EBID for APT Specimen Capping 323
Table 2. Compositions of the Electron Beam-Induced Deposition Layers as Measured by X-Ray Spectroscopy (EDX) and Atom Probe Tomography (APT).
Depositions Au
Au+O2 Co Fe Pd Pt
EDX Composition (at%)
Au27, C62, O10 >95% Au
Co80, C10, O10 Fe58, C3, O39
Pd28, C57, O8, F7 Pt18, C77, O5
depositions did not have sufficient or reliable statistics for confident assignment of an uncertainty. For the Au, Pd, and Pt depositions, the measured metal content by both EDX and APT was around 20–30 at% in all cases. The balance of those layers were carbon and oxygen. EDX and APT differed on the relative concentrations of those, with EDX measure- ments indicating more C and APTmeasurements indicating more O. These discrepancies could result from electron beam-assisted carbon deposition during the EDX scans, residual oxygen-containing species in the APT chamber, and/or undercounting of carbon in the atomprobe as a result of multiple ion events (Thuvander et al., 2011). As is discussed more in the next section, the APT measurements on these depositions collected relatively few ions and they each exhibited a two-phase structure. The Au+O2 deposition was measured as >95 at% gold
by EDX. All APT measurements of this deposition indicated not only gold but also displayed a large amount of silicon in the mass spectra, which precluded a reliable determination of the composition of just the Au layer. The reasons for this result are discussed more later. Composition of the Co and Fe layers asmeasured by the
sufficient contrast in the SEM between the deposition and the surface region of interest (ROI) for ease of targeting the endpoint and uniform milling. Figure 1 shows images of a sharpened tip for each deposition. In each case both of these criteria appear to be met. The additional criteria of adhesion of the layer to the specimen surface, potential peak inter- ferences in the mass spectrum, evaporation behavior and evaporation field of the deposition, and range of Ga+
two techniques agreed quite nicely. The Co deposition was shown to be 80 at% Co and roughly 10 at% each of C and O, which is in the range of values seen by others for this precursor (Utke et al., 2005; Fernández-Pacheco et al., 2009; Córdoba et al., 2010; Mulders et al., 2011; Pfeiffer et al., 2015). The Fe deposition was ~60 at% Fe and 40 at% O. These values are quite a bit different than previous reports using the same precursor, where ~15 at%C, 15 at%O, and 70 at%Fe was seen for deposition on a SiO2 substrate (Lavrijsen et al., 2011) and~2 at% C, 2 at% O, and 96 at% Fe was seen for deposition on gold (Pfeiffer et al., 2015). This variability suggests that deposition conditions, particularly the substratematerial, may exert a large influence over the final composition. Two key criteria for this application of EBID are having
APT Composition (at%)
Au23, C42, O35 x
Co82, C10, O8 Fe60, C0, O40
Pd20, C35, O44, F0 Pt31, C39, O30
APT Uncertainty (at%)
x x
Co3, C1, O3 Fe1, C0, O1
Pd7, C1, O6, F1 x
ion penetration into the deposition are considered for the individual depositions in the following discussion.
APT of Au, Pd, and Pt
The Au, Pd, and Pt depositions had similar APT results and, therefore, their results have been aggregated for discussion. These were analyzed using laser energies of 15 and 30pJ over a voltage range of 0.7–3.2 kV. The analyses acquired 40–430 k ions with an average of about 230 k ions. This corresponds roughly to a removed depth of 5–50nm.Eachanalysisincluded an abrupt transition from the deposition material to the silicon post as evidenced by a change in the mass spectrum to one consisting of only silicon. In each case, the transition occurred at applied biases slightly>3 kV. Shortly after this transition, the APT data collection was manually halted. From pre- and post- APT imaging in the SEM, it was determined that these transi- tions were indicative of microfracturing of the specimen. That is, the remainder of the deposited cap and some portion of the underlying Si post were lost during such an event. This is illu- strated by overlay of the before and after SEM images for the Au deposition in Figure 2. Consistent with TEM observations from EBID Pt (Rotkina et al., 2005) and with APT observations from ion beam deposited Pt (Gerstl et al., 2006), the Pt deposition reconstructions indicated 0.6–7-nm-sized Pt-rich regionswithin a C-rich matrix. This composite structure is the likely source for premature failure of these capping layers, with at least two plausible explanations. (1) It could be failure at the interface between the deposition and the Si post. No pretreatment of the Si was performed, therefore a thin oxide layer is expected on the surface. The Pt–C deposition on the oxidemay lead to poor adhesion as has been suggested by the work of others (Rykaczewski et al., 2011). (2) The failures could also occur within the depositions. The metal particles and carbon matrix are expected to have very different eva- poration fields (Tsong, 1978).Once a sufficient bias is reached, localized high fields at the metal particle—carbon matrix interfaces may result in decohesion and premature failure.
