Paramagnons and high-temperature superconductivity in a model family of cuprates

Cuprate superconductors have the highest critical temperatures (T-c) at ambient pressure, yet a consensus on the superconducting mechanism remains to be established. Finding an empirical parameter that limits the highest reachable T-c can provide crucial insight into this outstanding problem. Here, in the first two Ruddlesden-Popper members of the model Hg-family of cuprates, which are chemically nearly identical and have the highest T-c among all cuprate families, we use inelastic photon scattering to reveal that the energy of magnetic fluctuations may play such a role. In particular, we observe the single-paramagnon spectra to be nearly identical between the two compounds, apart from an energy scale difference of similar to 30% which matches their difference in T-c. The empirical correlation between paramagnon energy and maximal T-c is further found to extend to other cuprate families with relatively high T-c's, hinting at a fundamental connection between them.

Automated summary

By studying two members of the model Hg family, it is found that the energy of magnetic fluctuations may limit the highest critical temperature of cuprate superconductors, providing important clues for understanding the superconducting mechanism. Furthermore, the correlation between paramagnon energy and maximal critical temperature is also confirmed in other cuprate families.