Resonant Inelastic X-Ray Scattering Study of Electron-Exciton Coupling in High-Tc Cuprates

Explaining the mechanism of superconductivity in the high-Tccuprates requires an understanding of what causes electrons to form Cooper pairs. Pairing can be mediated by phonons, the screened Coulomb force, spin or charge fluctuations, excitons, or by a combination of these. An excitonic pairing mech...

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Bibliographic Details
Published in:Physical review. X Vol. 12; no. 2
Main Authors: Barantani, F, Tran, M K, Madan, I, Kapon, I, Bachar, N, Asmara, T C, Paris, E, Tseng, Y, Zhang, W, Y. Hu, Giannini, E, G. Gu, Devereaux, T P, Berthod, C, Carbone, F, Schmitt, T, van der Marel, D
Format: Journal Article
Language:English
Published: College Park American Physical Society 29-06-2022
American Physical Society (APS)
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Summary:Explaining the mechanism of superconductivity in the high-Tccuprates requires an understanding of what causes electrons to form Cooper pairs. Pairing can be mediated by phonons, the screened Coulomb force, spin or charge fluctuations, excitons, or by a combination of these. An excitonic pairing mechanism has been postulated, but experimental evidence for coupling between conduction electrons and excitons in the cuprates is sporadic. Here we use resonant inelastic x-ray scattering to monitor the temperature dependence of thed_dexciton spectrum ofBi2Sr2CaCu2O8−xcrystals with different charge carrier concentrations. We observe a significant change of thed_dexciton spectra when the materials pass from the normal state into the superconductor state. Our observations show that thed_dexcitons start to shift up (down) in the overdoped (underdoped) sample when the material enters the superconducting phase. We attribute the superconductivity-induced effect and its sign reversal from underdoped to overdoped to the exchange coupling of the site of thed_dexciton to the surrounding copper spins.
Bibliography:European Union (EU)
USDOE Office of Science (SC), Basic Energy Sciences (BES). Materials Sciences & Engineering Division
Swiss National Science Foundation (SNSF)
AC02-76SF00515; SC0012704; 179157; 178867; 160765; 701647
ISSN:2160-3308
2160-3308
DOI:10.1103/PhysRevX.12.021068