Generalized quasiharmonic approximation via space group irreducible derivatives

Mark A. Mathis, Amey Khanolkar, Lyuwen Fu, Matthew S. Bryan, Cody A. Dennett, Karl Rickert, J. Matthew Mann, Barry Winn, Douglas L. Abernathy, Michael E. Manley, David H. Hurley, Chris A. Marianetti

Research output: Contribution to journalArticlepeer-review

12 Scopus citations

Abstract

The quasiharmonic approximation (QHA) is the simplest nontrivial approximation for interacting phonons under constant pressure, bringing the effects of anharmonicity into temperature-dependent observables. Nonetheless, the QHA is often implemented with additional approximations due to the complexity of computing phonons under arbitrary strains, and the generalized QHA, which employs constant stress boundary conditions, has not been completely developed. Here we formulate the generalized QHA, providing a practical algorithm for computing the strain state and other observables as a function of temperature and true stress. We circumvent the complexity of computing phonons under arbitrary strains by employing irreducible second-order displacement derivatives of the Born-Oppenheimer potential and their strain dependence, which are efficiently and precisely computed using the lone irreducible derivative approach. We formulate two complementary strain parametrizations: a discretized strain grid interpolation and a Taylor series expansion in symmetrized strain. We illustrate our approach by evaluating the temperature and pressure dependence of select elastic constants and the thermal expansion in thoria (ThO2) using density functional theory with three exchange-correlation functionals. The QHA results are compared to our measurements of the elastic constant tensor using time-domain Brillouin scattering and inelastic neutron scattering. Our irreducible derivative approach simplifies the implementation of the generalized QHA, which will facilitate reproducible, data-driven applications.

Original languageEnglish
Article number014314
JournalPhysical Review B
Volume106
Issue number1
DOIs
StatePublished - Jul 1 2022

Funding

The development of the generalized QHA formalism by M.A.M. and C.A.M, first-principles calculations by M.A.M., L.F., and C.A.M., sample growth and analysis by K.R. and J.M.M., TDBS by A.K., C.A.D., and D.H.H., and INS measurements by M.S.B. and M.E.M. were supported by the Center for Thermal Energy Transport Under Irradiation (TETI), an Energy Frontier Research Center funded by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences. The symmetrized strain Taylor series by M.A.M., L.F., and C.A.M. was supported by Grant No. DE-SC0016507 funded by the U.S. Department of Energy, Office of Science. The computational research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. A portion of this research used resources at Spallation Neutron Source, a DOE Office of Science User Facility operated by the Oak Ridge National Laboratory.

FundersFunder number
Center for Thermal Energy Transport
U.S. Department of Energy
Office of ScienceDE-AC02-05CH11231
Basic Energy SciencesDE-SC0016507

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