First-principles band structure and FLEX approach to the pressure effect on $T_c$ of the cuprate superconductors
Hirofumi Sakakibara, Katsuhiro Suzuki, Hidetomo Usui, Kazuhiko Kuroki,, Ryotaro Arita, Douglas J. Scalapino, Hideo Aoki

TL;DR
This paper investigates how pressure influences the superconducting transition temperature (Tc) in cuprates, highlighting the roles of orbital hybridization and band width, with detailed analysis of multilayer structures and many-body effects.
Contribution
It extends previous models by analyzing the pressure effects on Tc with a focus on multilayer structures and many-body renormalization, providing deeper insight into orbital distillation and band width effects.
Findings
Pressure reduces orbital hybridization, enhancing Tc in multilayer cuprates.
Increase in band width under pressure decreases many-body renormalization, raising Tc.
Bi-layer materials show reduced orbital mixing effects due to pyramidal oxygen coordination.
Abstract
High-temperature cuprate superconductors have been known to exhibit significant pressure effects. In order to fathom the origin of why and how Tc is affected by pressure, we have recently studied the pressure effects on Tc adoptig a model that contains two cupper d-orbitals derived from first-principles band calculations, where the dz2 orbital is considere on top of the usually considered dx2-y2 orbital. In that paper, we have identified two origins for the Tc enhancement under hydrostatic pressure: (i) while at ambient pressure the smaller the hybridization of other orbital components the higher the Tc, an application of pressure acts to reduce the multiorbital mxing on the Fermi surface, which we call the orbital distillation effects, and (ii) the increase of the band width with pressure also contributes to the enhancement. In the present paper, we further elabolrate the two points.…
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