Predicting solid compounds via global exploration of the energy landscape of solids on the ab initio level without recourse to experimental information

2009 ◽  
Vol 247 (1) ◽  
pp. 23-39 ◽  
Author(s):  
J. Christian Schön ◽  
Klaus Doll ◽  
Martin Jansen
2011 ◽  
Vol 123 (20) ◽  
pp. 4723-4728 ◽  
Author(s):  
Klaus Doll ◽  
Martin Jansen
Keyword(s):  

Nanoscale ◽  
2020 ◽  
Vol 12 (20) ◽  
pp. 10994-11000
Author(s):  
Gabriele Tocci ◽  
Maria Bilichenko ◽  
Laurent Joly ◽  
Marcella Iannuzzi

Ab initio molecular dynamics reveals that subtle variations in the energy landscape and density correlations can change by up to one order of magnitude the slippage of water on two-dimensional materials.


2019 ◽  
Vol 1 (5) ◽  
pp. 1924-1935
Author(s):  
Sergio Conejeros ◽  
Neil L. Allan ◽  
Frederik Claeyssens ◽  
Judy N. Hart

Ab initio energy landscapes of thin ZnO and ZnS films reveal new structures, non-stoichiometry and different behaviour of adsorbed water.


2009 ◽  
Vol 1229 ◽  
Author(s):  
Flemming JH Ehlers ◽  
Randi Holmestad

AbstractA dramatic gain in the knowledge of precipitate formation, composition, and evolution in alloys has been achieved in the recent years with improvement of transmission electron microscopy techniques for direct structural imaging [1]. A detailed understanding of the microstructure is often essential for control and manipulation of materials properties: an important example for metals is the significant hardening of Al alloys by particular precipitates from a sequence strongly dependent on alloying element concentration and the treatment of the material [2]. The wealth of experimental information provides a playground for theory in the context of elucidating precipitate growth mechanisms and influence on the host material. A head-on approach to atomistic modelling of these phenomena using an ab initio based scheme is conventionally deemed highly desired but impractical. The basic argument is that the system of any reasonably sized (i.e. realistic) and well isolated microstructure will simply contain too many atoms. We will challenge this conventional view: it is argued that most of the atoms of the above mentioned system do not play an active role in the growth discussion, hence need not be included in the modelling. Subsequently, a model system is presented which offers a highly accurate description of the interface between the host lattice and a microstructure of an arbitrary size, for the case where this interface is coherent and compositionally abrupt. When used in conjunction with other approaches already available, this model system offers a direct approach to atomistic ab initio studies of microstructure growth. A general introduction to the modelling scheme will be presented, with the particular application being the main hardening precipitate β'' in the Al-Mg-Si alloy. [1] K. W. Urban, Nature Mater. 8, 260 (2009). [2] C. D. Marioara, S. J. Andersen, H. W. Zandbergen, and R. Holmestad, Metal. Mater. Trans. A 36A, 691 (2005).


2011 ◽  
Vol 135 (3) ◽  
pp. 034102 ◽  
Author(s):  
Eduardo Machado-Charry ◽  
Laurent Karim Béland ◽  
Damien Caliste ◽  
Luigi Genovese ◽  
Thierry Deutsch ◽  
...  

2014 ◽  
Vol 47 (6) ◽  
pp. 2100-2104 ◽  
Author(s):  
Anders Østergaard Madsen ◽  
Anna A. Hoser

A major update of theSHADEserver (http://shade.ki.ku.dk) is presented. In addition to all of the previous options for estimating H-atom anisotropic displacement parameters (ADPs) that were offered bySHADE2, the newest version offers two new methods. The first method combines the original translation–libration–screw analysis with input from periodicab initiocalculations. The second method allows the user to input experimental information from spectroscopic measurements or from neutron diffraction experiments on related structures and utilize this information to evaluate ADPs of H atoms. Tools are provided to set up theab initiocalculations and to derive the internal motion from the calculations. The new server was tested on a range of compounds where neutron diffraction data were available. In most cases, the results are significantly better than previous estimates, and for strong hydrogen bonds in proton sponges, theab initiocalculations become crucial.


2007 ◽  
Vol 9 (46) ◽  
pp. 6128 ◽  
Author(s):  
K. Doll ◽  
J. C. Schön ◽  
M. Jansen
Keyword(s):  

1972 ◽  
Vol 25 (8) ◽  
pp. 1601 ◽  
Author(s):  
L Radom ◽  
WA Lathan ◽  
WJ Hehre ◽  
JA Pople

Ab initio molecular orbital theory is used to study internal rotation in 20 organic molecules of the types X-Y, X-CH2-Y, X-SH-Y, X-O-Y, and X-CO-Y-where X and Y are methyl, amino, hydroxy, or formyl groups. In some of these molecules, internal rotation about two bonds is possible. The theoretical results are generally in moderate agreement with available experimental data and, in addition, lead to a number of predictions for molecules for which experimental information is lacking.


2012 ◽  
Vol 45 (1) ◽  
pp. 111-115 ◽  
Author(s):  
I. M. Markus ◽  
N. Adelstein ◽  
M. Asta ◽  
L. C. DeJonghe

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