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Possible weakly first-order superconducting transition induced by magnetic excitations in the YBCO system: A fluctuation conductivity study
Fluctuation conductivity is experimentally studied in the genuine critical region near the superconducting transition of YBa2Cu3O7−δ, YBa2Cu2.985Fe0.015O7−δ and Y0.95Ca0.05Ba2Cu3O7−δ single crystal samples. Two fluctuation regimes where the electrical conductivity diverges as a power-law of the redu...
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Published in: | Physics letters. A 2017-04, Vol.381 (14), p.1255-1260 |
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Main Authors: | , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Fluctuation conductivity is experimentally studied in the genuine critical region near the superconducting transition of YBa2Cu3O7−δ, YBa2Cu2.985Fe0.015O7−δ and Y0.95Ca0.05Ba2Cu3O7−δ single crystal samples. Two fluctuation regimes where the electrical conductivity diverges as a power-law of the reduced temperature were systematically observed. In the first regime, farther from the critical temperature Tc, the transition behaves as predicted by the thermodynamics of the three dimensional-XY (3D-XY) universality class characteristic of a second-order phase transition. In the asymptotic regime closer to Tc a power-law regime characterized by a much smaller exponent is observed. The smallest value ever reported for the fluctuation conductivity exponent in the high-Tc superconductors is obtained for the Fe- and Ca-doped systems. We suggest that the regime beyond 3D-XY is a crossover towards a weakly first-order transition induced by internal magnetic excitations.
•It is obtained the smallest value reported for fluctuation conductivity exponent in HSTC.•The supercritical regime is interpreted as a precursor to a weak first order SC transition.•Slightly doping YBCO with Fe or Ca improves the stability of supercritical fluctuations.•The weak first order in YBCO is related to internal magnetic excitations. |
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ISSN: | 0375-9601 1873-2429 |
DOI: | 10.1016/j.physleta.2017.02.001 |