E.E. Chaban
Alcatel-Lucent
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Featured researches published by E.E. Chaban.
Journal of Vacuum Science & Technology B | 1997
Marcus K. Weldon; V. E. Marsico; Yves J. Chabal; A. Agarwal; D. J. Eaglesham; J. Sapjeta; W. L. Brown; D. C. Jacobson; Y. Caudano; S. B. Christman; E.E. Chaban
We have investigated the fundamental mechanism underlying the hydrogen-induced exfoliation of silicon, using a combination of spectroscopic and microscopic techniques. We have studied the evolution of the internal defect structure as a function of implanted hydrogen concentration and annealing temperature and found that the mechanism consists of a number of essential components in which hydrogen plays a key role. Specifically, we show that the chemical action of hydrogen leads to the formation of (100) and (111) internal surfaces above 400 °C via agglomeration of the initial defect structure. In addition, molecular hydrogen is evolved between 200 and 400 °C and subsequently traps in the microvoids bounded by the internal surfaces, resulting in the build-up of internal pressure. This, in turn, leads to the observed “blistering” of unconstrained silicon samples, or complete layer transfer for silicon wafers joined to a supporting (handle) wafer which acts as a mechanical “stiffener.”
Applied Physics Letters | 1998
Marcus K. Weldon; M. Collot; Yves J. Chabal; V.C. Venezia; Aditya Agarwal; T. E. Haynes; D. J. Eaglesham; S. B. Christman; E.E. Chaban
Infrared spectroscopy and secondary ion mass spectrometry are used to elucidate the mechanism by which co-implantation of He with H facilitates the shearing of crystalline Si. By studying different implant conditions, we can separate the relative contributions of damage, internal pressure generation, and chemical passivation to the enhanced exfoliation process. We find that the He acts physically as a source of internal pressure but also in an indirect chemical sense, leading to the reconversion of molecular H2 to bound Si–H in “VH2-like” defects. We postulate that it is the formation of these hydrogenated defects at the advancing front of the expanding microcavities that enhances the exfoliation process.
Journal of Vacuum Science & Technology B | 1996
M. K. Weldon; Yves J. Chabal; D. R. Hamann; S. B. Christman; E.E. Chaban; L. C. Feldman
Silicon wafer bonding is achieved by joining two particle‐free silicon wafers and annealing to elevated temperatures (∼1100 °C). We have used multiple internal transmission infrared absorption spectroscopy to probe the interface between the wafers upon initial joining and also during subsequent annealing steps. For atomically flat hydrophobic wafers (H passivated), we observe a pronounced shift in the Si–H stretching frequency due to the physical interaction (van der Waals attraction) that occurs when the surfaces come into intimate contact. The hydrogen eventually disappears at high temperatures (1000 °C) and Si–Si bonds are formed between the two surfaces. For hydrophilic wafers (oxide passivated), we initially observe three to five monolayers of water at the interface (providing the initial attraction through H bonding), as well as the presence of hydroxyl groups that terminate the oxide at low temperature. Upon moderate heating (<400 °C), the water trapped at the interface dissociates and leads to the...
