2002
DOI: 10.1063/1.1506422
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Craters on silicon surfaces created by gas cluster ion impacts

Abstract: Atomic force microscopy ͑AFM͒ and high-resolution transmission electron microscope ͑HRTEM͒ cross section imaging of individual gas cluster ion impact craters on Si͑100͒ and Si͑111͒ substrate surfaces is examined. The comparison between 3 and 24 kV cluster impacts from Ar and O 2 gas sources is shown. Results for low fluence (10 10 ions/cm 2 ) 24 kV Ar individual cluster impacts onto a Si͑100͒ and Si͑111͒ substrate surfaces are compared with hybrid molecular dynamics ͑HMD͒ simulations. A HMD method is used for … Show more

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Cited by 56 publications
(40 citation statements)
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“…The total fluence of 1.5 × 10 16 ions/cm 2 has ∼2,000 atoms associated with each charge measured by the Faraday cup. The increased thickness of the undulating surface oxide after GCIB processing may be due to the stochastic overlay of the individual GCIB-impact craters 7,14 or from the growth of a GCIB oxide along the initial, sinusoidal type of thickness variation. The surface oxides formed by GCIB processing have been examined by spectroscopic ellipsometry and XPS.…”
Section: Resultsmentioning
confidence: 99%
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“…The total fluence of 1.5 × 10 16 ions/cm 2 has ∼2,000 atoms associated with each charge measured by the Faraday cup. The increased thickness of the undulating surface oxide after GCIB processing may be due to the stochastic overlay of the individual GCIB-impact craters 7,14 or from the growth of a GCIB oxide along the initial, sinusoidal type of thickness variation. The surface oxides formed by GCIB processing have been examined by spectroscopic ellipsometry and XPS.…”
Section: Resultsmentioning
confidence: 99%
“…With use of a final O 2 -GCIB process step (such as in this study) on material that is able to react with oxygen, the post-GCIB material typically forms a thicker (more stoichiometric) oxide surface. 7,14 The XPS analysis of the Ga 3p peak is shown in Fig. 5 for the pre-and post-GCIB GaSb surface.…”
Section: Resultsmentioning
confidence: 99%
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“…A crystal surface, with an initial average surface roughness of tens or hundreds of angstroms, becomes atomically flat, with the residual roughness of a few angstroms [5,7,8,11]. The GCIB smoothing typically occurs after irradiation by an ionized Ar n (n $ 1000-10 000) cluster beam at a charge fluence of 10 14 -10 16 ions/cm 2 .…”
Section: Introductionmentioning
confidence: 99%