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  • 1995-1999  (9)
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  • 1
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 79 (1996), S. 4087-4095 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The use of "Kissinger'' plots to analyze in situ resistance monitoring of thin-film reactions during heating at a constant rate is widely accepted. One obtains the activation energy for diffusion, at least in the case of diffusion-controlled reactions. The aim of this article is to extend the analysis one step further and show that, provided that the thickness of the layers formed is known, the same experimental and analytical techniques may yield the pre-exponential growth factor. The validity of the procedure is demonstrated by comparing the results thus obtained with data from the literature derived by conventional analysis of compound growth during isothermal annealing. Such comparisons have been made for Co2Si, CoSi, CoSi2, Pt2Si, PtSi, Ni2Si, and NiSi formation on undoped polycrystalline Si and single-crystal Si on sapphire substrates with ramp rates ranging from 10−2 °C/s to 102 °C/s. Measurements used both conventional furnace and rapid thermal annealing. In the past, the common practice has been to use the Kissinger method regardless of the sequence of growing phases. However, for phases other than the first one to be formed the direct Kissinger analysis needs to be modified. In the present cases the results obtained by means of an appropriately corrected procedure are not significantly different; that may not always be true. © 1996 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 2
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The formation of titanium silicides has been studied using simultaneous in situ x-ray diffraction with millisecond time resolution and sheet resistance measurements. The effect of a Mo interposed layer between Ti films and Si substrate was investigated by varying the thickness of the Mo interlayer from 0 (Ti/Si) to 1.8 nm (Ti/Mo/Si). The thickness of Ti was kept to 55 nm for all samples. Both isothermal annealing and ramp annealing in helium were performed in order to study the mechanism of silicide formation. While C49 TiSi2 was the only disilicide found after annealing Ti/Si at 650 °C for 20 min, C54 TiSi2 was readily formed in the presence of Mo. The formation of C49 TiSi2 was not observed with a 1.8 nm thick Mo interlayer. Instead, there was indication that C40 (Mo,Ti)Si2 was formed. In addition, broad diffraction peaks, weak in intensity, could be all assigned to Ti5Si4. However, the presence of Ti5Si4 alone did not induce the formation of C54 TiSi2. Even with a 20 °C increase in isothermal annealing temperature to 670 °C for 20 min, the presence of Mo was found to be a necessity for the formation of C54 TiSi2. When annealed in nitrogen, instead of helium, the formation of surface titanium nitride competes with the formation of silicides. The formation of C54 TiSi2 was even suppressed in the sample with a 1.8 nm Mo interlayer when annealed at 650 °C in nitrogen. The formation of Ti5Si4 and the role it plays in the formation of other silicides (C40, C49, and C54) are discussed on the basis of simple crystallographic considerations. The effect of a Mo interlayer and/or ramp-rate on the formation of C40 (Mo,Ti)Si2 and C49 TiSi2 is discussed in conjunction with variations of the preferential orientation of C54 TiSi2 films. © 1999 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Woodbury, NY : American Institute of Physics (AIP)
    Applied Physics Letters 73 (1998), S. 312-314 
    ISSN: 1077-3118
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The introduction of a thin layer of Al at the interface between Ti films and Si substrates enhances the formation of C49 TiSi2 and retards the transition from C49 to C54. An Al interlayer, 0.64 nm thick, reduces the time required to form C49 TiSi2 isothermally at 500 °C from 14 to 7 min. The C49–C54 transformation temperature is increased from 767 to 853 °C, when heating the samples at a constant ramp rate of 3 K/s. Most of the Al is found toward the interface between a Ti-rich silicide at the surface and TiSi2, rather than at the interface between TiSi2 and the Si substrate. The grain size of the C49 TiSi2 formed in the presence of Al is about five times smaller than that formed on a control sample with pure Ti, indicating that the increased density of grain boundaries in C49 TiSi2 in the presence of Al does not help the C49–C54 transformation. Therefore, the improved thermal stability of C49 TiSi2 is likely to be caused by other factors such as a reduced electron/atom ratio when replacing Si with Al in the disilicide. © 1998 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 82 (1997), S. 5773-5778 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The oxidation of polycrystalline SixGe1−x films with different compositions (i.e., different values of x) is carried out in pyrogenic steam at 800 °C for various lengths of time. It is found that the oxidation is enhanced by the presence of germanium and that the enhancement effect is more pronounced for the films richer in germanium. A mixed oxide in the form of either (Si,Ge)O2 or SiO2–GeO2 is found at the sample surface if the initial SixGe1−x contains more than 50% of germanium. However, a surface silicon cap layer of about 14 nm is found to have a significant impact on the oxidation of the Si0.5Ge0.5 films; it leads to the growth of about 115-nm-thick SiO2 which is about four times that of the SiO2 resulting from the oxidation of the cap layer itself. On the SixGe1−x films with only 30% of germanium, the SiO2 continues to grow after oxidation for 180 min resulting in 233-nm-thick SiO2 which is about 2.4 times greater than the SiO2 grown on 〈100〉 silicon substrates. Rejection of germanium results in piling up of germanium at the interface between the growing SiO2 and the remaining SixGe1−x. Substantial interdiffusion of silicon and germanium takes place in the remaining SixGe1−x. The experimental results are discussed in terms of thermodynamics