The Effect of Rare Earth on the Clearance of Carbon during High Speed Polishing of Diamond Films

2011 ◽  
Vol 697-698 ◽  
pp. 137-141
Author(s):  
Li Zhou ◽  
Shu Tao Huang ◽  
L.F. Xu

A new setup for polishing of diamond films on a high speed rotating stainless plate has been developed, and a rare earth metal plate was used to clear the carbon atoms diffused into the polishing plate. The surface morphology and clearance mechanism were studied by using scanning electron microscopy and X-ray photo-electron spectroscopy before and after polishing, respectively. The results showed that the chemical reaction between the rare earth metal and carbon diffused into the polishing plate took place and the rare earth metal could clear the carbon element effectively during the super-high speed polishing.

2014 ◽  
Vol 32 (11) ◽  
pp. 1073-1079 ◽  
Author(s):  
Ruiying MIAO ◽  
Xiaowei ZHANG ◽  
Qiong ZHU ◽  
Zhiqi ZHANG ◽  
Zhiqiang WANG ◽  
...  

2006 ◽  
Vol 61 (1) ◽  
pp. 17-22 ◽  
Author(s):  
Anette Imre ◽  
Albrecht Mewis

The new compounds Pr3Pd6Sb5 (a = 13.442(3), b = 4.442(1), c = 9.994(2) Å ), Nd3Pd6Sb5 (a = 13.412(3), b = 4.431(1), c = 9.962(2) Å), and Gd3Pd6Sb5 (a = 13.293(2), b = 4.397(1), c = 9.881(2) Å) are isotypic and crystallize with the Ce3Pd6Sb5 type structure (Pmmn; Z = 2). The rare-earth metal atoms are arranged in form of three pseudo-body-centered subcells, whereas Pd and Sb atoms form a three-dimensional arrangement derived from the well-known ThCr2Si2 and CaBe2Ge2 structures. GdPdSb (a = 4.566(1), c = 7.444(1) Å) and DyPdSb (a = 4.545(1), c = 7.354(1) Å) crystallize with an ordered variant of the CaIn2 type structure (P63mc; Z = 2), also called as LiGaGe type, with slightly puckered hexagon nets of Pd and Sb atoms, which trigonally coordinate each other. In this series a decreasing radius of the rare-earth metal allows a tetrahedral non-metal environment of the Pd atoms and accordingly ScPdSb (a = 6.310(1) Å) forms the MgAgAs type structure (F4̄3m; Z = 4), a filled variant of the sphalerite type. The antimonides were prepared by heating mixtures of the elements at 600 °C and subsequent annealing at 900 - 1100 °C. Their structures have been determined by single-crystal X-ray methods.


1983 ◽  
Vol 90 (2) ◽  
pp. 217-222 ◽  
Author(s):  
Yu.B. Kuz'ma ◽  
N.S. Bilonizhko ◽  
N.F. Chaban ◽  
G.V. Chernyak

1983 ◽  
Vol 14 (30) ◽  
Author(s):  
YU. B. KUZ'MA ◽  
N. S. BILONIZHKO ◽  
N. F. CHABAN ◽  
G. V. CHERNYAK

1985 ◽  
Vol 57 (8) ◽  
pp. 3619-3622 ◽  
Author(s):  
Doon Gibbs ◽  
D. E. Moncton ◽  
K. L. D’Amico

1981 ◽  
Vol 82 ◽  
pp. 364 ◽  
Author(s):  
Yu B. Kuz'ma ◽  
N.S Bilonizhko ◽  
N.F Chaban ◽  
G.V Chernjak

2020 ◽  
Vol 0 (0) ◽  
Author(s):  
Michael Zoller ◽  
Hubert Huppertz

AbstractThe rare earth oxoborates REB5O8(OH)2 (RE = Ho, Er, Tm) were synthesized in a Walker-type multianvil apparatus at a pressure of 2.5 GPa and a temperature of 673 K. Single-crystal X-ray diffraction data provided the basis for the structure solution and refinement. The compounds crystallize in the monoclinic space group C2 (no. 5) and are composed of a layer-like structure containing dreier and sechser rings of corner sharing [BO4]5− tetrahedra. The rare earth metal cations are coordinated between two adjacent sechser rings. Further characterization was performed utilizing IR spectroscopy.


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