The Effect of Thermal Reduction on the Photoluminescence and Electronic Structures of Graphene Oxides

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作者
C.-H. Chuang
Y.-F. Wang
Y.-C. Shao
Y.-C. Yeh
D.-Y. Wang
C.-W. Chen
J. W. Chiou
Sekhar C. Ray
W. F. Pong
L. Zhang
J. F. Zhu
J. H. Guo
机构
[1] Tamkang University,Department of Physics
[2] National Taiwan University,Department of Material Science and Engineering
[3] National University of Kaohsiung,Department of Applied Physics
[4] College of Science,Department of Physics
[5] Engineering and Technology,undefined
[6] University of South Africa,undefined
[7] Private Bag X6,undefined
[8] Florida,undefined
[9] 1710,undefined
[10] Science Campus,undefined
[11] National Synchrotron Radiation Laboratory,undefined
[12] University of Science and Technology of China,undefined
[13] Advanced Light Source,undefined
[14] Lawrence Berkeley National Laboratory,undefined
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摘要
Electronic structures of graphene oxide (GO) and hydro-thermally reduced graphene oxides (rGOs) processed at low temperatures (120–180°C) were studied using X-ray absorption near-edge structure (XANES), X-ray emission spectroscopy (XES) and resonant inelastic X-ray scattering (RIXS). C K-edge XANES spectra of rGOs reveal that thermal reduction restores C = C sp2 bonds and removes some of the oxygen and hydroxyl groups of GO, which initiates the evolution of carbonaceous species. The combination of C K-edge XANES and Kα XES spectra shows that the overlapping π and π* orbitals in rGOs and GO are similar to that of highly ordered pyrolytic graphite (HOPG), which has no band-gap. C Kα RIXS spectra provide evidence that thermal reduction changes the density of states (DOSs) that is generated in the π-region and/or in the gap between the π and π* levels of the GO and rGOs. Two-dimensional C Kα RIXS mapping of the heavy reduction of rGOs further confirms that the residual oxygen and/or oxygen-containing functional groups modify the π and σ features, which are dispersed by the photon excitation energy. The dispersion behavior near the K point is approximately linear and differs from the parabolic-like dispersion observed in HOPG.
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