Physical Properties of Grain-Boundary Materials: Comparison of EAM and Central-Force Potentials

Author(s):  
D. Wolf ◽  
J. Lutsko ◽  
M. Kluge
Alloy Digest ◽  
1993 ◽  
Vol 42 (8) ◽  

Abstract SUMITOMO 347AP is similar to what could be called Type 347LN and was developed to prevent polythionic acid cracking in chromium depleted grain boundary areas. The columbium (niobium) content is maintained at a ratio of greater than 15 times the carbon in addition to maintaining very low carbon levels. This datasheet provides information on composition, physical properties, hardness, elasticity, and tensile properties as well as creep. It also includes information on forming, heat treating, and joining. Filing Code: SS-548. Producer or source: Sumitomo Metal USA Corporation.


2012 ◽  
Vol 506 ◽  
pp. 234-237
Author(s):  
N. Lertcumfu ◽  
P. Jarupoom ◽  
Kamonpan Pengpat ◽  
T. Tunkasiri ◽  
Gobwute Rujijanagul

In the present study the effects of metal oxide nanoparticles addition on the microstructure, physical properties of the HA ceramics were investigated. Many techniques were used for the analysis. X-ray diffraction analysis revealed a co-exist phases between hydroxyapatite and tricalcium phosphate in the sintered samples. Addition of NiO resulted an increase in the lattice parameters of the tricalcium phosphates due to the bigger radii atom (Ni) substitution for the small radii atom (Ca). Energy dispersive spectroscopy suggested that most of NiO particles located at grain boundary, resulting in an improvement of hardness of the samples


2006 ◽  
Vol 530-531 ◽  
pp. 444-448
Author(s):  
A.P.P. Fontanesi ◽  
J.M. Cavenaghi ◽  
Vania Caldas de Sousa

Dopants such as Ta2O5 play a major role in the formation of barriers at the grain boundary in TiO2 varistors, increasing their nonlinear coefficient and decreasing their breakdown electric field. This paper discusses the microstructural and physical properties of Ta- and Cr-doped TiO2 systems in which imported tantalum oxide was replaced with an equivalent Brazilian raw material. Preliminary results confirm that this national oxide can be utilized to obtain electroceramics such as varistors.


2018 ◽  
Vol 217 ◽  
pp. 468-476
Author(s):  
Gomathi Natarajan ◽  
Niranjan Kumar ◽  
Ramanathaswamy Pandian ◽  
S. Amirthapandian

Alloy Digest ◽  
1994 ◽  
Vol 43 (4) ◽  

Abstract CM 186 LC is a rhenium-containing, directionally solidified (DS) superalloy. It has excellent DS castability and above average resistance to grain boundary cracking in complex cored, thin wall turbine airfoils. This datasheet provides information on composition and physical properties as well as creep. It also includes information on casting and heat treating. Filing Code: Ni-450. Producer or source: Cannon-Muskegon Corporation.


2016 ◽  
Vol 675-676 ◽  
pp. 303-306
Author(s):  
Sutee Chantrapakajee ◽  
Piyamas Chainok ◽  
Supphadate Sujinnapram ◽  
Thanarat Khuntak ◽  
Tunyanop Nilkamjon ◽  
...  

Abstract. In this research, we synthesized and investigate the physical properties of YBaCuO superconductor; Y123 and Y13-20-30. The melt process was used for heat treatment of our samples. We found that the critical temperature onset of Y13-20-33 and Y123 were at 90 K and 94 K, respectively. The morphology of Y123 superconductor has flat surface and more clear grain boundary than Y13-20-33 superconductor. However, more melted of grain boundary were found on Y13-20-33. Both samples were the orthorhombic crystal structure that c/a ratio of Y13-20-33 was higher than of Y123 superconductor.


1999 ◽  
Vol 8 (6) ◽  
pp. 996-1005 ◽  
Author(s):  
J.W. Steeds ◽  
A. Gilmore ◽  
K.M. Bussmann ◽  
J.E. Butler ◽  
P. Koidl

1976 ◽  
Vol 32 ◽  
pp. 365-377 ◽  
Author(s):  
B. Hauck
Keyword(s):  

The Ap stars are numerous - the photometric systems tool It would be very tedious to review in detail all that which is in the literature concerning the photometry of the Ap stars. In my opinion it is necessary to examine the problem of the photometric properties of the Ap stars by considering first of all the possibility of deriving some physical properties for the Ap stars, or of detecting new ones. My talk today is prepared in this spirit. The classification by means of photoelectric photometric systems is at the present time very well established for many systems, such as UBV, uvbyβ, Vilnius, Geneva and DDO systems. Details and methods of classification can be found in Golay (1974) or in the proceedings of the Albany Colloquium edited by Philip and Hayes (1975).


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