Contrasting pressure evolution of f -electron hybridized states in CeRhIn 5 and YbNi 3 Ga 9 : An optical conductivity study
Optical conductivity [σ(ω)] of CeRhIn 5 and YbNi 3 Ga 9 have been measured at external pressures to 10 GPa and at low temperatures to 6 K. Regarding CeRhIn 5 , at ambient pressure the main feature in σ(ω) is a Drude peak due to free carriers. With increasing pressure, however, a characteristic midinfrared (mIR) peak rapidly develops in σ(ω), and its peak energy and width increase with pressure. These features are consistent with an increased conduction (c)-f electron hybridization at high pressure and show that pressure has tuned the electronic state of CeRhIn 5 from very weakly to strongly hybridized ones. As for YbNi 3 Ga 9 , in contrast, a marked mIR peak is observed already at ambient pressure, indicating a strong c-f hybridization. At high pressures, however, the mIR peak shifts to lower energy and becomes diminished and seems to merge with the Drude component at 10 GPa. Namely, CeRhIn 5 and YbNi 3 Ga 9 exhibit some opposite tendencies in the pressure evolution of σ(ω) and electronic structure. Further, these results are discussed in terms of the pressure evolution of c-f hybridized electronic states in Ce and Yb compounds, in particular in terms of the electron-hole symmetry often considered between Ce and Yb.