Valence transition theory of the pressure-induced dimensionality crossover in superconducting Sr14-xCaxCu24 O41
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PhysRevB.108.134510.pdf
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Department of Physics, University of ArizonaIssue Date
2023-10-23
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American Physical SocietyCitation
Jeong-Pil Song, R. Torsten Clay, and Sumit Mazumdar Phys. Rev. B 108, 134510 – Published 23 October 2023Journal
Physical Review BRights
© 2023 American Physical Society.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
One of the strongest justifications for the continued search for superconductivity within the single-band Hubbard Hamiltonian originates from the apparent success of single-band ladder-based theories in predicting the occurrence of superconductivity in the cuprate coupled-ladder compound Sr14-xCaxCu24O41. Recent theoretical works have, however, shown the complete absence of quasi-long-range superconducting correlations within the hole-doped multiband ladder Hamiltonian including realistic Coulomb repulsion between holes on oxygen sites and oxygen-oxygen hole hopping. Experimentally, superconductivity in Sr14-xCaxCu24O41 occurs only under pressure and is preceded by dramatic transition from one to two dimensions that remains not understood. We show that understanding the dimensional crossover requires adopting a valence transition model within which there occurs transition in Cu-ion ionicity from +2 to +1, with transfer of holes from Cu to O ions [S. Mazumdar, Phys. Rev. B 98, 205153 (2018)10.1103/PhysRevB.98.205153]. The driving force behind the valence transition is the closed-shell electron configuration of Cu1+, a feature shared by cations of all oxides with a negative charge-transfer gap. We make a falsifiable experimental prediction for Sr14-xCaxCu24O41 and discuss the implications of our results for layered two-dimensional cuprates. © 2023 American Physical Society.Note
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2469-9950Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1103/PhysRevB.108.134510