Ferroelectricity, ionic conduction, and polar metals in hexagonal lead-apatite systems
ORAL
Abstract
The hexagonal apatites, A10(PO4)6X, where A = Ca, Pb or Bi, and X= F, Cl, or O) gained prominence after the recent contested claim of room-temperature superconductivity in Pb10−xCux(PO4)6O with x≈1. Apatites feature an approximate hexagonal close-packed structure with interstitial octahedral A-site channels in which X anions are mobile. Apatites like Ca10(VO4)6O, Pb10(PO4)6O and Bi9Li(SiO4)6O2 feature a non-centrosymmetric P63/m crystal structure and 2-3-eV band gaps. Here we report a DFT-based theoretical study of the structural and electronic properties of the pure and doped lead apatite system Pb10(PO4)6O. The primitive unit cell contains one formula unit with an even number of electrons, whereby replacing either a Pb or a channel O atom with an atom that has an odd number of electrons, one can generate metallic materials with an intriguing interplay of energy bands. Non-centrosymmetry is preserved. Thus, the doped materials are polar metals while the undoped materials are order-disorder ferroelectrics and ionic conductors in a way that is analogous to what happens in CuInP2S6 (CIPS). Here, it is the channel-ion sublattice that displaces in one of two directions, while more extended displacements can lead to ionic conduction. These insights can lead to novel applications.
Supported by DOE grant DE-FG-02-09ER46554 and DST-National Supercomputing Mission, File. No. DST/NSM/R&D_HPC_Applications/2021/34. Computations at NERSC and HPCC of the SRM.
Supported by DOE grant DE-FG-02-09ER46554 and DST-National Supercomputing Mission, File. No. DST/NSM/R&D_HPC_Applications/2021/34. Computations at NERSC and HPCC of the SRM.
* Supported by DOE grant DE-FG-02-09ER46554 and DST-National Supercomputing Mission, File. No. DST/NSM/R&D_HPC_Applications/2021/34. Computations at NERSC and HPCC of the SRM.
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Presenters
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M J Swamynadhan
SRM University
Authors
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M J Swamynadhan
SRM University
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Saurabh Ghosh
SRM Institute of Science and Technology KTR
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Sokrates T Pantelides
Department of Physics and Astronomy, Vanderbilt University