Exploration of the Hg-based cuprate superconductors by Raman spectroscopy under hydrostatic pressure
N. Auvray, B. Loret, S. Chibani, R. Grasset, Y. Guarnelli, P., Parisiades, A. Forget, D. Colson, M. Cazayous, Y. Gallais, Alain Sacuto

TL;DR
This study uses Raman spectroscopy under pressure to investigate Hg-based cuprate superconductors, revealing how pressure affects their superconducting properties and the relationship between pairing energy and critical temperature.
Contribution
It provides new insights into the pressure dependence of superconducting gap and charge transfer mechanisms in Hg-based cuprates, highlighting differences between Hg-1201 and Hg-1223.
Findings
$T_c$ increases slower in Hg-1223 due to charge imbalance.
The apical oxygen mode energy variation is consistent across compounds.
Binding energy of Cooper pairs decreases with pressure, not following $T_c$.
Abstract
The superconducting phase of the (Hg-1201) and (Hg-1223) cuprates has been investigated by Raman spectroscopy under hydrostatic pressure. Our analysis reveals that the increase of with pressure is slower in Hg-1223 cuprate compared to the Hg-1201 due to a charge carrier concentration imbalance (accentuated by pressure) between the layers of Hg-1223. We find that the energy variation under pressure of the apical oxygen mode from which the charge carriers are transferred to the layers, is the same for both the Hg-1223 and Hg-1223 cuprates and it is controlled by the inter-layer compressibility. At last, we show that the binding energy of the Cooper pairs related to the maximum amplitude of the wave superconducting gap at the anti-nodes,…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
