TY - JOUR
T1 - Molecular- and atomic-like photoionization of C60 in the extreme ultraviolet
AU - Kou, J.
AU - Mori, T.
AU - Ono, M.
AU - Haruyama, Y.
AU - Kubozono, Y.
AU - Mitsuke, K.
N1 - Funding Information:
We are grateful to Professors S. Kashino and Y. Yoshikawa for valuable discussions and the members of the UVSOR for their help in the course of the experiments. This work has been supported by the Joint Studies Program of the Institute for Molecular Science, by national funds appropriated for special research projects of the Institute for Molecular Science, and by a Grant-in-Aid for Scientific Research (Grant No. 14340188) from the Ministry of Education, Science, Sports, and Culture, Japan.
PY - 2003/6/4
Y1 - 2003/6/4
N2 - Photoion yield spectra of C60 in the gas phase were measured from 23 to 180 eV by synchrotron radiation. Two peaks at 26 and 34 eV and a flat area ranging 40-50 eV are newly observed in the high-energy side of the giant resonance at ∼20 eV. These features are assigned to the shape resonance on photoionization of the valence electrons of C60; the ionized electron is temporarily trapped inside a centrifugal barrier. Above ∼50 eV the yield curve shows a steady decrease with increasing photon energy like the photoabsorption cross section of atomic carbon. Thus, the spectrum is interpreted as essentially determined by photoionization of the 2s orbitals of carbon atoms.
AB - Photoion yield spectra of C60 in the gas phase were measured from 23 to 180 eV by synchrotron radiation. Two peaks at 26 and 34 eV and a flat area ranging 40-50 eV are newly observed in the high-energy side of the giant resonance at ∼20 eV. These features are assigned to the shape resonance on photoionization of the valence electrons of C60; the ionized electron is temporarily trapped inside a centrifugal barrier. Above ∼50 eV the yield curve shows a steady decrease with increasing photon energy like the photoabsorption cross section of atomic carbon. Thus, the spectrum is interpreted as essentially determined by photoionization of the 2s orbitals of carbon atoms.
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U2 - 10.1016/S0009-2614(03)00613-4
DO - 10.1016/S0009-2614(03)00613-4
M3 - Article
AN - SCOPUS:0038521549
SN - 0009-2614
VL - 374
SP - 1
EP - 6
JO - Chemical Physics Letters
JF - Chemical Physics Letters
IS - 1-2
ER -