Investigation of block depth distribution in PS-b-PMMA block copolymer using ultra-low-energy cesium sputtering in ToF-SIMS

2013 ◽  
Vol 46 (2) ◽  
pp. 83-91 ◽  
Author(s):  
T. Terlier ◽  
R. Tiron ◽  
A. Gharbi ◽  
X. Chevalier ◽  
M. Veillerot ◽  
...  
2010 ◽  
Vol 43 (1-2) ◽  
pp. 179-182 ◽  
Author(s):  
M. Py ◽  
J. P. Barnes ◽  
M. Charbonneau ◽  
R. Tiron ◽  
J. Buckley

2008 ◽  
Vol 255 (4) ◽  
pp. 1331-1333 ◽  
Author(s):  
R.G. Vitchev ◽  
J. Brison ◽  
L. Houssiau

2020 ◽  
Vol 1004 ◽  
pp. 581-586
Author(s):  
Judith Woerle ◽  
Thomas Prokscha ◽  
Ulrike Grossner

In this work, the potential of muon spin rotation (μSR) with low-energy muons (LE-μ) for the investigation of oxidation-induced defects at the SiO2/4H-SiC interface is explored. By using implantation energies for the muons in the keV range and comparing the fractions of muonium in different regions, the depth distribution of defects in the first 200 nm of the target material can be resolved. Defect profiles of interfaces with either deposited or thermally grown SiO2 layers on 4H-SiC are compared. The results show an increased number of defects in the case of a thermal oxide, both on the oxide and on the SiC side of the interface, with a spatial extension of a few tens of nm.


2020 ◽  
Vol 501 ◽  
pp. 144266 ◽  
Author(s):  
Nicolas Gauthier ◽  
Cécile Courrèges ◽  
Julien Demeaux ◽  
Cécile Tessier ◽  
Hervé Martinez

1994 ◽  
Vol 38 ◽  
pp. 291-298
Author(s):  
B. Schoβmann ◽  
J. Wernisch ◽  
H. Ebel

We have developed an algorithm for calculating the x-ray tube continuum based on the depth distribution function (DDF) proposed by Pochou and Pichoir, extended the description of white and characteristic radiation given by Wiederschwinger et al. to the low energy range from 5 to 30 keV and compared the results frorn these algorithms to the signals obtained from algorithms using the absorption correction of Philibert and of Sewell et al. Preceding calculations the measured spectra were separated into characteristic peak spectra and into the corresponding white spectra, where the background below the peak areas was numerically interpolated.


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