TY - JOUR
T1 - Charge dynamics and metal-insulator transition in perovskite SrIr1−xSnxO3
AU - Fujioka, Jun
AU - Okawa, Tatsuya
AU - Masuko, Makoto
AU - Yamamoto, Ayako
AU - Tokura, Yoshinori
N1 - Funding Information:
Acknowledgment We thank S. Sakai, M. Hirayama, and R. Arita for useful discussions. This work was partly supported by Grant-in-Aid for Science Research (Nos. 16H00981, 18H04214, 18H01171) from the MEXT, and by PRESTO (No. JPMJPR15R5) and CREST (No. JPMJCR16F1), Japan Science and Technology Japan.
Funding Information:
We thank S. Sakai, M. Hirayama, and R. Arita for usefu discussions. This work was partly supported by Grant-in-Aid for Science Research (Nos. 16H00981, 18H04214, 18H01171) from the MEXT, and by PRESTO (No. JPMJPR15R5) and CREST (No. JPMJCR16F1), Japan Science and Technology Japan.
Publisher Copyright:
©2018 The Physical Society of Japan
PY - 2018
Y1 - 2018
N2 - We investigate the variation of charge dynamics upon the metal-insulator transition for perovskite SrIr1−xSnxO3 by employing the optical spectroscopy. The Dirac semimetal of SrIrO3 turns into the antiferromagnetic insulator with a gap of 0.1 eV by the Sn-substitution, accompanying the reconstruction of electronic structure on an energy scale of 1 eV. The spectral intensity of optical excitation between Jeff = 1=2-orbitals is significantly reduced with increasing x, while that between the Jeff = 3=2- and 1=2-orbital shows merely moderate x-dependence. We anticipate that the substituted Sn significantly renormalizes the effective bandwidth of Jeff = 1=2-orbital while modestly changing the Jeff = 3=2-orbital.
AB - We investigate the variation of charge dynamics upon the metal-insulator transition for perovskite SrIr1−xSnxO3 by employing the optical spectroscopy. The Dirac semimetal of SrIrO3 turns into the antiferromagnetic insulator with a gap of 0.1 eV by the Sn-substitution, accompanying the reconstruction of electronic structure on an energy scale of 1 eV. The spectral intensity of optical excitation between Jeff = 1=2-orbitals is significantly reduced with increasing x, while that between the Jeff = 3=2- and 1=2-orbital shows merely moderate x-dependence. We anticipate that the substituted Sn significantly renormalizes the effective bandwidth of Jeff = 1=2-orbital while modestly changing the Jeff = 3=2-orbital.
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U2 - 10.7566/JPSJ.87.123706
DO - 10.7566/JPSJ.87.123706
M3 - Article
AN - SCOPUS:85057625649
SN - 0031-9015
VL - 87
JO - Journal of the Physical Society of Japan
JF - Journal of the Physical Society of Japan
IS - 12
M1 - 123706
ER -