2006
DOI: 10.1016/j.susc.2006.07.009
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Binding sites for SiH2/Si(001): A combined ab initio, tight-binding, and classical investigation

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Cited by 8 publications
(9 citation statements)
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“…The adsorption processes paths found are almost all barrierless (no intermittent minima in the path), and depend largely on the SiO initial position relative to the surface. Four unique binding sites on the Si surface, the so-called ondimer, intrarow, interrow, and inchannel [32] are identified from the adsorbed geometries and the final configurations are classified accordingly. In Fig.…”
Section: Binding Sites Of Sio On the Si(1 0 0) Surfacementioning
confidence: 99%
“…The adsorption processes paths found are almost all barrierless (no intermittent minima in the path), and depend largely on the SiO initial position relative to the surface. Four unique binding sites on the Si surface, the so-called ondimer, intrarow, interrow, and inchannel [32] are identified from the adsorbed geometries and the final configurations are classified accordingly. In Fig.…”
Section: Binding Sites Of Sio On the Si(1 0 0) Surfacementioning
confidence: 99%
“…In addition to the optimized rotational parameters (A 0 , B 0 , and C 0 ) and the origin (T 00 ), fits including various combinations of the centrifugal distortion parameters were attempted. Only ∆ J K for theX 1 A ′ state and ∆ K and δ J for theà 1 A ′′ state were required. The difference between the observed and calculated transition wavenumbers given in Table I …”
Section: A Energies and Transition Frequenciesmentioning
confidence: 99%
“…Modelling the role of SiH 2 in the fabrication of amorphous silicon thin films and polycrystalline silicon has also attracted significant interest. [1][2][3][4][5][6] Motivated primarily by the desire to garner a fundamental understanding of the properties of this simplest of silicon containing polyatomic molecules, and in part by the desire to develop a real time, in situ SiH 2 monitoring scheme, there have been numerous reported experimental and theoretical [29][30][31][32][33][34][35][36][37][38][39][40][41][42][43][44][45][46][47][48] studies of gas-phase SiH 2 , and to a lesser extent SiD 2 . In addition, SiH 2 is predicted to be abundant in circumstellar envelopes of carbon rich stars 49 and has been tentatively identified 50,51 via the detection of the 1 11 -0 00 pure rotational transition.…”
Section: Introductionmentioning
confidence: 99%
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