2014
DOI: 10.1116/11.20140506
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X-ray Photoelectron Spectroscopy Analyses of the Electronic Structure of Polycrystalline Ti1-xAlxN Thin Films with 0 ≤ x ≤ 0.96

Abstract: Metastable Ti 1-x Al x N (0 x 0.96) alloy thin films are grown by reactive magnetron sputter deposition using a combination of high-power pulsed magnetron (HIPIMS) and DC magnetron sputtering (DCMS). Layers are deposited from elemental Ti and Al targets onto Si(001) substrates at 500C. All Ti 1-x Al x N film surfaces are analyzed by x-ray photoelectron spectroscopy (XPS) employing monochromatic Al K a radiation (h = 1486.6 eV). Prior to spectra acquisition, TiAlN surfaces are sputter-cleaned in-situ with 4 keV… Show more

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Cited by 22 publications
(17 citation statements)
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References 24 publications
(12 reference statements)
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“…We select Al as the cap layer for the following reasons: (1) the Al native oxide, <2 nm thick at room temperature, is stable against spallation; 29 thus minimizing interfacial reactions; (3) and Al core-level peaks do not overlap with the primary Ti and N signals. We show that Al layers with thickness d Al ¼ 1.5 nm form a dense continuous, oxidized barrier that protects the TiN underlayer and allows for acquisition of high-resolution Ti 2p and N 1s core-level spectra, with clear pronounced satellite features, [30][31][32][33] which are in excellent agreement with those obtained from epitaxial TiN layers grown in-situ in an XPS system. 34 O 1s spectra reveal no evidence for Ti-O bonding.…”
Section: Introductionsupporting
confidence: 71%
“…We select Al as the cap layer for the following reasons: (1) the Al native oxide, <2 nm thick at room temperature, is stable against spallation; 29 thus minimizing interfacial reactions; (3) and Al core-level peaks do not overlap with the primary Ti and N signals. We show that Al layers with thickness d Al ¼ 1.5 nm form a dense continuous, oxidized barrier that protects the TiN underlayer and allows for acquisition of high-resolution Ti 2p and N 1s core-level spectra, with clear pronounced satellite features, [30][31][32][33] which are in excellent agreement with those obtained from epitaxial TiN layers grown in-situ in an XPS system. 34 O 1s spectra reveal no evidence for Ti-O bonding.…”
Section: Introductionsupporting
confidence: 71%
“…The Ti 2p 3/2 core levels recorded in point-B and D demonstrate the dramatic effects of ion irradiation. In the TiN layer a new lineshape of the Ti 2p slightly shifts to higher binding energies, and the shake-up peaks become more dominant in agreement with previously reported works [17,27]; a well spectral matching of the Ti 2p curve with reference spectrum [17] The irradiated sample still exhibits some form of a layered structure, but the layers become thicker and the contrast appears rather uniform, indicating that initially isolated phases become intermixed. A closer analysis shows that TiN layers appear to grow in thickness, consuming the adjacent AlN layers.…”
Section: Resultssupporting
confidence: 90%
“…In our case, the XRD reflexion at 37.5° of the eV and 461.36 eV correspond to Ti 2p3/2 and Ti 2p1/2 branchings, respectively. This is in agreement with the binding energy of Ti in the TiAlN structure [22,28], and no other signals of Ti-N bonds were found. The second doublet at 457.27 and 462.93 eV confirms the presence of TiOxNy bonds [28] and, the third doublet at 459.20 and 464.86 eV is associated with Ti-O bonds into TiO2 [29].…”
Section: Initial State Of the C-al066ti033n Coatingssupporting
confidence: 91%
“…Fig. 2c displays the N 1s spectrum with three components at 396.59, 397.68 and 400.36 eV corresponding to Al-Ti-N, Al-Ti-O-N and N-C bonds [22,[26][27][28].…”
Section: Initial State Of the C-al066ti033n Coatingsmentioning
confidence: 99%