From one to three, exploring the rungs of Jacob’s ladder in magnetic alloys

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Abstract

Magnetic systems represent an important challenge for electronic structure methods, in particular Density Functional Theory (DFT), which uses a single determinant wavefunction. To assess the predictions obtained by DFT in this type of materials, we benchmark different exchange correlation functionals with respect to each other, and with respect to available experimental data, on two families of binary iron alloys which are metallic and magnetic. We climb three rungs in Jacob’s ladder of DFT (i) the local density approximation, (ii) the industry standard approximation due to Perdew, Burke and Ernzerhof, and the revised version for solids, PBEsol (iii) and finally a very accurate meta-GGA functional SCAN, which corresponds to the third rung. More than 350 structures in ferromagnetic and antiferromagnetic configurations were considered. We compare the Convex Hull, the calculated magnetic moment, crystal structure, formation energy and electronic gap if present. We conclude that none of the functionals work in all conditions: whereas PBE and PBEsol can give a fair description of the crystal structure and the energetics, SCAN strongly overestimates the formation energy – giving values which are at least twice as large as PBE (and experiment). Magnetic moments are better predicted by PBE as well. Our results show that magnetic and strongly correlated materials are a tough litmus test for DFT, and that they represent the next frontier in the development of a truly universal exchange correlation functionals.

Original languageEnglish
Article number193
JournalEuropean Physical Journal B
Volume91
Issue number8
DOIs
Publication statusPublished - 1 Aug 2018
Externally publishedYes

Bibliographical note

Publisher Copyright:
© 2018, EDP Sciences, SIF, Springer-Verlag GmbH Germany, part of Springer Nature.

Funding

This work has been carried out in honor of Hardy Gross for his 65th birthday. He has been an excellent collaborator, an exceptional teacher and above all a very good friend. The project was carried out initially for fun, in a spirit of exploration and “what happens if”, which Hardy has always extolled as the true method of science. The authors acknowledge useful discussions with Gian-Marco Rignanese, Stefano Curtarolo, and Geoffroy Hautier. This work used the XSEDE which is supported by National Science Foundation grant number ACI-1053575. The authors also acknowledge the support from the Texas Advances Computer Center (with the Stampede2 and Bridges supercomputers), the Belgian Consortium des Equipements de Calcul Intensif en Fédération Wallonie Bruxelles (CECI), funded by the Fonds de la Recherche Scientifique de Belgique (FRS-FNRS) under convention 2.5020.11, and Zenobe tier-1 funded by CENAERO and the Walloon Region under G.A. 1117545. This work was supported by the DMREF-NSF 1434897, NSF OAC-1740111 and DOE DE-SC0016176 projects, and by the CommunautéFranc¸aise de Belgique Actions de Recherches Concertées project AIMED (GA 15/19-09).

FundersFunder number
Belgian Consortium des Equipements de Calcul Intensif en Fédération Wallonie Bruxelles
CECI
CENAERO
CommunautéFranc¸aise de Belgique Actions de Recherches Concertées project AIMEDGA 15/19-09
DMREF-NSF1434897
Texas Advances Computer Center
Walloon Region1117545
XSEDE
National Science Foundation1740111, OAC-1740111, ACI-1053575
U.S. Department of EnergyDE-SC0016176
Institut national de la recherche scientifique2.5020.11

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