2014
DOI: 10.1149/2.0141411jss
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Morphology of Oxygen Precipitates in RTA Pre-Treated Czochralski Silicon Wafers Investigated by FTIR Spectroscopy and STEM

Abstract: We used STEM and FTIR to investigate the morphology and stoichiometry of oxygen precipitates in samples pre-treated by RTA at 1250°C subsequently annealed in the temperature range between 800°C and 1000°C. The morphology of the oxygen precipitates depends on the temperature of the subsequent annealing. Annealing at 800°C results first of all in the formation of three dimensional dendritic precipitates while during annealing at 900°C or 1000°C mainly plate-like and octahedral precipitates are formed. The absorp… Show more

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Cited by 16 publications
(26 citation statements)
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“…11,21,[40][41][42] In fact, this can be very well explained based on the effective medium theory as it is shown in many works. 11,[13][14][15]17,21 The simulated absorption bands of the oxygen precipitates show a strong dependence on the morphology and stoichiometry of oxygen precipitates as it is shown in Fig. 7.…”
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confidence: 85%
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“…11,21,[40][41][42] In fact, this can be very well explained based on the effective medium theory as it is shown in many works. 11,[13][14][15]17,21 The simulated absorption bands of the oxygen precipitates show a strong dependence on the morphology and stoichiometry of oxygen precipitates as it is shown in Fig. 7.…”
mentioning
confidence: 85%
“…First, we analyzed FTIR spectra by effective medium theory in the samples with different morphologies of oxygen precipitates. 17 The important parameters for the calculations like the morphology and the size of precipitates were also measured by scanning transmission electron microscopy (STEM). In most cases, we obtained amorphous SiO 2 as the phase of the oxygen precipitates.…”
mentioning
confidence: 99%
“…Apparently, its aspect ratio is larger than that of the platelet precipitate morphology related with the 1230 cm −1 band. Returning now to the analysis of our results, we have to state that all the evidence from various studies so far lead us to correlate the 1170 cm −1 band to platelet precipitates, although the 1060 and 1080 cm −1 bands to spheroidal precipitates [72][73][74][75][76]. The band at 1040 cm −1 is just outside the frequency range (1050-1150 cm −1 ) where spheroidal precipitate bands appear [72].…”
Section: Resultsmentioning
confidence: 86%
“…The analysis shows the existence of five additional bands at around 1000, 1040, 1060, 1080 and 1170 cm −1 . Notably, the bands found by the above analysis of the Lorentzian deconvolution are physically meaningful since there is ample experimental evidence, from various measurements also at low temperature, that the bands are related with oxygen precipitate morphologies [11][12][13][71][72][73][74][75][76]. Initially, we will discuss the origin of each particular band in an attempt A mathematical way to study the behavior of a precipitate is to consider its shape as an ellipsoid with three main axes (a 1 , a 2 , a 3 ).…”
Section: Resultsmentioning
confidence: 99%
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