Computer simulations of nearest-neighbor distribution functions and related quantities for hard-sphere systems

1990 ◽  
Vol 167 (2) ◽  
pp. 361-383 ◽  
Author(s):  
S. Torquato ◽  
Sang Bub Lee
2000 ◽  
Vol 17 (3) ◽  
pp. 351-356 ◽  
Author(s):  
Soong-Hyuck Suh ◽  
Woong-Ki Min ◽  
Viorel Chihaia ◽  
Jae-Wook Lee ◽  
Soon-Chul Kim

2004 ◽  
Vol 848 ◽  
Author(s):  
Ariel A. Valladares ◽  
Alexander Valladares ◽  
R. M. Valladares ◽  
A. Calles

AbstractLiquid and amorphous metallic systems have proven difficult to model. Some efforts have relied on the use of parameterized classical potentials of the Lennard-Jones type or geometric hard sphere simulations, but first principles approaches have been rarely used. Clearly a knowledge of atomic structures is paramount for calculating physical properties. In this work we apply our recently developed ab initio DFT approach (A. A. Valladares et al., Eur. Phys. J. 22 (2001) 443) for the generation of amorphous semiconducting materials, to amorphize aluminum and an aluminum-nitrogen alloy. We report radial distribution functions (RDFs) and specific atomic structures of periodic amorphous/liquid cubic supercells of 108 atoms with a volume of (12.1485 Å)3, generated using the Harris functional.


1967 ◽  
Vol 160 (1) ◽  
pp. 225-236 ◽  
Author(s):  
A. Isihara ◽  
Arun K. Gupta

2013 ◽  
Author(s):  
Suvendu Mandal ◽  
Markus Gross ◽  
Dierk Raabe ◽  
Fathollah Varnik

1980 ◽  
Vol 35 (4) ◽  
pp. 412-414
Author(s):  
K. N. Swamy ◽  
P. C. Wankhede

Abstract The optimised cluster theory of Andersen and Chandler has been applied to calculate the radial distribution functions of a triangular well fluid with the width a the hard sphere diameter The results agree well with Monte Carlo Calculations of Card and Walkley.


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