, “Thorough subcells diagnosis in a multi-junction solar cell via absolute electroluminescence-efficiency measurements,” Sci. Rep. 5, 7836 (2015). [CrossRef]   [PubMed]  

21. O. D. Miller, “Photonic design: From fundamental solar cell physics to computational inverse design.” arXiv preprint arXiv:1308.0212 (2013).

22. M. A. Steiner, J. F. Geisz, I. Garcia, D. J. Friedman, A. Duda, and S. R. Kurtz, “Optical enhancement of the open-circuit voltage in high quality GaAs solar cells,” J. Appl. Phys. 113(12), 123109 (2013). [CrossRef]  

23. The lower bounds of ηext and ηint exist, which stem from neglect of thermal emission against luminescence, or Eg >> -kTclnηext .

24. Website of the National Renewable Energy Laboratory in the United States, “Best research-cell efficiencies” (2016). http://www.nrel.gov/ncpv/images/efficiency_chart.jpg

25. M. Yamaguchi, K. I. Nishimura, T. Sasaki, H. Suzuki, K. Arafune, N. Kojima, Y. Ohsita, Y. Okada, A. Yamamoto, T. Takamoto, and K. Araki, “Novel materials for high-efficiency III-V multi-junction solar cells,” Sol. Energy 82(2), 173–180 (2008). [CrossRef]  

26. W. Guter, R. Kern, W. Köstler, T. Kubera, R. Löckenhoff, M. Meusel, M. Shirnow, and G. Strobl, “III-V multijunction solar cells–new lattice-matched products and development of upright metamorphic 3J cells,” AIP Conf. Proc. 1407(1), 3658282 (2011).

27. M. S. Leite, R. L. Woo, J. N. Munday, W. D. Hong, S. Mesropian, D. C. Law, and H. A. Atwater, “Towards an optimized all lattice-matched InAlAs/InGaAsP/InGaAs multijunction solar cell with efficiency> 50%,” Appl. Phys. Lett. 102(3), 033901 (2013). [CrossRef]  

28. F. Dimroth, C. Baur, A. W. Bett, M. Meusel, and G. Strobl, “3-6 junction photovoltaic cells for space and terrestrial concentrator applications,” in Photovoltaic Specialists Conference (IEEE, 2005), pp. 525–529. [CrossRef]  

29. T. N. Tibbits, P. Beutel, M. Grave, C. Karcher, E. Oliva, G. Siefer, A. Wekkeli, M. Schachtner, F. Dimroth, and A. W. Bett, “New efficiency frontiers with wafer-bonded multi-junction solar cells,” in Proceedings of the 29th European Photovoltaic Solar Energy Conference and Exhibition (2014), pp. 1-4.

30. J. F. Geisz, M. A. Steiner, I. García, S. R. Kurtz, and D. J. Friedman, “Enhanced external radiative efficiency for 20.8% efficient single-junction GaInP solar cells,” Appl. Phys. Lett. 103(4), 041118 (2013). [CrossRef]  

31. M. Y. Feteha and G. M. Eldallal, “The effects of temperature and light concentration on the GaInP/GaAs multijunction solar cell’s performance,” Renew. Energy 28(7), 1097–1104 (2003). [CrossRef]  

32. K. Nishioka, T. Takamoto, T. Agui, M. Kaneiwa, Y. Uraoka, and T. Fuyuki, “Evaluation of temperature characteristics of high-efficiency InGaP/InGaAs/Ge triple-junction solar cells under concentration,” Sol. Energy Mater. Sol. Cells 85(3), 429–436 (2005). [CrossRef]  

33. K. Nishioka, T. Takamoto, T. Agui, M. Kaneiwa, Y. Uraoka, and T. Fuyuki, “Annual output estimation of concentrator photovoltaic systems using high-efficiency InGaP/InGaAs/Ge triple-junction solar cells based on experimental solar cell’s characteristics and field-test meteorological data,” Sol. Energy Mater. Sol. Cells 90(1), 57–67 (2006). [CrossRef]  

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Figures (5)

