Temperatur Dependence of the Upper Critical Field of Superconducting Eu0.5K0.5Fe2As2


Temperatur Dependence of the Upper Critical Field of Superconducting Eu0.5K0.5Fe2As2

Weickert, F.; Hirale, J. S.; Gegenwart, P.

The discovery of superconductivity (SC) in FeAs-layered systems has triggered enormous activities on this field of solid state physics. Up to now a variety of compounds based on the two families RFeOAs (R = rare-earth element) and AFe2As2 (A = Ba, Sr, ...) were found with transition temperatures up to 57 K. A main feature of these compounds is, that SC occurs in close proximity to magnetic order, which suggests, that magnetic fluctuations play a crucial role in the formation of the superconducting ground state. In the system EuFe2As2 even two different types of magnetic order have been found. At 190 K a Fe spin density wave (SDW) forms, which is accompanied by a structural phase-transition. Below 19 K a second magnetic phase transition is observed, where Eu2+-irons order antiferromagnetically. Band structure calculation suggest, that both magnetic lattices are predominantly decoupled. A detailed study of Eu1-xKxFe2As2 indicates the complete suppression of the SDW order for x = 0.5 and the simultaneous development of SC below 32 K. In the contribution, we present magnetoresistance measurements carried out at the Hochfeldmagnetlabor Dresden on polycrystalline samples of Eu0.5K0.5Fe2As2 in pulsed magnetic fields up to 60 T. We could determine the complete temperature dependence of the upper critical field Hc2(T), at temperatures down to 1.5 K. The initial slope µ0dHc2/dT in the proximity of Tc(H = 0) varies between -1.60 T/K (0.1 Rn) and -1.75 T/K (0.9 Rn), dependent on the used criterion, and is rather small compared to other pnictides of the same family. A comparison of our results with the Werthamer-Helfand-Hohenberg (WHH) model indicates that the upper critical field in Eu0.5K0.5Fe2As2 is not Pauli limited. Moreover, the experimentally estimated critical field µ0Hc2(T → 0) of 45 T is significant higher than the value of 38 T expected for orbital limiting in the WHH model.

  • Poster
    RHMF 09 (Research in High Magnetic Fields 2009), 22.-25.07.2009, Dresden, Deutschland

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