Silicon meets group-II metals in energy and electronic applications—How to handle reactive sources for high-quality films and bulk crystals

Author:

Suemasu T.1ORCID,Hara K. O.2ORCID,Udono H.3ORCID,Imai M.4ORCID

Affiliation:

1. Faculty of Pure and Applied Sciences, Department of Applied Physics, University of Tsukuba, Tsukuba, Ibaraki 305-8573, Japan

2. Center for Crystal Science and Technology, University of Yamanashi, Kofu, Yamanashi 400-8511, Japan

3. Department of Electrical and Electronic Engineering, Ibaraki University, Hitachi, Ibaraki 316-8511, Japan

4. Research Center for Functional Materials, National Institute for Materials Science, Tsukuba, Ibaraki 305-0047, Japan

Abstract

In the present advanced information society, the group IV element Si is inevitably used for various high-performance devices, such as transistors and solar cells. When Si meets group-II elements such as Mg, Ca, Sr, or Ba, semiconducting silicides are formed, which are applicable to energy conversion devices such as thin-film solar cells and thermoelectric devices. In this Tutorial, we focus on two representative typical semiconducting silicides among them: Mg2Si and BaSi2 composed of earth-abundant elements. Mg2Si has been extensively studied for light-weight high-performance thermoelectric devices, whereas BaSi2 has been studied for thin-film solar cells, and recently has also been attracting attention as a thermoelectric material. However, these group-II elements are highly reactive with oxygen and water. Thus, we need to be careful when handling these elements. In this Tutorial, we provide guidance on how to handle these group-II elements and their compounds in an easy-to-understand manner for beginners. In addition, we introduce thin-film growth and bulk growth techniques, as well as the points to be considered when characterizing these materials.

Funder

Japan Society for the Promotion of Science

Adaptable and Seamless Technology Transfer Program through Target-Driven R and D

Publisher

AIP Publishing

Subject

General Physics and Astronomy

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