International Scholarly Research Notices

International Scholarly Research Notices / 2012 / Article

Research Article | Open Access

Volume 2012 |Article ID 862790 | 5 pages |

Limiting Solar Cell Heat-Up by Quantizing High Energy Carriers

Academic Editor: M. Zoulias
Received25 Apr 2012
Accepted03 Jun 2012
Published25 Jul 2012


Under solar radiation the efficiency of solar cells decreases as a result of heating up by short wavelengths photons. To minimize loss of efficiency with increasing temperatures, we designed a heterostructure AlGaAs/AlGaAs/GaAs cascaded p-i-n solar cells with 30 Å wide quantum wells and 10 Å wide barriers in p and i regions. Our modeling demonstrated that quantizing high energy carriers in the superlattice prevents scattering of excessive electron energies, thus decreasing the temperature rise per unit of time by a factor of 2. The modeling based on continuity equations included integration of absorption coefficients for various wavelengths and summarizes all thermodynamic heat exchanges in the designed solar cell.

1. Introduction

Effect of temperature on photovoltaic conversion has been a cause of much study for a long time. Rise in temperature does not significantly affect the light-generated current of the cell [1]. However, reverse saturation current increases exponentially with temperature. Furthermore, open circuit voltage reduces with temperature. It has been experimentally observed that the efficiency of a GaAs cell at 50°C drops by 10% from its efficiency at 28°C (i.e., 𝜂50=0.9𝜂28) [1]. It has been observed that the temperature of a c-Si cell array can reach up to about 55°C in about 25 minutes when exposed to a radiation of 1100 W/m2 [2]. It is imperative to reduce the heat build-up in the cell in order to improve conversion efficiencies.

It was established that the reason for heat build-up during cell operation is the generation of hot electrons [3]. Incident solar radiation is a combination of light of various wavelengths or photons of various energies. A semiconductor of band gap 𝐸𝑔 would absorb photons of energy equal to or higher than the band gap. Energy in excess of the band gap is utilized in exciting electrons and holes to higher energy levels. These carriers (hot carriers) eventually relax back to the band edges, thereby liberating the excess energy as heat. For this reason, higher band gap materials are said to generate less heat. Successful usage of various energy gaps was demonstrated in multijunction cascade solar cell structure with tunnel junction [4] and, more recently, in design of AlGaAs/GaAs cascade structure [5]. It has been proved that large band gaps improve the cell efficiency at higher temperature due to smaller temperature coefficients for reverse saturation current (dark current). Structures involving quantum well, quantum dots, and quantum wires possess quantized energy level that can accommodate high energy electron, thereby providing larger effective band gaps. Experimental results proved expected temperature effects in p-i-n GaAs/AlGaAs QW solar cell for well periods of 23 and 40 in [6]. It has been observed that the cell with 40 QWs exhibits enhanced performance when compared to similar cells of well or barrier material.

In this study we demonstrate that performance of the solar cell can be improved by reducing the heat generated by hot carries. We use thermodynamic modeling in predicting the temperature rise in AlGaAs/AlGaAs/GaAs cascade p-i-n structure [5] under solar irradiance of AM1.5. We propose a model based on quantization and continuity equation to calculate photocurrent for a superlattice structure. We also show that use of superlattice structure would reduce the temperature rise in the cell. Section 1 elucidates the theoretical framework. The parameters of the p-i-n cascade cell are described in Section 2. In Section 3, we discuss the effect of QWs in p and i regions of the designed structure. Simulation results are presented in Section 4.

