Photoemission spectral weight distribution

K. Morikawa, T. Mizokawa, A. Fujimori, Y. Taguchi, Y. Tokura

研究成果: Article査読

72 被引用数 (Scopus)


We have studied (Formula presented)(Formula presented)(Formula presented) by photoemission and inverse-photoemission spectroscopy. Valence-band photoemission spectra show a d-band peak ∼1.4 eV below the Fermi level ((Formula presented)), which evolves into the lower Hubbard band in the x= 0 ((Formula presented)) limit. The spectra show quasiparticle emission at (Formula presented) with an extremely small spectral weight, z∼0.01, which vanishes as the system approaches either the Mott insulator limit (x=0) or the band insulator limit (x=1). Correspondingly, inverse-photoemission spectra show the upper Hubbard band and a quasiparticle feature in the unoccupied state. The fact that the observed quasiparticle spectral weight is smaller than that of (Formula presented)(Formula presented)(Formula presented) is attributed to the larger U/W, where U is the on-site d-d Coulomb energy and W is the d-band-width. The presence of the ∼1.4-eV peak for a nearly empty d band (x∼ 1) and the small spectral weight at (Formula presented) cannot be explained within the Hubbard model, indicating the importance of interactions which are not included in the model, such as the long-range Coulomb interaction and the electron-phonon interaction.

ジャーナルPhysical Review B - Condensed Matter and Materials Physics
出版ステータスPublished - 1996

ASJC Scopus subject areas

  • 電子材料、光学材料、および磁性材料
  • 凝縮系物理学


「Photoemission spectral weight distribution」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。