Surface Science | 1996
Marcus K. Weldon; V.E. Marsico; Yves J. Chabal; D.R. Hamann; S. B. Christman; E.E. Chaban
Abstract In this paper, we review our recent infrared studies of the fundamental physical and chemical processes occurring at the interface of bonded silicon wafers, as a function of surface preparation and annealing temperature. We present a brief overview of the practical aspects of silicon-wafer bonding and the techniques used to evaluate the interface integrity, which highlight the need for fundamental studies of the microscopic interface phenomena. Importantly, we show that the interface between two silicon wafers approximates an ideal spectroscopic environment, in that there is a 28-fold enhancement in the sensitivity to the normal component of the interface absorption over any other surface optical geometry. Furthermore, the interface region is almost infinitely stable at room temperature, but can exhibit partial pressures ranging from near vacuum to several atmospheres upon annealing. We present results for two distinct types of wafer bonding: hydrophobic (hydrogen-terminated) and hydrophilic (oxide-terminated), since the origin of the initial attraction between the opposing surfaces is quite different in the two cases. Specifically, we show that ideally hydrogen-terminated Si(111) surfaces come within a few A, under the influence of a Van der Waals attraction, as evidenced by a pronounced perturbation of the isolated SiH stretch mode. In contrast, the initial attraction between hydrophilic surfaces is via hydrogen bonding, which is mediated by the presence of 2–4 monolayers of water that are trapped at the interface upon room-temperature joining. We demonstrate that vibrational spectroscopy provides unprecedented mechanistic insight into the thermal evolution of the molecular interface, which necessarily has a profound influence on the bonding process. Throughout the paper, emphasis is given to the need for a wide variety of additional (fundamental) studies of the surface phenomena occurring in these novel, technologically important systems.
Journal of Chemical Physics | 1997
Joseph Eng; Krishnan Raghavachari; Lisa M. Struck; Yves J. Chabal; Brian E. Bent; George W. Flynn; S. B. Christman; E.E. Chaban; Gwyn P. Williams; K. Radermacher; S. Mantl
The adsorption of ethanol-d0, -d3, and -d6 on Si(100) has been studied in the mid- to far-infrared region using surface infrared absorption spectroscopy. The acquisition of infrared spectra in this frequency range (<1450 cm−1) is made possible by using specially prepared Si(100) wafers which have a buried metallic CoSi2 layer that acts as an internal mirror. We find that ethanol dissociatively adsorbs across the Si(100) dimers near room temperature to form surface bound hydrogen and ethoxy groups. Furthermore, the ethoxy groups are oriented such that the C3v axis of the methyl group is nearly perpendicular to the surface, unlike the case for ethoxy groups bound to metal surfaces. This adsorption geometry is deduced on the basis of the surface dipole selection rule, which applies to these Si(100) samples with a buried CoSi2 layer. Ab initio cluster calculations using gradient-corrected density functional methods confirm the proposed adsorption geometry for ethoxy on Si(100) and accurately reproduce the obs...
Surface Science | 1997
L.M. Struck; Joseph Eng; Brian E. Bent; George W. Flynn; Yves J. Chabal; S. B. Christman; E.E. Chaban; Krishnan Raghavachari; Gwyn P. Williams; K. Radermacher; S. Mantl
Abstract The vibrational spectrum of water dissociatively adsorbed on Si(100) surfaces is obtained with surface infrared absorption spectroscopy. Low frequency spectra ( −1 are acquired using a buried CoSi 2 layer as an internal mirror to perform external reflection spectroscopy. On clean Si(100), water dissociates into H and OH surface species as evidenced by EELS results [1] in the literature which show a SiH stretching vibration (2082 cm −1 ), and SiOH vibrations (OH stretch at 3660 cm −1 and the SiOH bend and SiO stretch of the hydroxyl group centered around 820 cm −1 ). In this paper, infrared (IR) measurements are presented which confirm and resolve the issue of a puzzling isotopic shift for the SiO mode of the surface hydroxyl group, namely, that the SiO stretch of the OH surface species formed upon H 2 O exposure occurs at 825 cm −1 , while the SiO stretch of the OD surface species formed upon D 2 O exposure shifts to 840 cm −1 , contrary to what is expected for simple reduced mass arguments. The higher resolution of IR measurements versus typical EELS measurements makes it possible to identify a new mode at 898 cm −1 , which is an important piece of evidence in understanding the anomalous frequency shift. By comparing the results of measurements for adsorption of H 16 2 O, H 18 2 O and D 2 O with the results from recently performed first-principles calculations, it can be shown that a strong vibrational interaction between the SiO stretching and SiOH bending functional group vibrations of the hydroxyl group accounts for the observed isotopic shifts.
