Analytical second derivatives in the Amsterdam density functional package

2005 ◽  
Vol 104 (5) ◽  
pp. 645-659 ◽  
Author(s):  
Stephen K. Wolff
2016 ◽  
Vol 38 (4) ◽  
pp. 238-249 ◽  
Author(s):  
Danny Schlüns ◽  
Mirko Franchini ◽  
Andreas W. Götz ◽  
Johannes Neugebauer ◽  
Christoph R. Jacob ◽  
...  

1997 ◽  
Vol 100 (3) ◽  
pp. 263-276 ◽  
Author(s):  
Heiko Jacobsen ◽  
Attila Bérces ◽  
David P. Swerhone ◽  
Tom Ziegler

2014 ◽  
Vol 997 ◽  
pp. 85-88
Author(s):  
Biao Yan ◽  
Hong Yu Zhou

3-Amino-4-aminoximidofurazan (AAOF) and 3-Amino-4-chloroximidofurazan (ACOF) are important precursor of synthesizing new furazanon (furoxano) energetic compounds. The density functional theory (DFT) method of the Amsterdam density functional (ADF) was used to calculate the geometry and frequency of AAOF and ACOF. The detonation velocity (D) and pressure (P) of the two compounds were estimated using the nitrogen equivalent equation according to the experimental density. Results showed that the initial decomposition step of AAOF and ACOF is the loss of OH from N4, the changed in group have some effect on HOMO, but this have little effect on HOMO, AAOF has better thermal stability and detonation performance than ACOF.


2001 ◽  
Vol 65 (2) ◽  
pp. 181-191 ◽  
Author(s):  
P. Martin ◽  
G. D. Price ◽  
L. Vočadlo

AbstractAn investigation into the relative stabilities and equations of state of stoichiometric FeS was conducted using first-principles pseudopotential calculations. These calculations were based on density functional theory and performed using ultrasoft Vanderbilt pseudopotentials within the generalized gradient approximation. We have identified four stable polymorphs of FeS along the 0 K isotherm as a function of pressure: troilite, an orthorhombic MnP-type structure, a monoclinic structure, and a CsCl-type structure. The calculated internal energy as a function of volume for each polymorph was fitted to 4th order logarithmic and 3rd order Birch-Murnaghan equations of state, yielding values for the bulk modulus, K, and its first and second derivatives with respect to pressure, K′ and K″. These equations of state may be used to characterize models of planetary cores.


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