Atomic surface reduction of interfaces utilizing vapor phase approach: High energy LiNixMnyCoz oxide as a test case

2019 ◽  
Vol 19 ◽  
pp. 261-269 ◽  
Author(s):  
Eliran Evenstein ◽  
Rosy ◽  
Shira Haber ◽  
Hadar Sclar ◽  
Lothar Houben ◽  
...  
2019 ◽  
Vol 31 (10) ◽  
pp. 3840-3847 ◽  
Author(s):  
Rosy ◽  
Hadar Sclar ◽  
Eliran Evenstein ◽  
Shira Haber ◽  
Sandipan Maiti ◽  
...  

2019 ◽  
Vol 55 (21) ◽  
pp. 3109-3112 ◽  
Author(s):  
Iva Saric ◽  
Robert Peter ◽  
Maria Kolympadi Markovic ◽  
Ivana Jelovica Badovinac ◽  
Celia Rogero ◽  
...  

Different from other gas-phase methods, a novel pulsed vapor phase approach to copper-free surface click-chemistry by ALD processing is introduced.


2020 ◽  
Vol 496 (3) ◽  
pp. 3572-3581 ◽  
Author(s):  
M Popescu ◽  
J de León ◽  
C de la Fuente Marcos ◽  
O Vaduvescu ◽  
R de la Fuente Marcos ◽  
...  

ABSTRACT The first known asteroid with the orbit inside that of Venus is 2020 AV2. This may be the largest member of a new population of small bodies with the aphelion smaller than 0.718 au, called Vatiras. The surface of 2020 AV2 is being constantly modified by the high temperature, by the strong solar wind irradiation that characterizes the innermost region of the Solar system, and by high-energy micrometeorite impacts. The study of its physical properties represents an extreme test-case for the science of near-Earth asteroids. Here, we report spectroscopic observations of 2020 AV2 in the 0.5–1.5-μm wavelength interval. These were performed with the Nordic Optical Telescope and the William Herschel Telescope. Based on the obtained spectra, we classify 2020 AV2 as a Sa-type asteroid. We estimate the diameter of this Vatira to be $1.50_{-0.65}^{+1.10}$ km by considering the average albedo of A-type and S-complex asteroids ($p_V=0.23_{-0.08}^{+0.11}$), and the absolute magnitude (H = 16.40 ± 0.78 mag). The wide spectral band around 1 μm shows the signature of an olivine-rich composition. The estimated band centre BIC = 1.08 ± 0.02 μm corresponds to a ferroan olivine mineralogy similar to that of brachinite meteorites.


2007 ◽  
Vol 1040 ◽  
Author(s):  
L. E. Rodak ◽  
Sridhar Kuchibhatla ◽  
P. Famouri ◽  
Ting Liu ◽  
D. Korakakis

AbstractAluminum nitride (AlN) is a promising material for a number of applications due to its temperature and chemical stability. Furthermore, AlN maintains its piezoelectric properties at higher temperatures than more commonly used materials, such as Lead Zirconate Titanate (PZT) [1, 2], making AlN attractive for high temperature micro and nano-electromechanical (MEMs and NEMs) applications including, but not limited to, high temperature sensors and actuators, micro- channels for fuel cell applications, and micromechanical resonators.This work presents a novel AlN micro-channel fabrication technique using Metal Organic Vapor Phase Epitaxy (MOVPE). AlN easily nucleates on dielectric surfaces due to the large sticking coefficient and short diffusion length of the aluminum species resulting in a high quality polycrystalline growth on typical mask materials, such as silicon dioxide and silicon nitride [3,4]. The fabrication process introduced involves partially masking a substrate with a silicon dioxide striped pattern and then growing AlN via MOVPE simultaneously on the dielectric mask and exposed substrate. A buffered oxide etch is then used to remove the underlying silicon dioxide and leave a free standing AlN micro-channel. The width of the channel has been varied from 5 ìm to 110 ìm and the height of the air gap from 130 nm to 800 nm indicating the stability of the structure. Furthermore, this versatile process has been performed on (111) silicon, c-plane sapphire, and gallium nitride epilayers on sapphire substrates. Reflection High Energy Electron Diffraction (RHEED), Atomic Force Microscopy (AFM), and Raman measurements have been taken on channels grown on each substrate and indicate that the substrate is influencing the growth of the AlN micro-channels on the SiO2 sacrificial layer.


Author(s):  
Rosy ◽  
Sarah Taragin ◽  
Eliran Evenstein ◽  
Sebastian Maletti ◽  
Daria Mikhailova ◽  
...  

Author(s):  
Alexander L. Brown ◽  
Richard A. Jepsen

Because we want to be able to model fires from high energy impact events as found in transportation accidents, we are interested in accurate representation of secondary impacts and splash, which presumably contribute significantly to the outcome of the event. We are focused on a Lagrangian/Eulerian framework as a simulation method. Historically, drop impact modeling has been driven by spray combustion applications, as reviewed in a paper by Cossali et al. [1]. They note numerous deficiencies, including that regime accuracy for many of the models is narrow. Testing and model development has provided improved sub-models that have allowed us to construct what we believe to be a more accurate and comprehensive model for impacting drops. The details of this model are presented along with a detailed description of the sub-model components. The model is employed to predict a 10 cm diameter, 10 and 20 m/s water drop impact test. This test case serves as an initial verification and validation test of the implemented code.


1999 ◽  
Vol 4 (S1) ◽  
pp. 322-326 ◽  
Author(s):  
Eric Rehder ◽  
M. Zhou ◽  
L. Zhang ◽  
N. R. Perkins ◽  
S. E. Babcock ◽  
...  

The surface morphology and structure of AlN deposited by metal organic vapor phase epitaxy (MOVPE) on Si (111) at growth temperatures ranging from 825 to 1175°C was investigated. Transmission electron microscopy (TEM), reflection high energy electron diffraction (RHEED), atomic force microscopy (AFM), and secondary ion mass spectrometry (SIMS) techniques were used to study the resulting film structure. Growth at high temperatures but less than ∼1100°C, resulted in a wire texture with some degree of in-plane alignment with (0001)AlN/ /(111)Si, < 10 0>AlN//< 11>Si, and 110>AlN//<10>Si. Deposition at temperatures greater than 1100°C results in single crystal films consisting of domains 60 nm across with an aspect ratio near unity. Growth below1100°C leads to degraded crystal quality with the grains developing random rotational misalignments around the AlN [0001] axis. Growth at lower temperatures produces islands elongated along the [110] direction. At the growth temperature of 825°C, the aspect ratio of the islands increased to 3 and a width of 25 nm. Cross-sectional TEM reveals that these islands are faceted due to slow growth on the {1 01}planes.


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