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Evolution of Fermi Liquid Interactions in Sr\(_2\)RuO\(_4\) under Pressure

Forsythe, D., Julian, S.R., Bergemann, C, Pugh, E., Steiner, M.J., Alireza, P.L., McMullan, G.J., Nakamura, F., Haselwimmer, R.K.W., Walker, I.R., and others. (2002) Evolution of Fermi Liquid Interactions in Sr\(_2\)RuO\(_4\) under Pressure. Physical Review Letters, 89 . Article Number 166402. ISSN 0031-9007. (doi:10.1103/PhysRevLett.89.166402) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:84508)

The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided.
Official URL:
http://dx.doi.org/10.1103/PhysRevLett.89.166402

Abstract

We have measured the temperature and field dependence of the resistivity of the unconventional superconductor Sr\(_2\)RuO\(_4\) at pressures up to 3.3 GPa. Using the Shubnikov–de Haas effect, we find that the Fermi surface sheet believed to be primarily responsible for superconductivity becomes more two-dimensional with increasing pressure, a surprising result that is, however, consistent with a recent model of orbital-dependent superconductivity in this system. Many-body enhancements and the superconducting transition temperature all fall gradually with increasing pressure, contrary to previous suggestions of a ferromagnetic quantum critical point at ∼ 3 GPa.

Item Type: Article
DOI/Identification number: 10.1103/PhysRevLett.89.166402
Subjects: Q Science > QC Physics
Divisions: Divisions > Division of Natural Sciences > Physics and Astronomy
Depositing User: Emma Pugh
Date Deposited: 27 Nov 2020 18:33 UTC
Last Modified: 05 Nov 2024 12:50 UTC
Resource URI: https://kar.kent.ac.uk/id/eprint/84508 (The current URI for this page, for reference purposes)

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