arXiv · 2010.07168
The Tin Pest Problem as a Test of Density Functionals Using High-Throughput Calculations
Abstract
At ambient pressure tin transforms from its ground-state semi-metal $\alpha$-Sn (diamond structure) phase to the compact metallic $\beta$-Sn phase at 13$^\circ$C (286K). There may be a further transition to the simple hexagonal $\gamma$-Sn above 450K. These relatively low transition temperatures are due to the small energy differences between the structures, $\approx 20$\,meV/atom between $\alpha$- and $\beta$-Sn. This makes tin an exceptionally sensitive test of the accuracy of density functionals and computational methods. Here we use the high-throughput Automatic-FLOW (AFLOW) method to study the energetics of tin in multiple structures using a variety of density functionals. We look at the successes and deficiencies of each functional. As no functional is completely satisfactory, we look Hubbard U corrections and show that the Coulomb interaction can be chosen to predict the correct phase transition temperature. We also discuss the necessity of testing high-throughput calculations for convergence for systems with small energy differences.
Explore related subjects
Keep this discovery
Michael J. Mehl, Mateo Ronquillo, David Hicks, Marco Esters, Corey Oses, Rico Friedrich, Andriy Smolyanyuk, Eric Gossett, Daniel Finkenstadt, Stefano Curtarolo. 2020-10-14. The Tin Pest Problem as a Test of Density Functionals Using High-Throughput Calculations. https://doi.org/10.1103/physrevmaterials.5.083608
Cite the original work for its findings. Save a collection to share your selection of sources.