Investigation of veryintenseD3-band emission in multi-crystalline silicon wafers using electron microscopy and hyperspectral photoluminescence imaging

Author:

Thøgersen Annett1ORCID,Jensen Ingvild J. T.1,Graff Joachim S.1ORCID,Gudem Ringdalen Inga2,Almeida Carvalho Patricia1,Mehl Torbjørn3ORCID,Zhu Junjie4,Burud Ingunn3,Olsen Espen3,Søndenå Rune4ORCID

Affiliation:

1. SINTEF, Materials Physics, Forskningsveien 1, 0373 Oslo, Norway

2. SINTEF, Materials Physics, Høgskoleringen 5, 7034 Trondheim, Norway

3. Norwegian University of Life Sciences (NMBU), Institue of Physics, Universitetstunet 3, 1433 Ås, Norway

4. Institute for Energy Technology, Department of Solar Energy, Instituttveien 18, 2007 Kjeller, Norway

Abstract

Defects in high performance multi-crystalline silicon wafers can be detrimental to the lifetime of the solar cell. It is, therefore, important to study and understand the underlying structure and chemical elements present at these defective areas in order to suppress them. The underlying cause of the D-band emission line “[Formula: see text]” (VID3) has not yet been understood, although many theories have been proposed. In this paper, we have investigated the underlying causes of the d-band emission peak VID3 by hyperspectral photoluminescence imaging, scanning electron microscopy, electron backscatter diffraction, scanning transmission electron microscopy, and density functional theory (DFT) to understand the defect structure in areas of a VID3 emission peak in more detail. We found a high VID3 peak intensity at sub-grain and [Formula: see text] twin boundaries bordering to grains with a small misorientation, which suggests higher stress in these regions. Defects close to the twin boundary indicate a light element dopant in the area, such as oxygen. DFT calculations show that oxygen is prone to segregate to this boundary.

Funder

Norges Forskningsr�d

Publisher

AIP Publishing

Subject

General Physics and Astronomy

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