Optical characterization of hydrogenated silicon thin films using interference technique

Citation
T. Globus et al., Optical characterization of hydrogenated silicon thin films using interference technique, J APPL PHYS, 88(4), 2000, pp. 1907-1915
Citations number
38
Categorie Soggetti
Apllied Physucs/Condensed Matter/Materiales Science
Journal title
JOURNAL OF APPLIED PHYSICS
ISSN journal
00218979 → ACNP
Volume
88
Issue
4
Year of publication
2000
Pages
1907 - 1915
Database
ISI
SICI code
0021-8979(20000815)88:4<1907:OCOHST>2.0.ZU;2-M
Abstract
This work introduces an application of an "interference spectroscopy techni que" (IST) for determination of absorption coefficient and refractive index spectra of amorphous silicon (a-Si:H) and related thin film materials. The technique is based on computer analysis of measurements of optical transmi ssion and specular reflection (T & R) of thin films (including the films on substrates) over a wide range of the incident photon energies (0.5-2.8 eV) using carefully controlled spectrometer conditions. IST is used to investi gate the absorption spectrum in the sub-gap energy range (0.8-1.6 eV) of in trinsic and phosphorous-doped a-Si:H, "polymorphous-Si:H," and microcrystal line silicon films. The enhanced sensitivity of the technique over conventi onal analysis of T & R data results from utilization of interference to obt ain absorption coefficient values at the maxima of transmission. The factor s limiting the accuracy of the calculated absorption coefficient are discus sed in detail. Measurement on films of thickness ranging from 0.1 to 5 mu m identifies that the sub-gap absorption in these films arises from the bulk rather than the surface. A set of samples prepared under widely different conditions that appear to have overlapping (alpha=20 cm(-1)) sub-gap absorp tion spectra measured using photo-thermal deflection spectroscopy (PDS), re veal significant differences (alpha=10 to 100 cm(-1)) using IST. Changes (f actor of 2) in sub-gap absorption spectra due to light soaking are also cle arly observable using IST. (C) 2000 American Institute of Physics. [S0021-8 979(00)04116-5].