Journal of Vacuum Science and Technology | 2001
X. Zhang; Yves J. Chabal; S. B. Christman; E.E. Chaban; Eric Garfunkel
The initial stages of O2 oxidation of H-passivated flat and vicinal Si(111) surfaces are investigated by monitoring the Si–H stretch vibrations with infrared absorption spectroscopy. We find that the incorporation of oxygen into silicon is activated (1.66±0.10 eV on flat surfaces), involving a multistep process. Oxygen molecules are incorporated into Si–Si bonds without removing surface hydrogen and this process is facilitated at steps.
Journal of Chemical Physics | 1998
Joseph Eng; Krishnan Raghavachari; Lisa M. Struck; Yves J. Chabal; Brian E. Bent; Mark M. Banaszak-Holl; F. R. McFeely; Amy M. Michaels; George W. Flynn; S. B. Christman; E.E. Chaban; Gwyn P. Williams; K. Radermacher; S. Mantl
Motivated by a controversy about the proper interpretation of x-ray photoelectron spectra of Si/SiO2 interfaces derived from the adsorption of H8Si8O12 spherosiloxane clusters on Si(100) surfaces, we have studied the adsorption geometry of the H8Si8O12 clusters on deuterium-passivated and clean Si(100) surfaces by using external reflection infrared spectroscopy. Access to frequencies below 1450 cm−1 was made possible through the use of specially prepared Si(100) samples which have a buried metallic CoSi2 layer that acts as an internal mirror. A comparison of the infrared spectrum of the clusters on a deuterium-passivated Si(100) surface at 130 K with an infrared spectrum of the clusters in a carbon tetrachloride solution reveals that the clusters are only weakly physisorbed on the D/Si(100) surface and also provides evidence for the purity of the cluster source. We also present infrared spectra of clusters directly chemisorbed on a clean Si(100) surface and show evidence that the clusters are adsorbed on ...
Surface Science | 2002
H. Fukidome; Olivier Pluchery; K.T. Queeney; Y. Caudano; Krishnan Raghavachari; Marcus K. Weldon; E.E. Chaban; S.B. Christman; H. Kobayashi; Yves J. Chabal
Abstract The surface of SiO 2 in contact with a liquid has been studied in situ by Fourier transform infrared spectroscopy, electrochemistry and ab initio quantum chemical calculations. Experimental issues arising from the cell designed have been addressed, notably the influence of the medium above the SiO 2 film on the line shape of the Si–O vibrations. Using electrical potential control of the surface with electrochemistry, the hydrated states of the SiO 2 surface have been identified, featuring a neutral SiOH species and pentavalent Si(OH)OH − anionic centers.
international soi conference | 1997
M.K. Weldon; V. E. Marsico; Yves J. Chabal; M. Collot; Y. Caudano; S. B. Christman; E.E. Chaban; D.C. Jacobson; W. L. Brown; J. Sapjeta; C.-M. Hsieh; C.A. Goodwin; Aditya Agarwal; V.C. Venezia; T. E. Haynes; W.B. Jackson
There has been much interest in reproducing Si exfoliation by H implantation and in understanding the mechanism leading to such a remarkably uniform shearing. We have previously demonstrated that, contrary to the initial speculation, there are in fact three distinct aspects to the process: i) the generation of damage to the crystalline material by the implantation; ii) the unique surface chemistry of hydrogen and silicon that drives the thermal evolution of this damage region and; iii) the creation of internal pressure that ultimately causes exfoliation ofthe overlying Si layer. Therefore, a detailed understanding of the exfoliation mechanism involves the study of initial damage, of H-passivation of various internal structures and of the mechanical forces exerted by trapped gases as a function of hydrogen implantation dose/depth and annealing temperature. In this work, we have used different hydrogen implantation conditions (ion energies ranging from 1 eV to 1 MeV and substrate crystallographic orientations) as well as co-implantation of a variety of other elemental species, in combination with novel spectroscopic configurations, to further explore these different mechanistic aspects.