2. Theory

Consider a semiconductor material of band gap 𝐸𝑔. When this material is exposed to a photon of energy 𝑣>𝐸𝑔, carriers are excited to energy levels above band edges as in Figure 1. Eventually, these energetic carriers heat up the material though scattering mechanism. The heat energy that would be dissipated due to carrier relaxation following photon absorption is (it is assumed that all the excess energy is converted into thermal energy) given in (1): Δ𝐸=Δ𝐸𝑒+Δ𝐸=𝑣𝐸𝑔eV.(1) If ΔΦ𝜆 is the photon flux (#/m2s) absorbed by the material, then the total power (density) dissipated as heat due to carrier scattering is given by (2): 𝑃𝐻𝜆=Δ𝐸𝑒+Δ𝐸ΔΦ𝜆=Δ𝐸Φ0𝜆1𝑒𝛼𝜆𝑊𝑊𝑚2,(2) where Φ0𝜆-photon flux (at wavelength 𝜆) at the surface, 𝑊-thickness, 𝛼𝜆-absorption coefficient.

Thus, power dissipated in heat due to carrier scattering in a heterostructute (multilayer) structure is given in (3): 𝑃𝐻𝜆=𝑘Δ𝐸𝑒𝑘+Δ𝐸𝑘𝜙0𝜆𝑒𝑚𝑘1𝛼𝑚𝜆𝑊𝑚1𝑒𝛼𝑘𝜆𝑊𝑘𝑊𝑚2,(3) where Δ𝐸𝑒𝑘, Δ𝐸𝑘-Electron energy above conduction band and hole energy above valance band in  𝑘th layer, respectively, 𝑊𝑘-thickness of  𝑘th layer, 𝛼𝑘𝜆-absorption coefficient of  𝑘th layer.

This heat is utilized in increasing the temperature of the materials. From basic laws of thermodynamics, the total thermodynamic power density required to raise the temperature of a multijunction cell though Δ𝑇 is given in (4): 𝑃𝐻=Δ𝑇Δ𝑡𝑛𝑘=1𝜌𝑘𝑊𝑘𝐶𝑘,(4) where 𝑚𝑘, 𝜌𝑘, 𝐶𝑘-mass, density and specific heat of material in  𝑘th layer. From (3) and (4), the rate of temperature rise is given by (5): Δ𝑇=𝑃Δ𝑡𝐻𝜆𝑛𝑘=1𝜌𝑘𝑊𝑘𝐶𝑘.(5) The photon flux at any given wavelength can be calculated from the solar spectrum data. In the present case, solar spectrum data for AM1.5 was utilized.

3. Solar Cell Design

3.1. 𝐼-𝑉  Characteristics

We designed a pin cascade solar cell with and without superlattices in p and i regions to address heating issues. First we consider the solar cell without superlattices (Figure 2). The materials for p-i-n regions were Al0.43Ga0.57As/Al0.25Ga0.75As/GaAs, respectively. The p-i-n thicknesses were 0.1 𝜇m, 4 𝜇m, and 2 𝜇m, respectively. The doping in p and n regions was 1018/cm3.

The dark current for such a cell would be the reverse saturation diode current. Forward currents in p, i, and n regions were calculated by solving the continuity equation in each region [7]. The total current in each region is created by photogeneration of wavelengths above the band gap and is defined by (6): 𝐽=𝜆0𝐽𝜆𝑑𝜆=1.24/𝐸𝑔𝑝0𝐽𝑝+(𝜆)𝑑𝜆1.24/𝐸𝑔𝑖0𝐽𝑖(𝜆)𝑑𝜆+1.24/𝐸𝑔𝑛0𝐽𝑛(𝜆)𝑑𝜆,(6) where 𝐽-total current density, 𝐽p,i,n-Current contribution from p, i, and n regions at a wavelength 𝜆. This gives a current density of 24.6 mA/cm2. With the open circuit voltage of 1.04 V the efficiency was 25%. 𝐼-𝑉 characteristics are given in Figure 3.

3.2. Thermal Calculation

The power dissipated in heat is given by (5) for subindex 𝑘=p,i,n.

