Abstract

Abstract Due to the detrimental effects of boron (B) on the efficiency of silicon (Si) photovoltaic cells, complete boron removal from Si is necessary to produce solar grade Si (SoG–Si, with a maximum limit of 0.1 ppmw boron). Gas refining is a promising technique for boron removal from Si, in which the thermodynamic equilibrium never establishes. Hence, by starting from any B concentration in the melt, the required limit for SoG–Si will be achieved. This research is devoted to studying the refractory interactions’ effect with melt and the chamber atmosphere on boron removal. For this purpose, gas refining experiments were carried out in alumina and graphite crucibles with H2 and H2–3% H2O refining gases. Gas refining in Ar, He, and continuous vacuuming conditions were also carried out to study the effect of chamber atmosphere. The gas refining results are supported by the characterization of the evaporated species by molecular beam mass spectroscopy (MBMS) technique. The MBMS measurements indicated that the boron evaporation occurs by the formation of the volatile species BH x , BO y , and B z H x O y compounds. Most of these compounds are already known in the literature. However, HBO, HBOH, and AlBO (in the case of alumina refractories) were measured experimentally in this work. Results indicate that the evaporation of B in the form of AlBO x compounds leads to higher mass transfer coefficients for boron removal in alumina crucibles. Density-functional theory (DFT) and coupled cluster calculations are carried out to provide a thermodynamic database for the gaseous compounds in the H–B–O–Al system, including enthalpy, entropy, and C P values for 21 compounds.

Highlights

  • Among all the impurities that should be removed from Si to reach the solar grade Si (SoG–Si), boron (B) is one of the most harmful elements to exist, which will reduce the efficiency of the PV modules

  • Boron exists in the metallurgical grade Si (MG–Si) in tens of ppmw, while a maximum limit of only 0.1 ppmw is acceptable for SoG–Si

  • It is obvious that the kB in the experiment (5) is greater than the experiment (1). Both experiments were carried out at 1,500°C and with dry H2(g), but in alumina and graphite crucibles, respectively. These results are in good agreement with the molecular beam mass spectroscopy (MBMS) measurements where we showed that in the case of applying alumina crucibles new volatile compounds of B like AlBO+ evaporate from the melt surface, and the kinetics of the refining process could be accelerated in the alumina crucibles

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Summary

Introduction

Power production by photovoltaic (PV) panels has increased almost ten times over the past decade and will continue rising in the future [1–3]. The Si for PV applications must have a purity degree of 6N (99.9999%), known as solar grade Si (SoG–Si). Among all the impurities that should be removed from Si to reach the SoG–Si, boron (B) is one of the most harmful elements to exist, which will reduce the efficiency of the PV modules. Boron exists in the metallurgical grade Si (MG–Si) in tens of ppmw, while a maximum limit of only 0.1 ppmw is acceptable for SoG–Si. Most metallic impurities can be removed from MG–Si through the directional solidification technique – the last key step in ingot production for solar cells. Reliable methods are required for B removal from Si

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