T. Kadono
University of Tokyo
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Publication
Featured researches published by T. Kadono.
Journal of the Physical Society of Japan | 2015
Yuina Kanai; Takeo Mori; Sho Naimen; Kohei Yamagami; H. Fujiwara; Atsushi Higashiya; T. Kadono; S. Imada; T. Kiss; A. Tanaka; Kenji Tamasaku; Makina Yabashi; Tetsuya Ishikawa; Fumitoshi Iga; Akira Sekiyama
We have successfully observed linear dichroism in angle-resolved Yb3+ 3d5/2 core-level photoemission spectra for YbB12 in cubic symmetry. Its anisotropic 4f charge distribution due to the crystal-field splitting is responsible for the linear dichroism, which has been verified by spectral simulations using ionic calculations with the full multiplet theory for a single-site Yb3+ ion in cubic symmetry. The observed linear dichroism as well as the polarization-dependent spectra in two different photoelectron directions for YbB12 are quantitatively reproduced by theoretical analysis for the Γ8 ground state, indicating the Γ8 ground-state symmetry for the Yb3+ ions mixed with the Yb2+ state.
Physical Review B | 2015
K. Ishigami; Kohei Yoshimatsu; D. Toyota; M. Takizawa; T. Yoshida; Goro Shibata; T. Harano; Yu Takahashi; T. Kadono; V. K. Verma; Vijay Singh; Yukiharu Takeda; Tetsuo Okane; Y. Saitoh; Hiroshi Yamagami; Tsuneharu Koide; M. Oshima; Hiroshi Kumigashira; A. Fujimori
Thin films of the ferromagnetic metal
Physical Review B | 2014
Goro Shibata; Kohei Yoshimatsu; Enju Sakai; Vijay Singh; V. K. Verma; K. Ishigami; T. Harano; T. Kadono; Yukiharu Takeda; Tetsuo Okane; Y. Saitoh; Hiroshi Yamagami; Akihito Sawa; Hiroshi Kumigashira; Masaharu Oshima; Tsuneharu Koide; Atsushi Fujimori
{\mathrm{SrRuO}}_{3}
IEEE Transactions on Applied Superconductivity | 2012
Mitsuho Furuse; Makoto Okano; Shuichiro Fuchino; Akira Uchida; Jun-ichi Fujihira; Seiichi Fujihira; T. Kadono; Atsushi Fujimori; Tsuneharu Koide
(SRO) show a varying easy magnetization axis depending on the epitaxial strain, and undergo a metal-to-insulator transition with decreasing film thickness. We have investigated the magnetic properties of SRO thin films with varying thicknesses fabricated on
EPL | 2014
Yoshinori Takahashi; Vk K. Verma; Goro Shibata; T. Harano; K. Ishigami; Kohei Yoshimatsu; T. Kadono; Atsushi Fujimori; A. Tanaka; Fh-H. Chang; Hj-J. Lin; Dj J. Huang; Ct T. Chen; Banabir Pal; D. D. Sarma
{\mathrm{SrTiO}}_{3}
Journal of Synchrotron Radiation | 2016
H. Fujiwara; Sho Naimen; Atsushi Higashiya; Yuina Kanai; Hiroshi Yomosa; Kohei Yamagami; T. Kiss; T. Kadono; S. Imada; A. Yamasaki; Kouichi Takase; Shintaro Otsuka; Tomohiro Shimizu; Shoso Shingubara; Shigemasa Suga; Makina Yabashi; Kenji Tamasaku; Tetsuya Ishikawa; Akira Sekiyama
(001) substrates by soft x-ray magnetic circular dichroism at the Ru
Applied Physics Letters | 2013
T. Harano; Goro Shibata; K. Ishigami; Y. Takashashi; V. K. Verma; Vijay Singh; T. Kadono; Atsushi Fujimori; Yukiharu Takeda; Tetsuo Okane; Y. Saitoh; Hiroshi Yamagami; Tsuneharu Koide; Hiroshi Yamada; Akihito Sawa; Masashi Kawasaki; Y. Tokura; A. Tanaka
{M}_{2,3}
Physical Review B | 2014
Yukio Takahashi; T. Kadono; S. Yamamoto; Vijay Singh; V. K. Verma; K. Ishigami; Goro Shibata; T. Harano; Yukiharu Takeda; Tetsuo Okane; Y. Saitoh; Hiroshi Yamagami; M. Takano; A. Fujimori
edge. Results have shown that, with decreasing film thickness, the film changes from ferromagnetic to nonmagnetic at around 3 monolayer thickness, consistent with previous magnetization and magneto-optical Kerr effect measurements. The orbital magnetic moment perpendicular to the film was found to be
IEEE Transactions on Applied Superconductivity | 2013
Mitsuho Furuse; Makoto Okano; Shuichiro Fuchino; Akira Uchida; Jun-ichi Fujihira; Seiichi Fujihira; T. Kadono; Atsushi Fujimori; Tsuneharu Koide
\ensuremath{\sim}0.1{\ensuremath{\mu}}_{\text{B}}/\mathrm{Ru}
Physical Review B | 2013
Kohei Yoshimatsu; H. Wadati; Enju Sakai; Takayuki Harada; Yu Takahashi; T. Harano; Goro Shibata; K. Ishigami; T. Kadono; Tsuneharu Koide; T. Sugiyama; Eiji Ikenaga; Hiroshi Kumigashira; Mikk Lippmaa; M. Oshima; A. Fujimori
, and remained nearly unchanged with decreasing film thickness while the spin magnetic moment decreases. A mechanism for the formation of the orbital magnetic moment is discussed based on the electronic structure of the compressively strained SRO film.