Increasing the absorption angle is a commonly used method to suppress this loss process. Non-radiative recombination loss and series loss are extremely significant for the high-concentration-ratio photovoltaic system, covering 15%–40% of the total incident solar energy for the cells with bandgap below 2.0 eV in the case of 100 suns.
Abstract To improve the performance of solar photovoltaic devices one should mitigate three types of losses: optical, electrical and thermal. However, further reducing the optical and electrical losses in modern photovoltaic devices is becoming increasingly costly. Therefore, there is a rising interest in minimizing the thermal losses.
Loss processes in solar cells consist of two parts: intrinsic losses (fundamental losses) and extrinsic losses. Intrinsic losses are unavoidable in single bandgap solar cells, even if in the idealized solar cells .
Dominant losses and parameters of affecting the solar cell efficiency are discussed. Non-radiative recombination loss is remarkable in high-concentration-ratio solar cells. Series resistance plays a key role in limiting non-radiative recombination loss.
Solar photovoltaic systems have made topical advances in the use of highly effective solar cell materials to achieve high efficiency. In this analysis, performance parameters are influenced by the internal and external conditions of the solar photovoltaic systems and they lead to an increase in the loss of the system.
Efficiency losses in the solar cell result from parasitic absorption, in which absorbed light does not help produce charge carriers. Addressing and reducing parasitic absorption is necessary to increase the overall efficiency and performance of solar cells (Werner et al., 2016a).