Fig. 1
Fig. 1 Structures of the multi-junction solar cells considered in this work (a) no intermediate reflectors, (b) with perfect intermediate reflectors (PIR) and (c) with air-gap intermediate reflectors. All of three versions of solar cells have planar surfaces, perfect front-surface AR coating on topmost cell and perfect rear mirror in bottommost cell.
Fig. 2
Fig. 2 (a) The efficiency ηsc and (b) optimized Eg set of 3-junction solar cells without intermediate reflectors as function of ηint* under various combinations of (ηint1, ηint2, ηint3). Black, red, blue, and green curves in (a) respectively represent the values of η sc at the case of ηint1 = ηint2 = ηint3, ηint2 = ηint3 = 0.3, ηint1 = ηint3 = 0.3, and ηint1 = ηint2 = 0.3. Circles, triangles, inverted triangles and squares represent more than 15 random combinations of (ηint1, ηint2, ηint3) that independently vary between 0.3 and 10−10 but their geometric means ηint* are fixed as 0.1, 0.01, 0.001, and 0.0001, which were amplified in (c)-(f).
Fig. 3
Fig. 3 The optimized efficiency ηsc [%] of multi-junction solar cells with no (dashed curves), air-gap (dotted curves) and perfect intermedium reflectors (solid curves) as function of junction number at various values of ηint* = 10−5, 10−3, 0.1, and 1 for (a) α sun ¯ l = 5 and α lumi ¯ l = 1 (1-sun), (b) α sun ¯ l = 5 and α lumi ¯ l = 1 (1000-sun), (c) α sun ¯ l = 5 and α lumi ¯ l = 2 (1-sun) and (d) α sun ¯ l = 2 and α lumi ¯ l = 1 (1-sun).
Fig. 4
Fig. 4 The efficiency η sc of 3-junction solar cells with no (dashed curves), air-gap (dotted curves) and perfect intermedium reflectors (solid curves) at η int * fixed as 1, 0.1, and 0.001 as function of a lumi ¯ l for (a) a sun ¯ l = 5 and (b) a sun ¯ l = 2.
Fig. 5
Fig. 5 The optimized set of bandgaps E gi [eV] as function of junction number at various values of η int * = 0.00001~1, for α sun ¯ l = 5 and α lumi ¯ l = 1 under (a) AM1.5G (1-sun) and (b) AM1.5D (1000-sun).

Equations (6)

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α suni ¯ = E gi E gi1 or α(E) ϕ sun (E)dE E gi E gi1 or ϕ sun (E)dE and α lumii ¯ = E gi α(E) ϕ lumi (E)dE E gi ϕ lumi (E)dE ,
{ J/q = R sun ( E g1 ,) R ext1 ( E g1 ,, V 1 )[( 1 η int1 1) 4 α lumi1 ¯ l 1 n 1 2 a lumi1 ¯ +(1+ n i 2 )],(a) J/q = R sun ( E gi , E gi1 )+ n i1 2 R exti1 ( E gi1 ,, V i1 ) R exti ( E gi ,, V i )[( 1 η inti 1) 4 α lumii ¯ l i n i 2 a lumii ¯ +(1+ n i 2 )] (i=2,3,..n1),(b) J/q = R sun ( E gn , E gn1 )+ n n1 2 R extn1 ( E gn1 ,, V n1 ) R extn ( E gn ,, V n )[( 1 η intn 1) 4 α lumin ¯ l n n n 2 a lumin ¯ +1],(c)
{ J/q = R sun ( E g1 ,) R int1 ( E g1 ,, V 1 )[( 1 η int1 1)+ a lumi1 ¯ 4 α lumi1 ¯ l 1 n 1 2 (1+ n 1 2 )],(a) J/q = R sun ( E gi , E gi1 )+ n i1 2 R exti1 ( E gi1 ,, V i1 ) R inti ( E gi ,, V i )[( 1 η inti 1)+ a lumii ¯ 4 α lumii ¯ l i n i 2 (1+ n i 2 )] (i=2,3,..n1),(b) J/q = R sun ( E gn , E gn1 )+ n n1 2 R extn1 ( E gn1 ,, V n1 ) R intn ( E gn ,, V n )[( 1 η intn 1)+ a lumin ¯ 4 α lumin ¯ l n n n 2 ],(c)
J/q = R sun ( E gi , E gi1 )+ R exti1 ( E gi1 ,, V i1 ) R exti ( E gi ,, V i )[( 1 η inti 1) 4 α lumii ¯ l i n i 2 a lumii ¯ +2],
and J/q = R sun ( E gi , E gi1 ) R exti ( E gi ,, V i )[( 1 η inti 1) 4 α lumii ¯ l i n i 2 a lumii ¯ +1], respectively.
η sc ( η int1 , η int2 ,, η intn )= Max E g1 , E g2 E gn i=1 n I V i P in .
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