Microscopic structure of a VH4 center trapped by C in Si

Chao Peng, Haoxiang Zhang, Michael Stavola, W. Beall Fowler, Benjamin Esham, Stefan K. Estreicher, Andris Docaj, Lode Carnel, and Mike Seacrist
Phys. Rev. B 84, 195205 – Published 28 November 2011

Abstract

The Si materials typically used to fabricate solar cells often contain high concentrations of carbon and hydrogen impurities. One of the more thermally stable defects in Si that contains both C and H gives rise to a Si-H vibrational line at 2184.3 cm1. We show that this center also gives rise to additional weak Si-H and C-H lines at 2214.4 and 2826.9 cm1 (4.2 K). When D is partially substituted for H, rich isotopic splittings of these IR lines are produced. An analysis of these data reveals that the 2184.3, 2214.4, and 2826.9 cm1 lines are due to a VH4 defect bound to a substitutional C impurity, i.e., a VH3-HC center.

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  • Received 9 September 2011

DOI:https://doi.org/10.1103/PhysRevB.84.195205

©2011 American Physical Society

Authors & Affiliations

Chao Peng1, Haoxiang Zhang1, Michael Stavola1,*, W. Beall Fowler1, Benjamin Esham1,†, Stefan K. Estreicher2, Andris Docaj2, Lode Carnel3, and Mike Seacrist4

  • 1Department of Physics and the Sherman Fairchild Laboratory, Lehigh University, Bethlehem, Pennsylvania 18015, USA
  • 2Texas Tech University, Lubbock, Texas 79409, USA
  • 3REC Wafer AS, NO-3908 Porsgrunn, Norway
  • 4MEMC Electronic Materials, St. Peters, Missouri 63376, USA

  • *michael.stavola@lehigh.edu
  • Present address: Department of Physics, University of Illinois at Urbana-Champaign, Urbana, IL 61801.

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Issue

Vol. 84, Iss. 19 — 15 November 2011

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