TY - JOUR
T1 - Huge isotope effect on the vibrational lifetimes of an H2*(C) defect in Si
AU - Gibbons, T. M.
AU - Estreicher, S. K.
AU - Potter, K.
AU - Bekisli, F.
AU - Stavola, M.
PY - 2013/3/13
Y1 - 2013/3/13
N2 - The hydrogenation of C-rich Si leads to the formation of two (almost) energetically degenerate H2*(C) complexes, each containing one substitutional C (Cs) and two interstitial H atoms which are located at a bond-centered (bc) and an antibonding (ab) site, respectively. The two defects are trigonal: Cs-Hbc Si-Hab and H ab-Cs Hbc-Si. Fourier-transform infrared (FTIR) absorption spectra of these two defects should show two Cs-H and two Si-H stretch modes, but the Hab-Cs mode was absent in earlier studies. The missing line has now been observed by FTIR in especially C rich Si material. The line is unexpectedly broad, suggesting a very short vibrational lifetime. Partial D substitutions result in the formation of a Hab-Cs Dbc-Si center. In this defect, the Hab-Cs line shifts by only 0.3cm-1 but becomes very sharp, suggesting a long lifetime. The IR line widths show that the vibrational lifetime of the Hab-Cs mode in H ab-Cs Dbc-Si is about 16 times longer than that of the same Hab-Cs mode in Hab-Cs Hbc-Si. This paper contains experimental data and first-principles calculations which explain this isotope effect.
AB - The hydrogenation of C-rich Si leads to the formation of two (almost) energetically degenerate H2*(C) complexes, each containing one substitutional C (Cs) and two interstitial H atoms which are located at a bond-centered (bc) and an antibonding (ab) site, respectively. The two defects are trigonal: Cs-Hbc Si-Hab and H ab-Cs Hbc-Si. Fourier-transform infrared (FTIR) absorption spectra of these two defects should show two Cs-H and two Si-H stretch modes, but the Hab-Cs mode was absent in earlier studies. The missing line has now been observed by FTIR in especially C rich Si material. The line is unexpectedly broad, suggesting a very short vibrational lifetime. Partial D substitutions result in the formation of a Hab-Cs Dbc-Si center. In this defect, the Hab-Cs line shifts by only 0.3cm-1 but becomes very sharp, suggesting a long lifetime. The IR line widths show that the vibrational lifetime of the Hab-Cs mode in H ab-Cs Dbc-Si is about 16 times longer than that of the same Hab-Cs mode in Hab-Cs Hbc-Si. This paper contains experimental data and first-principles calculations which explain this isotope effect.
UR - http://www.scopus.com/inward/record.url?scp=84875360217&partnerID=8YFLogxK
U2 - 10.1103/PhysRevB.87.115207
DO - 10.1103/PhysRevB.87.115207
M3 - Article
AN - SCOPUS:84875360217
SN - 1098-0121
VL - 87
JO - Physical Review B - Condensed Matter and Materials Physics
JF - Physical Review B - Condensed Matter and Materials Physics
IS - 11
M1 - 115207
ER -