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Enhanced superconducting pairing strength near a nonmagnetic nematic quantum critical point

Authors :
Mukasa, K.
Ishida, K.
Imajo, S.
Qiu, M. W.
Saito, M.
Matsuura, K.
Sugimura, Y.
Liu, S.
Uezono, Y.
Otsuka, T.
Čulo, M.
Kasahara, S.
Matsuda, Y.
Hussey, N. E.
Watanabe, T.
Kindo, K.
Shibauchi, T.
Source :
Phys. Rev. X 13, 011032 (2023)
Publication Year :
2022

Abstract

The quest for high-temperature superconductivity at ambient pressure is a central issue in physics. In this regard, the relationship between unconventional superconductivity and the quantum critical point (QCP) associated with the suppression of some form of symmetry-breaking order to zero temperature has received particular attention. The key question is how the strength of the electron pairs changes near the QCP, and this can be verified by high-field experiments. However, such studies are limited mainly to superconductors with magnetic QCPs, and the possibility of unconventional mechanisms by which nonmagnetic QCP promotes strong pairing remains a nontrivial issue. Here, we report systematic measurements of the upper critical field $H_{{\rm c2}}$ in nonmagnetic FeSe$_{1-x}$Te$_{x}$ superconductors, which exhibit a QCP of electronic nematicity characterized by spontaneous rotational-symmetry breaking. As the magnetic field increases, the superconducting phase of FeSe$_{1-x}$Te$_{x}$ shrinks to a narrower dome surrounding the nematic QCP. The analysis of $H_{{\rm c2}}$ reveals that the Pauli-limiting field is enhanced toward the QCP, implying that the pairing interaction is significantly strengthened via nematic fluctuations emanated from the QCP. Remarkably, this nonmagnetic nematic QCP is not accompanied by a divergent effective mass, distinct from the magnetically mediated pairing. Our observation opens up a nonmagnetic route to high-temperature superconductivity.<br />Comment: 6 pages, 4 figures

Details

Database :
arXiv
Journal :
Phys. Rev. X 13, 011032 (2023)
Publication Type :
Report
Accession number :
edsarx.2202.11657
Document Type :
Working Paper
Full Text :
https://doi.org/10.1103/PhysRevX.13.011032