Electronic structure of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="normal">Ca</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="italic">x</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mrow><mml:mn>60</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math>fullerides

Y. Chen(University of Minnesota), D. M. Poirier(University of Minnesota), Matej Jošt(University of Minnesota), Changbiao Gu C Gu(University of Minnesota), Toshinobu Ohno(University of Minnesota), José Luı́s Martins(University of Minnesota), J. H. Weaver(University of Minnesota), L. P. F. Chibante(University of Minnesota), R. E. Smalley(Rice University)
Physical review. B, Condensed matter
September 15, 1992
Cited by 53

Abstract

Photoemission and inverse photoemission studies of ${\mathrm{Ca}}_{\mathit{x}}$${\mathrm{C}}_{60}$ films show insulating character for x3\ifmmode\pm\else\textpm\fi{}0.3 as states derived primarily from the LUMO orbitals of ${\mathrm{C}}_{60}$ are occupied. Metallic character is observed at higher Ca content as a second band of states is partially occupied. This band has mixed character since it is derived from the LUMO+1 orbitals of ${\mathrm{C}}_{60}$ and the Ca s states. These states are responsible for superconductivity in ${\mathrm{Ca}}_{5}$${\mathrm{C}}_{60}$.


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