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Polarization-dependent X-ray photoemission spectroscopy for High-T^sub c^ cuprate superconductors

We have performed photon energy (hv) and linear polarization dependent X-ray photoemission for optimal doped Pb-Bi2Sr2CaCu2O8+δ (Bi2212) to investigate the ground Cu 3d orbital symmetry. We identified that the bulk Cu 3d components in valence-band spectra develop with decreasing hv from 7900 eV to 4...

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Published in:Physica. B, Condensed matter Condensed matter, 2018-05, Vol.536, p.843
Main Authors: Yamagami, Kohei, Kanai, Yuina, Naimen, Sho, Fujiwara, Hidenori, Kiss, Takayuki, Tanaka, Arata, Higashiya, Atsushi, Imada, Shin, Kadono, Toshiharu, Tamasaku, Kenji, Muro, Takayuki, Yabashi, Makina, Ishikawa, Tetsuya, Eisaki, Hiroshi, Miyasaka, Shigeki, Tajima, Setsuko, Sekiyama, Akira
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container_title Physica. B, Condensed matter
container_volume 536
creator Yamagami, Kohei
Kanai, Yuina
Naimen, Sho
Fujiwara, Hidenori
Kiss, Takayuki
Tanaka, Arata
Higashiya, Atsushi
Imada, Shin
Kadono, Toshiharu
Tamasaku, Kenji
Muro, Takayuki
Yabashi, Makina
Ishikawa, Tetsuya
Eisaki, Hiroshi
Miyasaka, Shigeki
Tajima, Setsuko
Sekiyama, Akira
description We have performed photon energy (hv) and linear polarization dependent X-ray photoemission for optimal doped Pb-Bi2Sr2CaCu2O8+δ (Bi2212) to investigate the ground Cu 3d orbital symmetry. We identified that the bulk Cu 3d components in valence-band spectra develop with decreasing hv from 7900 eV to 460 eV. Moreover, the photoelectron intensity ratio of the valence-band spectra measured at hv = 460 eV has shown that the Cu 3dx2-y2 orbital contributions are dominant near the Fermi level (EF). Meanwhile, we revealed that the bulk Cu 2p3/2 core-level spectra without the Bi 4s component is detected at hv = 1550 eV compared with hv and linear-polarization-dependent spectra.
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subjects Band spectra
Crystal structure
Linear polarization
Photoelectric emission
Spectrum analysis
Superconductivity
Superconductors
Temperature
title Polarization-dependent X-ray photoemission spectroscopy for High-T^sub c^ cuprate superconductors
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