4. Controlling High Energy Carriers

One-dimensional quantization of carriers can be achieved by superlattice built between high band gap and low band gap materials. The relative location of discrete energy levels from valance and conduction band edges was obtained by solving the Schrödinger wave equation for particles bounded by finite potential barriers. Finite difference method was used to convert the wave equation to a Hamiltonian matrix form. Eigenvalues of this matrix represent the energy levels, and the eigenvectors identify the wave function. The effective band gap of the region with quantum well would then be 𝐸𝑔+Δ𝐸𝑐𝑛+𝐸𝑣𝑛, where Δ𝐸𝑐𝑛 and Δ𝐸𝑣𝑛 are  𝑛th energy level inside the well from conduction and valance band edges, respectively. These energy distances would define the energy of the photon that can be absorbed in the well.

Quantum well dimensions in a superlattice were selected to provide sufficiently high energy levels for carriers. The barrier thickness of about 10 Å was chosen to ensure good quantum transparency. Aluminum phosphide (AlP) with a band gap of 3.57 eV was used as a barrier material in p and i regions. This resulted in barriers of potential 0.954 eV in conduction band and 0.636 eV in valance band, respectively. In i region, this was 1.08 eV in conduction band and 0.72 eV in valance band. A well width of 30 Å with 10 Å barriers resulted in 4 energy levels in conduction and valance bands in p and i regions. Well period was 23 and 998, respectively, in p and i regions. Due to narrow barrier thickness, these energy levels penetrate into adjoining well. Since all the wells were identical, the energy levels were identical, resulting in resonant tunneling through the region. We feel that QWs in n-region might not be required as most of the high energy photon absorption takes place in p and i regions.

4.1. Carrier Transport through Superlattices Structure

Carrier transport can be analyzed by using a particle through a potential barrier paradigm [8, 9]. Transmission and reflection for an electron at an energy level Δ𝐸𝑘 from a conduction band or valance band edges are related by (7): 𝑇𝑛0=𝑀𝑛1𝑅𝑛=𝑚11𝑚12𝑚21𝑚221𝑅,(7) where 1𝑀=4𝑒𝑖𝑘𝑤𝐿𝑏𝑒𝑖𝑘𝑤𝐿𝑏𝑒𝑖𝑘𝑤𝐿𝑏𝑒𝑖𝑘𝑤𝐿𝑏𝑒𝑘𝑏𝐿𝑏𝑒𝑘𝑏𝐿𝑏𝑖𝑘𝑏𝑘𝑤𝑒𝑘𝑏𝐿𝑏𝑖𝑘𝑏𝑘𝑤𝑒𝑘𝑏𝐿𝑏1𝑖𝑘𝑤𝑘𝑏1+𝑖𝑘𝑤𝑘𝑏1+𝑖𝑘𝑤𝑘𝑏1𝑖𝑘𝑤𝑘𝑏,𝑘(8)𝑤=2𝑚Δ𝐸𝑘,𝑘𝑏=2𝑚𝑉0Δ𝐸𝑘,(9)𝑉0-Barrier potential above band edge.

Tunneling probability through 𝑛-barriers is given by 𝑃𝑛=𝑇𝑛𝑇𝑛.

4.2. 𝐼-𝑉  Characteristics

The current in the QWSC was obtained by solving the continuity equation for carrier concentration in each well and barrier regions with boundary conditions 𝛿𝑛𝑘(𝑥𝑥0𝑘)=0. Here, 𝛿𝑛𝑘 is the carrier concentration in the  𝑘th well or barrier. The current contribution from  𝑘th well or barrier (Figure 4) is given by (10) 𝐽𝑘=𝑞𝑃𝑛𝑘𝐷𝑘𝑑𝛿𝑛𝑘,𝑑𝑥(10) where 𝐷𝑘-Diffusion coefficient of the material, 𝑃𝑛-𝑘-Probability of tunneling through 𝑛-𝑘 barriers obtained from Section 3.1.

Our model also took into account the fact that there would be no generation in barrier region for photons energies less than the barrier band gap. The wave nature of the electron would enable them to tunnel through the barriers. The presence of high field in i-region eliminates recombination. The current contribution in each region (at wavelength 𝜆) is the sum of current due to each well and barrier regions. The total current due to entire spectrum can be calculated from (7). It gave a current density of 18.3 mA and open circuit voltage of 1.1 V. The efficiency thus obtained was 20%.

