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Phys. Rev. B 74, 224509 (2006) [9 pages]

Incident energy and polarization-dependent resonant inelastic x-ray scattering study of La2CuO4

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L. Lu1, J. N. Hancock2, G. Chabot-Couture1, K. Ishii3, O. P. Vajk4, G. Yu5, J. Mizuki3, D. Casa6, T. Gog6, and M. Greven1,2
1Department of Applied Physics, Stanford University, Stanford, California 94305, USA
2Stanford Synchrotron Radiation Laboratory, Stanford, California 94309, USA
3Synchrotron Radiation Research Unit, Japan Atomic Energy Agency, Hyogo 679-5148, Japan
4NIST Center for Neutron Research, National Institute of Standards and Technology, Gaithersburg, Maryland 20899, USA
5Department of Physics, Stanford University, Stanford, California 94305, USA
6CMC-XOR, Advanced Photon Source, Argonne National Laboratory, Argonne, Illinois 60439, USA

Received 10 July 2006; published 28 December 2006

We present a detailed Cu K-edge resonant inelastic x-ray scattering (RIXS) study of the Mott insulator La2CuO4 in the 1–7 eV energy loss range. As initially found for the high-temperature superconductor HgBa2CuO4+δ, the spectra exhibit a multiplet of weakly dispersive electron-hole excitations, which are revealed by utilizing the subtle dependence of the cross section on the incident photon energy. The close similarity between the fine structures for in-plane and out-of-plane polarizations is indicative of the central role played by the 1s core hole in inducing charge excitations within the CuO2 planes. On the other hand, we observe a polarization dependence of the spectral weight, and careful analysis reveals two separate features near 2 eV that may be related to different charge-transfer processes. The polarization dependence indicates that the 4p electrons contribute significantly to the RIXS cross section. Third-order perturbation arguments and a shake-up of valence excitations are then applied to account for the final-energy resonance in the spectra. As an alternative scenario, we discuss fluorescence-like emission processes due to 1s→4p transitions into a narrow continuum 4p band.

© 2006 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.74.224509
DOI:
10.1103/PhysRevB.74.224509
PACS:
74.25.Jb, 74.72.−h, 78.70.Ck, 71.35.−y