Observation of a metal-to-insulator transition with both Mott-Hubbard and Slater characteristics in Sr2IrO4 from time-resolved photocarrier dynamics
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Hsieh-2012-Observation of a metal-to-insulator transition with both Mott-Hubbard.pdf
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Author(s)
Hsieh, David
Mahmood, Fahad
Torchinsky, Darius Hosseinzadeh
Cao, Gang
Gedik, Nuh
Date Issued
July 2012
Journal
Physical Review B
Publisher
American Physical Society
Citation
Hsieh, D. et al. “Observation of a Metal-to-insulator Transition with Both Mott-Hubbard and Slater Characteristics in Sr[subscript 2]IrO[subscript 4] from Time-resolved Photocarrier Dynamics.” Physical Review B 86.3 (2012). ©2012 American Physical Society
Version
Final published version
Abstract
We perform a time-resolved optical study of Sr[subscript 2]IrO[subscript 4] to understand the influence of magnetic ordering on the low energy electronic structure of a strongly spin-orbit coupled J[subscript eff] = 1/2 Mott insulator. By studying the recovery dynamics of photoexcited carriers, we find that upon cooling through the Néel temperature T[subscript N] the system evolves continuously from a metal-like phase with fast (∼50 fs) and excitation density independent relaxation dynamics to a gapped phase characterized by slower (∼500 fs) excitation density-dependent bimolecular recombination dynamics, which is a hallmark of a Slater-type metal-to-insulator transition. However our data indicate that the high energy reflectivity associated with optical transitions into the unoccupied J[subscript eff] = 1/2 band undergoes the sharpest upturn at T[subscript N], which is consistent with a Mott-Hubbard type metal-to-insulator transition involving spectral weight transfer into an upper Hubbard band. These findings show Sr[subscript 2]IrO[subscript 4] to be a unique system in which Slater- and Mott-Hubbard-type behaviors coexist and naturally explain the absence of anomalies at T[subscript N] in transport and thermodynamic measurements.
MIT Department
Massachusetts Institute of Technology. Department of Physics
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DOI of Published Version
http://dx.doi.org/10.1103/PhysRevB.86.035128
