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Impact of the magnetic field on solar cell parameters: A study using the conventional classical approach

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Abstract

In this work, we have developed a theoretical study based on the classical traditional approach. In fact, the application of the fundamental dynamics relationship in the steady-state regime, taking into account both friction and Lorentz forces, allowed us to determine the velocity components of charge carriers, namely, electrons and holes. By applying Ohm's law, we determined the matrix of electrical resistivity. Knowledge of the resistivity \({{\varvec{\rho}}}_{{\varvec{x}}{\varvec{x}}}\) in the direction of the current and the dimensions of the solar cell allowed us to determine the expression for longitudinal resistance RL as a function of the magnetic field B. Similarly, from the formula for resistivity \({{\varvec{\rho}}}_{{\varvec{y}}{\varvec{x}}}\), we determined the expression for transverse resistance RT as a function of B. A qualitative comparison between RT and RL shows that RT is negligible compared to RL. Consequently, we turned our attention to the impact of the magnetic field on RL, and our theoretical study revealed that it increases with the increase in B. Once this theoretical study has been proposed, it must undergo testing to ensure its validity. Therefore, it is subjected to two tests: one under illumination, for which we referred to the work of Dioari Ulrich Combari et al. (Adv Condens Matter Phys 18:1, 2018). To extract the parameters \({I}_{SC}\), \({I}_{0}\), \({R}_{S}\), \({R}_{Sh}\), n, and \({V}_{OC}\) of the cell, we employed our method of least squares (LMS). The other test is conducted in the dark and is carried out by El-Aasser et al. (Intern J Adv Appl 3:196, 2014) in the presence of a magnetic field B under both direct and indirect biasing conditions. Both tests demonstrate that our theoretical study is in perfect agreement with practical results. In fact, an increase in the intensity of the magnetic field beyond 1 millitesla (mT) automatically results in an increase in the series resistance RS, denoted as RL in our study. Ultimately, an increase in RS leads to a direct decrease in current, maximum power, and efficiency.

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Acknowledgements

We would like to express our gratitude to the research team led by D. Ulrich Combari and his collaborators, as well as to the research team led by M. El-Aasser and his collaborators, to use their experimental results to verify and validate our study. Their contribution has been of invaluable importance in advancing our research.

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Khalis, M., Masrour, R. Impact of the magnetic field on solar cell parameters: A study using the conventional classical approach. Indian J Phys (2023). https://doi.org/10.1007/s12648-023-03045-8

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