4.7 Article

A thin Cu interlayer-mediated control of phase evolution of Cu2ZnSnS4 thin films grown by RF magnetron sputtering of a single elementary target with high white light sensitivity

Journal

APPLIED SURFACE SCIENCE
Volume 539, Issue -, Pages -

Publisher

ELSEVIER
DOI: 10.1016/j.apsusc.2020.148149

Keywords

Kesterite; Sputtering; Thin films; Solar cells

Funding

  1. Department of Science and Technology, Government of India [EMR/2014/000217]
  2. Thapar Institute of Engineering and Technology, Patiala, India

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A rational strategy for phase-pure kesterite CZTS film deposition using RF magnetron sputtering with a thin Cu interlayer was demonstrated to suppress the growth of secondary phases. The films showed excellent photoresponse with a bandgap of 1.58 eV, making them suitable for potential use in thin film solar cells.
Although sputter deposition from a single target to prepare Cu2ZnSnS4 (CZTS) thin films appears attractive, it must suppress the growth of secondary phases that detrimentally affect performance of CZTS based thin film solar cells. Here we demonstrate a rational strategy for deposition of phase pure kesterite CZTS films by RF magnetron sputtering using a single target prepared from elemental powders via a thin Cu interlayer-mediated control of phase evolution. The films grown from a target of stoichiometric elemental proportion were Cu poor that determined the reaction pathway during sulfurization and resulted in growth of spurious phases despite a large variation in the sulfurization configuration. Inserting a 195 nm thick Cu interlayer between successively sputtered precursor layers provided improved compositional stability through thermally activated diffusion of Cu from the intermediate layer towards both the sides and resulted in the formation of kesterite CZTS even at a modest sulfurization temperature of 500 degrees C. The obtained phase-pure films have a bandgap of similar to 1.58 eV. The films show excellent photoresponse behavior characterized by increase in current by three orders of magnitude at a bias of 3 V upon white light illumination, typically that required for a potential absorber layer in thin film solar cells.

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