4.3. Thermal Calculations

In the presence of QWs, the amount of heat dissipated in each region is given by (11): 𝑃𝐻𝜆=𝑘=0Δ𝐸𝑒𝑐𝑘+Δ𝐸𝑐𝑘𝜙0𝑘1𝑒𝛼𝑘𝜆𝑊𝑘𝑊𝑚2,(11) where Δ𝐸𝑒𝑐𝑘+Δ𝐸𝑐𝑘𝐸=𝑣𝑔+Δ𝐸𝑐+Δ𝐸𝑣,𝜙0𝑘=𝜙0e𝑘1𝑚=1𝛼𝑚𝑊𝑚.(12) Here Δ𝐸𝑐, Δ𝐸𝑣 is the energy level below the electron energy in the conduction band and energy level below the hole energy in the valance band, respectively, 𝛼𝑘-absorption coefficient of  𝑘th region and 𝑊𝑘-thickness of the  𝑘th region. Here, the high energy carriers settle on closest quantized energy level provided by the superlattice structure. Our modeling also took into account heat-up due to this small energy loss.

5. Modeling and Results

In our modeling, absorption coefficient is not a constant but a function of wavelengths for AM1.5 solar spectrum obtained from [10]. Superlattices in p and i regions were included to prevent scattering of high energy electrons. However, we did not consider energy scattering in contact areas. This is because they are very thin, and carriers will not have sufficient time to reduce their energies while traversing the contacts; thus recombination heating was not considered.

Our modeling assumed that QW energy levels in p and i regions were not aligned before illumination. Under solar radiation, the built-in potential step of p-i-n junction will be eliminated, thereby aligning the energy levels in p and i regions. This ensures carrier tunneling and transport across the junction.

Temperature increase for each wavelength of incident photon was calculated using the theory presented in Section 1 through 3 for cases with and without quantum wells, respectively. Figure 5(a) presents the distribution of temperature increase caused by photons of different wavelengths. It is clear that photons of energy about 2.5 eV (490 nm) bring about maximum temperature rise. The cumulative impact is presented by summation of all temperature rises. With no superlattices, the cumulative increase of temperature per unit of time is 8°C/s. As a result, the heating up by energetic carriers would attain a thermodynamic equilibrium at some temperature above the ambient temperature. However, the time to reach this equilibrium is not a concern of our modeling.

Designing superlattices in a, p, and i regions of our solar cell demonstrated that high energy carriers, having an option to occupy certain energy levels provided by our design, become less harmful as far as cell heating is considered. While analyzing the effect of quantum wells on temperature rise, it was assumed that the photons of energies lying within the gaps between the discrete energy levels would excite the charge carriers to energy levels just below such a gap. Figure 5(b) shows the temperature distribution when p and i regions are superlattice structures. The cumulative temperature rise is about 4°C/s.

Clearly, there is significant reduction in the temperature rise. The 10 Å width barriers would ensure quantum tunneling of electrons through the barrier. The wider band gap also ensured that the barriers were optically inactive.

6. Conclusion

A formalized approach has been presented to assess the heating impact of high energy carriers. Modeling of current in superlattice structures for a solar cell under illumination was also proposed. Modeling shows that heat-up per unit of time was 8.5°C/s with no quantum wells (cumulative) for a p-i-n heterostructure solar cell. As a remedy to solar cell heating, we designed superlattice structure with 30 Å wide quantum wells and 10 Å wide barriers in p and i regions. The modeling shows that the cumulative temperature rise per unit of time of operational solar cell equipped with superlattices was about 4°C/s. This implies a reduction of heating up per unit of time by a factor 2. Modeling results also indicate reduction in current with the inclusion of quantum wells. This was expected as there would be no carrier generation inside barriers by photons with longer wavelengths. However, such a reduction can be remedied by increasing the thickness of the p and i regions. Our design ensures enhanced performance of a solar cell as reduction in heat-up leads to higher efficiency.


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Copyright © 2012 L. Devarakonda and S. Mil'shtein. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

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