Abstract:
Based on Cu 2p core-level spectroscopy and theoretical calculations, it has been demonstrated that the Cu-O charge-transfer excitation energy which determines the Cu 2p satellite intensity also plays a crucial role in the superconductivity of cuprates. The relative intensity of the satellite generally decreases with an increase in the Tc or in the hole concentration in a given series of cuprate superconductors. In the case of Bi2Ca1-xRxSr2Cu2O8+δ (R=rare earth), the satellite intensity goes through a minimum around the same composition where the hole concentration as well as the Tc show maxima.
