2017
DOI: 10.1116/1.4978030
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Electronic and optical properties of rocksalt-phase tungsten nitride (B1-WN)

Abstract: The optical and electronic properties of rocksalt structure tungsten nitride (B1-WN) were investigated by x-ray photoelectron spectroscopy (XPS) and UV–visible-Fourier transform infrared optical reflectivity. Both 111-textured polycrystalline and epitaxial WN(111) films with [N]/[W] ratios of 1.12 and 0.87, respectively, were found to be electron conductors with partially filled W-5d conduction bands. However, their electronic behavior is dominated by high conduction electron losses, which are attributed to sc… Show more

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Cited by 15 publications
(11 citation statements)
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“…MoN0.69 the fit renders the values Epu= 9.12 eV and D=1.48 eV, that provide a resistivity value of 133  cm, which is in fair agreement with the electrically measured 250  cm; this value is at least an order of magnitude smaller than the values for WNx20 , and comparable to the resistivity of other polycrystalline conductive nitrides5 , stoichiometric epitaxial NbN39 and TaN40 , under-stoichiometric (x<1) epitaxial TiNx41 and HfNx42 , epitaxial TiN with point defects43 , albeit higher by an order of magnitude than the resistivity of stoichiometric epitaxial TiN 41 , ZrN44 , HfN42 , and VN45 .…”
supporting
confidence: 66%
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“…MoN0.69 the fit renders the values Epu= 9.12 eV and D=1.48 eV, that provide a resistivity value of 133  cm, which is in fair agreement with the electrically measured 250  cm; this value is at least an order of magnitude smaller than the values for WNx20 , and comparable to the resistivity of other polycrystalline conductive nitrides5 , stoichiometric epitaxial NbN39 and TaN40 , under-stoichiometric (x<1) epitaxial TiNx41 and HfNx42 , epitaxial TiN with point defects43 , albeit higher by an order of magnitude than the resistivity of stoichiometric epitaxial TiN 41 , ZrN44 , HfN42 , and VN45 .…”
supporting
confidence: 66%
“…The two Lorentz oscillators are located at an energy position E 0 j = ℏω 0 j , with strength f j and damping (broadening) factor γ j . The Drude term in eq is characterized by the unscreened plasma energy E pu = ℏω pu , (which is associated with conduction electron density ,,,,, ) and the damping factor Γ D , which accounts for the various electron scattering mechanisms; for the particular case of B1-MoN 0.69 , the fit renders the values E pu = 9.12 eV and Γ D = 1.48 eV, which provide a resistivity value of 133 μΩ cm, which is in fair agreement with the electrically measured 250 μΩ cm; this value is at least an order of magnitude smaller than the values for WN x and comparable to the resistivity of other polycrystalline conductive nitrides, stoichiometric epitaxial NbN and TaN, understoichiometric ( x < 1) epitaxial TiN x and HfN x , and epitaxial TiN with point defects, albeit higher by an order of magnitude than the resistivity of stoichiometric epitaxial TiN, ZrN, HfN, and VN …”
Section: Resultsmentioning
confidence: 52%
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“…Numerous calculations have recently predicted the same thermodynamically stable cubic tungsten mononitride of cP6-WN, which is structurally isotypic with NbO and can be viewed as a defective cF8-WN with ordered vacant W and N sites (i.e., rocksalt-like phase) (Figure c). Note that rocksalt cF8-WN can readily be experimentally accessible, especially in thin-film forms, , although its stoichiometric sample with a large valence electron concentration (VEC) of 11 is electronically unfavorable due to the overfilling effect of its valence band with a maximum VEC of 10.5. , This indicates that the nitrogen deficiency should be intrinsic and occurs randomly in cF8-WN to reach a favorable valence-band filling for stabilizing its structure. , However, due to the challenging sample synthesis and difficulties in probing nitrogen and atomic vacancies, the crystal structures, compositions, and formation mechanisms of these two cubic tungsten nitrides have not yet been clearly elucidated, leading to many ambiguities of their mechanical and thermal properties.…”
Section: Introductionmentioning
confidence: 99%
“…Figure 2i depicts the N 1s spectrum of WMCNFs, where the N−W bond at 396.9 eV further verifies the formation of the WN phase in the composite. 43 Besides, the distinguishable nitrogen species including pyridinic N, pyrrolic N, and graphitic N indicate that the amidogen of CFs can not only serve as the nitrogen source for WN but also be incorporated into the carbon framework to achieve the in situ N-modification.…”
Section: Resultsmentioning
confidence: 99%