APT of Au+O2 APT analyses on this deposition were attempted using a range of conditions: laser energies from 30–240 pJ, corresponding to biases of 5.2–1.1 kV. In each case the mass
Page 1 |
Page 2 |
Page 3 |
Page 4 |
Page 5 |
Page 6 |
Page 7 |
Page 8 |
Page 9 |
Page 10 |
Page 11 |
Page 12 |
Page 13 |
Page 14 |
Page 15 |
Page 16 |
Page 17 |
Page 18 |
Page 19 |
Page 20 |
Page 21 |
Page 22 |
Page 23 |
Page 24 |
Page 25 |
Page 26 |
Page 27 |
Page 28 |
Page 29 |
Page 30 |
Page 31 |
Page 32 |
Page 33 |
Page 34 |
Page 35 |
Page 36 |
Page 37 |
Page 38 |
Page 39 |
Page 40 |
Page 41 |
Page 42 |
Page 43 |
Page 44 |
Page 45 |
Page 46 |
Page 47 |
Page 48 |
Page 49 |
Page 50 |
Page 51 |
Page 52 |
Page 53 |
Page 54 |
Page 55 |
Page 56 |
Page 57 |
Page 58 |
Page 59 |
Page 60 |
Page 61 |
Page 62 |
Page 63 |
Page 64 |
Page 65 |
Page 66 |
Page 67 |
Page 68 |
Page 69 |
Page 70 |
Page 71 |
Page 72 |
Page 73 |
Page 74 |
Page 75 |
Page 76 |
Page 77 |
Page 78 |
Page 79 |
Page 80 |
Page 81 |
Page 82 |
Page 83 |
Page 84 |
Page 85 |
Page 86 |
Page 87 |
Page 88 |
Page 89 |
Page 90 |
Page 91 |
Page 92 |
Page 93 |
Page 94 |
Page 95 |
Page 96 |
Page 97 |
Page 98 |
Page 99 |
Page 100 |
Page 101 |
Page 102 |
Page 103 |
Page 104 |
Page 105 |
Page 106 |
Page 107 |
Page 108 |
Page 109 |
Page 110 |
Page 111 |
Page 112 |
Page 113 |
Page 114 |
Page 115 |
Page 116 |
Page 117 |
Page 118 |
Page 119 |
Page 120 |
Page 121 |
Page 122 |
Page 123 |
Page 124 |
Page 125 |
Page 126 |
Page 127 |
Page 128 |
Page 129 |
Page 130 |
Page 131 |
Page 132 |
Page 133 |
Page 134 |
Page 135 |
Page 136 |
Page 137 |
Page 138 |
Page 139 |
Page 140 |
Page 141 |
Page 142 |
Page 143 |
Page 144 |
Page 145 |
Page 146 |
Page 147 |
Page 148 |
Page 149 |
Page 150 |
Page 151 |
Page 152 |
Page 153 |
Page 154 |
Page 155 |
Page 156 |
Page 157 |
Page 158 |
Page 159 |
Page 160 |
Page 161 |
Page 162 |
Page 163 |
Page 164 |
Page 165 |
Page 166 |
Page 167 |
Page 168 |
Page 169 |
Page 170 |
Page 171 |
Page 172 |
Page 173 |
Page 174 |
Page 175 |
Page 176 |
Page 177 |
Page 178 |
Page 179 |
Page 180 |
Page 181 |
Page 182 |
Page 183 |
Page 184 |
Page 185 |
Page 186 |
Page 187 |
Page 188 |
Page 189 |
Page 190 |
Page 191 |
Page 192 |
Page 193 |
Page 194 |
Page 195 |
Page 196 |
Page 197 |
Page 198 |
Page 199 |
Page 200 |
Page 201 |
Page 202 |
Page 203 |
Page 204 |
Page 205 |
Page 206 |
Page 207 |
Page 208 |
Page 209 |
Page 210 |
Page 211 |
Page 212 |
Page 213 |
Page 214 |
Page 215 |
Page 216 |
Page 217 |
Page 218 |
Page 219 |
Page 220 |
Page 221 |
Page 222 |
Page 223 |
Page 224 |
Page 225 |
Page 226 |
Page 227 |
Page 228 |
Page 229 |
Page 230 |
Page 231 |
Page 232 |
Page 233 |
Page 234 |
Page 235 |
Page 236 |
Page 237 |
Page 238 |
Page 239 |
Page 240 |
Page 241 |
Page 242 |
Page 243 |
Page 244 |
Page 245 |
Page 246 |
Page 247 |
Page 248 |
Page 249 |
Page 250 |
Page 251 |
Page 252 |
Page 253 |
Page 254 |
Page 255 |
Page 256 |
Page 257 |
Page 258 |
Page 259 |
Page 260 |
Page 261 |
Page 262 |
Page 263 |
Page 264 |
Page 265 |
Page 266 |
Page 267 |
Page 268 |
Page 269 |
Page 270 |
Page 271 |
Page 272 |
Page 273 |
Page 274 |
Page 275 |
Page 276 |
Page 277 |
Page 278 |
Page 279 |
Page 280 |
Page 281 |
Page 282 |
Page 283 |
Page 284