Infrared-absorption and photoinduced-absorption spectroscopy of semiconductingYBa2Cu3O6+xA(A=16 and 18; 0≤x≤0.3)

Abstract
We report the infrared (ir) absorption and photoinduced absorption (PA) spectra of semiconducting YBa2 Cu3 O6+xA for A=16 and 18 and for 0≤x≤0.3. We observe ten ir absorption modes for x=0.3 and report the first observation for all 11 allowed ir modes for x=0.0. The ir modes for x=0.0 and x=0.3 are nearly the same. Shifts of the ir modes with substitution of O16 with O18 are in accord with the expected role of oxygen in the various vibrational modes. The PA spectra of YBa2 Cu3 O6+x for pumping with 2.71-eV light across the band gap reveals the presence of a photoinduced electronic absorption band that varies with increasing oxygen content from a broad and nearly featureless peak at 1300 cm1 for x=0.0, to photoinduced transitions at 750, 950, 1100, and 1300 cm1 for x=0.13 and 0.20, and to a stronger PA peak centered at 950 cm1 with a shoulder at 750 cm1 for x=0.3. There are corresponding changes in the PA ir spectra with increasing x, with, in particular, bleaching of ir modes associated with the tetragonal x=0 lattice and enhancement of ir modes associated with the orthorhombic x=1.0 lattice. Based on our results and those from the following paper (Leng et al.), we propose a model for the formation of positively and negatively charged defects, D+ and D. We suggest that while the D+ defects reside on the CuO2 planes, the D defects consist of electrons initially in the conduction band for x=0.0. With increasing oxygen content, the electrons are trapped in CuO chains of increasing length and form localized D defects.