Spectroscopic ellipsometry on thin titanium oxide layers grown on titanium by plasma oxidation

Abstract : Electronic devices based on tunnel junctions require tools able to accurately control the thickness of thin metal and oxide layers on the order of the nanometer. This article shows that multisample ellipsometry is an accurate method to reach this goal on plain uniform layers, in particular for titanium. From these measurements, the authors carefully studied the oxidation rate of titanium thin films in an oxygen plasma. The authors found that the oxide thickness saturates at 5.4±0.4 nm5.4±0.4 nm after 10 min in the plasma with an ion acceleration power of 30 W. Increasing this power to 240 W increases the saturation value to 7.6±0.4 nm7.6±0.4 nm. An x-ray photoelectron spectroscopy study of the oxide has shown that the oxide created by O2O2 plasma is stoichiometric (TiO2)(TiO2). The developed model was also used to measure the thicknesses of titanium and titanium oxide layers that have been polished using a chemical mechanical planarization process and a material removal rate of 5.9 nm/min is found with our planarization parameters. I. INTRODUCTIO

Rapidly assessing the risks of infectious diseases to wildlife species

Predicting the likelihood of rare events is increasingly demanded by risk managers. A key challenge is dealing with different types of uncertainty, including epistemic uncertainties (lack of knowledge), stochasticity (inherent randomness) and natural variation. One potentially catastrophic event which is impacted by high levels of all three of these uncertainty types is the transmission of livestock pathogens to wildlife, particularly for endangered species. There is often a lack of basic information, e.g. about a given pathogen's presence in local livestock populations or the susceptibility of a given wildlife species to infection by the pathogen. We adapted the OIE (World Organisation for Animal Health) risk assessment framework to rapidly assess and prioritize the risks of livestock pathogens for wildlife, taking account of epistemic uncertainties, stochasticity, seasonal movement of animals and interaction between different species at different spatial and temporal scales. We demonstrate the approach using the endangered saiga antelope (Saiga tatarica tatarica) as a case study. We conclude that, in general, transmission events are likely to be rare and limited to small geographical areas; however, their impact could be high. Brucella spp. and foot-and-mouth disease virus are among those most likely to be transmitted from livestock to the Betpak-Dala saiga population

Regolith and landscape evolution in Peninsular India and West Africa: morphoclimatic evolution of the two continents over the Cenozoic

Shields’ surfaces of the tropical belt have been continuously shaped over the Cenozoic under the combined or alternating effects of chemical weathering and mechanical erosion that left stepped relict lateritic paleolandsurfaces exposing different generations and type of regolith in today’s sceneries. These lateritic paleolandscape remnants are well preserved in West Africa and in highland Peninsular India, particularly on Deccan Traps. The stepped character of such paleolandscape remnants allows to describing a common geomorphic sequence of three successive sub-continental scale lateritic paleolandsurfaces on the two sub regions. The first surface is defined by the oldest remnants, which are generally topped by Al-Fe (mostly bauxitic) lateritic duricrusts upon distant kmscale mesas or as larger provinces on high relictual topographic massifs (e.g., Fouta Djalon in West Africa or Nilgiri hills in South India). The relict bauxitic landforms generally dominate from less than ca. 300 m the relicts of a second geomorphic level (so-called “intermediate” surface), which is mantled by ferruginous lateritic duricrusts. The third and last paleolandsurface remnants lie less than ca. 400 m below the bauxitic landforms, and consist in a weathered lateritic pediment that is locally capped by a ferricrete. The ages of these continental-scale lateritic paleolandsurfaces may be bracketed using 40Ar/39Ar dating of K-Mn oxides (cryptomelane) formed in their underlying weathering profiles in the African and Indian contexts [1,2,3]. The first surface is Eocene and correlates with the Eocene climatic optimum (ca. 50 Ma) that is recorded throughout the tropical belt by the production of bauxite. In South India, the Intermediate surface has evolved by dominant chemical weathering since the Late Eocene (ca. 37 Ma) and records peak weathering activity in the Late Oligocene. In West Africa, that paleolandsurface seems to have only record the late Oligocene interval (ca. 29-24 Ma) of intense weathering. Abandonment of the Intermediate landscape as a result of its dissection by the river network took place in the Latest Oligocene on both continents. By contrast, the later pediment seems to have been shaped quite rapidly (ca. 32-29 Ma) and was weathered around the Oligocene- Miocene boundary (ca. 29-24 Ma) in India, whereas it took longer to form (ca. 24-18 Ma) and was weathered mostly during the Mid-Miocene (ca. 18-11 Ma) in West Africa. The contrasts in the morphoclimatic record of the two sub regions are linked to the spatial diversification of climatic regimes after the Eocene climatic optimum. However, the combination of the ages with the elevation differences between each lateritic paleolandsurface documents denudation rates with comparable and very low amplitudes (5-15 m/m.y.) in these two continents over the last 50 Ma. [1] Beauvais A and Chardon D (2013) Geochem Geophys Geosyst 14:1590-1608, doi:10.1002/ggge.20093. [2] Bonnet NJ et al. (2014) Earth Planet Sci Lett 386:126-137, doi:10.1016/j.epsl.2013.11.002 [3] Bonnet NJ et al. (2016) Chem Geol, in press

Signatures of Galaxy-Cluster Interactions: Spiral Galaxy Rotation Curve Asymmetry, Shape, and Extent

The environmental dependencies of the characteristics of spiral galaxy rotation curves are studied in this work. We use our large, homogeneously collected sample of 510 cluster spiral galaxy rotation curves to test the claim that the shape of a galaxy's rotation curve strongly depends on its location within the cluster, and thus presumably on the strength of the local intracluster medium and on the frequency and strength of tidal interactions with the cluster and cluster galaxies. Our data do not corroborate such a scenario, consistent with the fact that Tully-Fisher residuals are independent of galaxy location within the cluster; while the average late-type spiral galaxy shows more rise in the outer parts of its rotation curve than does the typical early-type spiral galaxy, there is no apparent trend for either subset with cluster environment. We also investigate as a function of cluster environment rotation curve asymmetry and the radial distribution of H II region tracers within galactic disks. Mild trends with projected cluster-centric distance are observed: (i) the (normalized) radial extent of optical line emission averaged over all spiral galaxy types shows a 4%+/-2% increase per Mpc of galaxy-cluster core separation, and (ii) rotation curve asymmetry falls by a factor of two between the inner and outer cluster for early-type spirals (a negligible decrease is found for late-type spirals). Such trends are consistent with spiral disk perturbations or even the stripping of the diffuse, outermost gaseous regions within the disks as galaxies pass through the dense cluster cores.Comment: 17 pages; to appear in the April 2001 Astronomical Journa