(Translated by https://www.hiragana.jp/)
Phys. Rev. B 105, 205106 (2022) - Observation of bands with ${d}_{xy}$ orbital character near the Fermi level in ${\mathrm{NdFeAs}}_{1\ensuremath{-}x}{\mathrm{P}}_{x}{\mathrm{O}}_{0.9}{\mathrm{F}}_{0.1}$ using angle-resolved photoemission spectroscopy

Observation of bands with dxy orbital character near the Fermi level in NdFeAs1xPxO0.9F0.1 using angle-resolved photoemission spectroscopy

Z. H. Tin, T. Adachi, A. Takemori, K. Yoshino, N. Katayama, S. Miyasaka, S. Ideta, K. Tanaka, and S. Tajima
Phys. Rev. B 105, 205106 – Published 6 May 2022

Abstract

We studied the band structure of NdFeAs1xPxO0.9F0.1 (x=0, 0.2, 0.4, and 0.6) using angle-resolved photoemission spectroscopy (ARPES) measurements. Two of the hole bands, αあるふぁ1 (dxz) and αあるふぁ3 (dz2), were observed at the Brillouin zone center in the P-polarized light configuration, while the other two hole bands, αあるふぁ2 (dyz) and γがんま (dxy), were observed in the S-polarized alternative. The observed γがんま band shifts downward as x increases, which is consistent with the theoretical prediction for the change in bond angle of As/P-Fe-As/P. Furthermore, a small amount of the dxy orbital component was observed at the same binding energy as that of the top of the αあるふぁ1 band, thus indicating the band reconstruction of the originally degenerate αあるふぁ1 and αあるふぁ2 (dxz/dyz) bands by the unoccupied dxy band. The change in the energy level of the αあるふぁ1 band top with dxy orbital character is accompanied by a Tc upturn at 0.2<x<0.4. The Tc continues to increase as the αあるふぁ1 band shifts downward, crossing the Fermi level. The incipient band with the dxy orbital character on its top could be an important ingredient for high Tc 1111-type iron-based superconductors.

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  • Received 7 May 2020
  • Revised 10 April 2022
  • Accepted 14 April 2022

DOI:https://doi.org/10.1103/PhysRevB.105.205106

©2022 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Z. H. Tin1,*, T. Adachi1, A. Takemori1, K. Yoshino1, N. Katayama1, S. Miyasaka1, S. Ideta2,3, K. Tanaka3,4, and S. Tajima1

  • 1Department of Physics, Osaka University, Osaka 560-0043, Japan
  • 2Hiroshima Synchrotron Radiation Center, Hiroshima University, Higashi-Hiroshima 739-0046, Japan
  • 3UVSOR Synchrotron Facility, Institute for Molecular Science, Okazaki 444-8585, Japan
  • 4School of Physical Sciences, The Graduate University for Advanced Studies (SOKENDAI), Okazaki 444-8585, Japan

  • *zihow92@hotmail.com

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Vol. 105, Iss. 20 — 15 May 2022

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