and kinetics. © 1997 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 83 (1998), S. 90-99 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The interdiffusion of Cu and Sn, and the formation and dissolution of Cu–Sn precipitates have been examined for Cu alloy films. Cu(Sn) films were deposited by electron beam evaporation either as Sn/Cu bilayers or Cu/Sn/Cu trilayers, with overall Sn concentrations from 0.1 to 5 at. %. In situ resistance, calorimetry, electron, and x-ray diffraction measurements indicate that η–Cu6Sn5 forms during film deposition. Upon heating, ε–Cu3Sn forms at 170 °C, then this phase dissolves into the Cu matrix at approximately 350 °C. Finally, ζ–Cu10Sn3 forms and precipitates after thermal cycling to 500 °C. The final resistivity of Cu/Sn/Cu films with more than 2 at. % Sn exceeds 3.5 μΩ cm. However, resistivities from 1.9 to 2.5 μΩ cm after annealing were reached in Cu/Sn/Cu films with less than 2 at. % Sn. Auger and Rutherford backscattering analysis of Cu/Sn bilayers (1 mm thick) showed that the homogenization of Sn in Cu requires annealing in excess of 350 °C for 30 min; after annealing, the Sn concentration at the surface is approximately 20 at. %. The interdiffusion of Sn and Cu is inhibited by contamination at the Sn/Cu interface caused by air exposure. © 1998 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 82 (1997), S. 5779-5787 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: A mathematical model of oxidation of SixGe1−x alloys is presented. The growth of SiO2 is simulated in conjunction with the determination of silicon distribution in SixGe1−x using numerical methods. The main feature of the model is the assumption of simultaneous oxidation of germanium and silicon when exposing the SixGe1−x to an oxidizing atmosphere. In accordance with thermodynamics, the GeO2 formed is subsequently reduced by the (free) silicon available at the interface between the growing SiO2 and the remaining SixGe1−x through a reduction reaction. Thus, the enhanced oxidation of silicon in the presence of germanium is modeled as a result of the rapid oxidation of germanium followed by the quick reduction of GeO2 by silicon. The growth of a mixed oxide in the form of either (Si,Ge)O2 or SiO2–GeO2 only occurs when the supply of silicon to the SiO2/SixGe1−x interface is insufficient. A comparison is made between simulation and experiment for wet oxidation (in pyrogenic steam) of polycrystalline SixGe1−x films. It is found that the model gives a good account of the oxidation process. Kinetic parameters, i.e., interfacial reaction rate constant for oxidation of germanium and diffusion coefficient of silicon (germanium) in SixGe1−x, are extracted by fitting the simulation to the experiment. © 1997 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    Woodbury, NY : American Institute of Physics (AIP)
    Applied Physics Letters 66 (1995), S. 58-60 
    ISSN: 1077-3118
    Source: AIP Digital Archive
    Topics: Physics
    Notes: In spite of much work, the formation of epitaxial CoSi2 from Ti/Co on (100) Si remains something of a mystery. It has been proposed that epitaxy occurs via the formation of an intermediate phase of CoSi with a (311) preferred orientation. In the absence of sufficient information it is impossible to validate or to invalidate the specific original claim. However, one shows that the formation of preferably oriented CoSi is not a necessary condition for the subsequent growth of epitaxial CoSi2. Careful measurements of diffraction intensities reveal the probable, temporary formation of a metastable form of CoSi2, based on a diamond cubic rather than the usual CaF2 structure. © 1995 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    Woodbury, NY : American Institute of Physics (AIP)
    Applied Physics Letters 71 (1997), S. 3531-3533 
    ISSN: 1077-3118
    Source: AIP Digital Archive
    Topics: Physics
    Notes: We demonstrate that the temperature at which the C49 TiSi2 phase transforms to the C54 TiSi2 phase can be lowered more than 100 °C by alloying Ti with small amounts of Mo, Ta, or Nb. Titanium alloy blanket films, containing from 1 to 20 at. % Mo, Ta, or Nb were deposited onto undoped polycrystalline Si substrates. The temperature at which the C49–C54 transformation occurs during annealing at constant ramp rate was determined by in situ sheet resistance and x-ray diffraction measurements. Tantalum and niobium additions reduce the transformation temperature without causing a large increase in resistivity of the resulting C54 TiSi2 phase, while Mo additions lead to a large increase in resistivity. Titanium tantalum alloys were also used to form C54 TiSi2 on isolated regions of arsenic doped Si(100) and polycrystalline Si having linewidths ranging from 0.13 to 0.56 μm. The C54 phase transformation temperature was lowered by over 100 °C for both the blanket and fine line samples. As the concentration of Mo, Ta, or Nb in the Ti alloys increase, or as the linewidth decreases, an additional diffraction peak appears in in situ x-ray diffraction which is consistent with increasing amounts of the higher resistivity C40 silicide phase. © 1997 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 9
    ISSN: 1077-3118
    Source: AIP Digital Archive
    Topics: Physics
    Notes: We report that the ion implantation of a small dose of Mo into a silicon substrate before the deposition of a thin film of Ti lowers the temperature required to form the commercially important low resistivity C54–TiSi2 phase by 100–150 °C. A lesser improvement is obtained with W implantation. In addition, a sharp reduction in the dependence of C54 formation on the geometrical size of the silicided structure is observed. The enhancement in C54 formation observed with the ion implantation of Mo is not explained by ion mixing of the Ti/Si interface or implant-induced damage. Rather, it is attributed to an enhanced nucleation of C54–TiSi2 out of the precursor high resistance C49–TiSi2 phase. © 1995 American Institute of Physics.
    Type of Medium: Electronic Resource
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