scholarly journals Large area nanoimprint enables ultra-precise x-ray diffraction gratings

2017 ◽  
Vol 25 (19) ◽  
pp. 23334 ◽  
Author(s):  
D. L. Voronov ◽  
E. M. Gullikson ◽  
H. A. Padmore
1982 ◽  
Vol 21 (15) ◽  
pp. 2787 ◽  
Author(s):  
Shinji Matsui ◽  
Kazuyuki Moriwaki ◽  
Hiroaki Aritome ◽  
Susumu Namba ◽  
Shik Shin ◽  
...  

1996 ◽  
Vol 449 ◽  
Author(s):  
L.J. Lauhon ◽  
S. A. Ustin ◽  
W. Ho

ABSTRACTAlN, GaN, and SiC thin films were grown on 100 mm diameter Si(111) and Si(100) substrates using Supersonic Jet Epitaxy (SJE). Precursor gases were seeded in lighter mass carrier gases and free jets were formed using novel slit-jet apertures. The jet design, combined with substrate rotation, allowed for a uniform flux distribution over a large area of a 100 mm wafer at growth pressures of 1–20 mTorr. Triethylaluminum, triethylgailium, and ammonia were used for nitride growth, while disilane, acetylene, and methylsilane were used for SiC growth. The films were characterized by in situ optical reflectivity, x-ray diffraction (XRD), atomic force microscopy (AFM), and spectroscopic ellipsometry (SE).


Author(s):  
H. I. Smith ◽  
E. H. Anderson ◽  
A. M. Hawryluk ◽  
M. L. Schattenburg

1997 ◽  
Author(s):  
Ulf Kleineberg ◽  
Hans-Juergen Stock ◽  
D. Menke ◽  
O. Wehmeyer ◽  
Ulrich Heinzmann ◽  
...  

2020 ◽  
Vol 27 (5) ◽  
pp. 1447-1458 ◽  
Author(s):  
Daryl L. Howard ◽  
Martin D. de Jonge ◽  
Nader Afshar ◽  
Chris G. Ryan ◽  
Robin Kirkham ◽  
...  

The X-ray fluorescence microscopy (XFM) beamline is an in-vacuum undulator-based X-ray fluorescence (XRF) microprobe beamline at the 3 GeV Australian Synchrotron. The beamline delivers hard X-rays in the 4–27 keV energy range, permitting K emission to Cd and L and M emission for all other heavier elements. With a practical low-energy detection cut-off of approximately 1.5 keV, low-Z detection is constrained to Si, with Al detectable under favourable circumstances. The beamline has two scanning stations: a Kirkpatrick–Baez mirror microprobe, which produces a focal spot of 2 µm × 2 µm FWHM, and a large-area scanning `milliprobe', which has the beam size defined by slits. Energy-dispersive detector systems include the Maia 384, Vortex-EM and Vortex-ME3 for XRF measurement, and the EIGER2 X 1 Mpixel array detector for scanning X-ray diffraction microscopy measurements. The beamline uses event-mode data acquisition that eliminates detector system time overheads, and motion control overheads are significantly reduced through the application of an efficient raster scanning algorithm. The minimal overheads, in conjunction with short dwell times per pixel, have allowed XFM to establish techniques such as full spectroscopic XANES fluorescence imaging, XRF tomography, fly scanning ptychography and high-definition XRF imaging over large areas. XFM provides diverse analysis capabilities in the fields of medicine, biology, geology, materials science and cultural heritage. This paper discusses the beamline status, scientific showcases and future upgrades.


2014 ◽  
Vol 996 ◽  
pp. 162-168 ◽  
Author(s):  
Andrei Benediktovitch ◽  
Tatjana Ulyanenkova ◽  
Jozef Keckes ◽  
Alex Ulyanenkov

X-ray residual stress analysis is a widespread nondestructive technique to investigate the residual stress and residual stress gradient in thin films and protective coatings.In the present contribution we introduce a new method based on the noncomplanar measurement geometry that allow to span large area of sin2ψ and penetration depth values without sample inclination. The refraction correction and absorption is considered in details for the noncomplanar measurements. The proposed technique is applied to determine stress gradients of blasted hard TiN coatings.


2012 ◽  
Author(s):  
A. Konstantinidis ◽  
T. Anaxagoras ◽  
M. Esposito ◽  
N. Allinson ◽  
R. Speller

2010 ◽  
Vol 25 (12) ◽  
pp. 2426-2429 ◽  
Author(s):  
Guangjun Wang ◽  
Gang Cheng ◽  
Binbin Hu ◽  
Xiaoli Wang ◽  
Shaoming Wan ◽  
...  

In this paper, polycrystalline CuIn(SxSe1–x)2 thin films with tunable x and Eg (band gap) values were prepared by controlling the sulfurization temperature (T) of CuInSe2 thin films. X-ray diffraction indicated the CuIn(SxSe1–x)2 films exhibited a homogeneous chalcopyrite structure. When T increases from 150 to 500 °C, x increases from 0 to 1, and Eg increases from 0.96 to 1.43 eV. The relations between x and Eg and the sulfurization process of CuIn(SxSe1–x)2 thin films have been discussed. This work provides an easy and low-cost technique for preparing large area absorber layers of solar cell with tunable Eg.


2014 ◽  
Vol 493 ◽  
pp. 012019 ◽  
Author(s):  
A C Thompson ◽  
E M Westbrook ◽  
W M Lavender ◽  
J C Nix

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