Optical particle counting for thin films and wafers

Cryo-SEM imaging with EDX elemental mapping for fragile samples that require cryogenic preparation to withstand the SEM vacuum and electron beam. The analysis includes the following steps: Cryo-fixing of the sample., Imaging of the sample surface with a scanning electron microscope., EDX map for elemental composition.. The results will include 10–20 SEM images with annotations showing the observed features. 1–2 EDX elemental maps will also be provided, depending on the magnification.

Imaging of the sample using scanning electron microscopy (SEM). Typically, several images are taken with varying magnifications to get a good overview of the sample. Non-conductive samples can be prepared with a metallic coating to allow imaging. For cross-section measurement, additional preparation might be needed: FIB, BIB, or freeze fracturing. Cryo preparation is available for biological materials and other sensitive sample types. If compositional analysis is also needed, please see the SEM-EDX measurement. We also offer high-temperature SEM analyses at temperatures up to 1400 °C. Do not hesitate to ask for a quote.

Imaging of the sample using a scanning electron microscope (SEM) with energy-dispersive X-ray spectroscopy (EDX or EDS). Typically, several images are taken with varying magnifications to get a good overview of the sample. An EDX mapping, line scan, or point measurement is collected to measure the sample composition (elemental at.% or wt.%). Non-conductive samples can be prepared with a metallic coating. For cross-section measurement, additional preparation might be needed: FIB, BIB, or freeze fracturing.

X-Ray Reflectometry (XRR) analysis is used to measure the density (g/cm3), thickness (nm), and roughness (nm) of thin films. The method is applicable to the characterization of single- or multilayered thin films, as it provides information on the thickness and density of individual layers of the sample material as well as the roughness of the interphases. Greatest accuracy for XRR thickness measurements is generally achieved for samples containing 1-150 nm thick surface layers with under 5 nm RMS roughness. Thicker films and coatings with rougher surfaces can also be characterized, but the accuracy of thickness determination decreases as the thickness and roughness of the film or film stack increase. >150 mm wafers are typically cut to fit the sample holder. Please let us know if you need testing for larger wafers that cannot be cut into pieces. The available temperature range for XRR measurements is 25-1100 °C, and crystallinity can be studied as a function of temperature. The measurements can be performed under a normal atmosphere, inert gas, or vacuum. Measurements are typically performed using one of the following instruments: Rigaku SmartLab, Panalytical X'Pert Pro MRD, Bruker D8 Discover. Please let us know if you have a preference for a specific instrument.

During this analysis, the surface of a smooth and hard sample is imaged with an atomic force microscope (AFM). Topological images are typically provided from three locations around the sample. The measurement area is 5 x 5 micrometers, if not otherwise agreed. Measurements are typically done using the following instrument: Bruker Dimension Icon.

Analysis of the specific surface area of porous, solid materials according to the BET (Brunauer–Emmett–Teller) theory. Analysis can be performed with N2 or Kr gases, depending on the expected surface area of the material. BET curve and the specific surface area (in m2/g) are reported. The required sample amount depends on the expected surface area. As a rule of thumb, at least 5 m2 of surface area should be available for measurement. The following gas adsorption devices are used for this measurement: Micromeritics Gemini VII 2390, Micromeritics ASAP 2020, Micromeritics TriStar II 3020, Anton Paar Nova 800.

Rutherford Backscattering Spectrometry (RBS) can be used to measure the composition of solid samples quantitatively at the surface as well as depth profiling. RBS is used for the analysis of heavy elements and can be combined with ToF-ERDA when lighter elements also need to be analyzed. Elements with similar mass can be difficult to differentiate.

