Raman-active phonons and mode softening in superconductingHgBa2CuO4+δ

Abstract
Polarized micro-Raman spectra of a single crystallite of HgBa2 CuO4+δ have been measured and used to assign phonon modes of A1g and Eg symmetry intrinsic to the superconducting phase. Predictions of the peak positions, linewidths, and Raman cross sections from compounds with similar bonding, i.e., HgO, Y-124, and Y-123, are closely matched and suggest assignments of the high-frequency A1g modes at 592 and 568 cm1 to apical oxygen stretch vibrations of the ideal structure and of a Cu or O defect (in the Hg plane). The low-frequency 168, 161, and 75 cm1 modes are assigned to O and Ba vibrations of Eg,A1g and Eg symmetry, respectively. An anomaly in the phonon frequency and linewidth of the 568-cm1 A1g mode is observed below Tc. If interpreted as a change in the phonon self-energy due to the onset of superconductivity, this behavior is consistent with a gap energy near 568 cm1, i.e., 8.7kTc in HgBa2 CuO4+δ and constitutes a first estimate of the superconducting gap in this material. The Raman tensor elements for the assigned A1g and Eg modes are given in absolute units.