Recombination via transition metals in solar silicon: the significance of hydrogen-metal reactions and lattice sites of metal atoms

Jack Mullins, Simon Leonard, Vladimir Markevich, Ian Hawkins, P Santos, J. Coutinho, A Marinopoulos, D Murphy, Matthew Halsall, Anthony Peaker

    Research output: Contribution to journalArticlepeer-review

    Abstract

    The move towards lower cost sources of solar silicon has intensi-fied efforts to investigate the possibilities of passivating or reduc-ing the recombination activity caused by deep states associated with transition metals. This is particularly important for the case of the slow diffusing metals early in the periodic sequence which are not removed by conventional gettering. In this paper we examine reactions between hydrogen and transition metals and discuss the possibility of such reactions during cell processing. We analyse the case of hydrogenation of iron in p-type Si and show that FeH can form under non-equilibrium conditions. We consider the electrical activity of the slow diffusing metals Ti, V and Mo, how this is affected in the presence of hydrogen, and the stability of TM-H complexes formed. Finally we discuss recent experiments which indicate that re-siting of some transition metals from the interstitial to substitutional site is possible in the presence of excess vacancies, leading to a reduction in recombination activity.
    Original languageEnglish
    Article number1700304
    JournalPhysica Status Solidi. A: Applications and Materials Science
    Volume214
    Issue number7
    Early online date12 Jun 2017
    DOIs
    Publication statusPublished - 6 Jul 2017

    Keywords

    • solar silicon
    • non-radiative recombination
    • hydrogen
    • passivation
    • interstitial and substitutional transition metals

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