VPD ICP-MS allows the determination of trace metal contamination on the surface of wafers. The full surface of the wafer is scanned during the analysis, unless edge exclusion (2 mm, 5 mm, etc.) is requested. VPD ICP-MS is performed using acid to dissolve the top surface of the wafer before the determination of elemental concentrations with ICP-MS. Please note that lighter elements, such as H, C, N, O, and F, cannot be analyzed. We offer different analysis packages for a wide range of elements: 58 element analysis: Al, As, B, Ba, Be, Bi, Ca, Cd, Ce, Co, Cr, Cs, Cu, Dy, Er, Eu, Fe, Ga, Gd, Ge, Hf, Hg, Ho, In, K, La, Li, Lu, Mg, Mn, Mo, Na, Nb, Nd, Ni, Pb, Pr, Rb, Sb, Sc, Se, Sm, Sn, Sr, Ta, Tb, Te, Th, Ti, Tl, Tm, U, V, W, Y, Yb, Zn, Zr, 41 element analysis: Al, As, B, Ba, Be, Bi, Ca, Cd, Co, Cr, Cs, Cu, Ga, Ge, Fe, Hf, Ir, K, Li, Mg, Mn, Mo, Na, Nb, Ni, Pb, Re, Sb, Sn, Sr, Ta, Te, Th, Ti, Tl, U, W, V, Y, Zn, Zr, 30 element analysis: Al, As, B, Ba, Be, Bi, Ca, Cd, Co, Cr, Cu, Ga, Ge, Fe, K, Li, Mg, Mn, Mo, Na, Ni, Pb, Sb, Sn, Sr, Ti, W, V, Zn, Zr, Custom 30-element package: You choose any 30 elements from our full 58-element list., Additional noble metals: Add the analysis of noble metals to any package from the options given below: Ag, Au, Pd, Pt, Rh, Ru, Ag, Au, Pt, Pd.. Additional elements are available upon request, Detection limits are in the ppm–ppb range (106–1010at/cm2), See this example report: VPD ICP-MS analysis, for more details. This measurement is primarily intended for 100, 150, 200, and 300 mm bare-silicon wafers, but we also offer ICP-MS analyses for other wafer sizes and thin films up to a few µm thickness. The most typically used instruments include the following: Perkin-Elmer NexION 350S ICP-MS, Perkin-Elmer Sciex ELAN 6100 DRC II ICP-MS, Thermo Fisher iCAP TQe ICP-MS, Finnigan element2 ICP-MS. Express turnaround (1–3 business days) can be arranged upon request for an additional charge. Contact us for more information and to request a quote.

XPS is a semi-quantitative technique used to measure the elemental composition of material surfaces. In addition, it can also determine the binding state of the atoms. XPS is a surface-sensitive technique. Typical probing depth is 3-9 nm, and detection limits range roughly between 0.1 and 1 atomic %. XPS can measure elements from Li to U. The elemental composition is reported in at.% and measured on 1 area of a few 100 µm. Upon request, we can measure smaller areas or depth profiles, and a binding state determination can also be provided. Measurements are typically performed using one of the following instruments: PHI Genesis, Thermo Fisher ESCALAB 250Xi, PHI Quantum 2000. Synchrotron XPS is also available. Contact us for more information and a quote for your project.

Grazing incidence X-ray diffraction (GI-XRD) measurement for thin films and surface layers. The measurement provides the following information: XRD spectrum and identification of the phase(s), Crystallinity, crystallite size, lattice parameters, and strain of the phase. NOTE that these parameters are determined if the samples are highly crystalline. It may not be possible to determine them if the crystallinity is insufficient.. For a practical illustration of how the results are expressed, see our example report: GI-XRD measurement. Best GI-XRD results are typically achieved for samples containing up to 300 nm thick surface layers with under 10 nm RMS roughness. Thicker films and coatings with rougher surfaces can also be characterized, but the quality of the data is generally lower for rough samples, and the sample properties below 300 nm depths are typically not reflected in the results. One of the following instruments is typically used to perform the measurements: Rigaku SmartLab, Panalytical X'Pert Pro MPD, Bruker D8 Discover, Malvern Empyrean, GNR APD2000PRO. By default, the GI-XRD is conducted in ambient conditions, but temperatures of 25 to 1100 °C can be used to study crystallinity as a function of temperature. The measurements can also be performed under inert gas or vacuum if needed. Please contact our experts to discuss the available temperature and atmosphere combinations.