Non-centrosymmetric superconductors have received considerable attention because of their possible possession of unconventional spin-triplet pairing.For this reason,the non-centrosymmetric Re<sub>3</sub>W with <i>α</i> -Mn structure has been widely concerned.However,almost all the previous studies support that the non-centrosymmetric phase of Re<sub>3</sub>W is a conventional weak-coupling s-wave superconductor.Later on,it is proved that Re<sub>3</sub>W has two different superconducting phases,one is the non-centrosymmetric phase and the other has a centrosymmetric hexagonal structure.Thus,a comparative study of these two superconducting phases could provide more information about the effect of non-centrosymmetric structure on the pairing symmetry of Re<sub>3</sub>W.</br>In this paper,point-contact Andreev reflection experiments are carried out on Re<sub>3</sub>W/Au and the data can be well fitted by isotropic s-wave Blonder-Tinkham-Klapwijk (BTK) theory.In combination with our previous researches,we find that both centrosymmetric and non-centrosymmetric phases have similar temperature dependence of superconducting gap (<i>△</i>) with almost the same gap ratio of <i>△</i>/<i>T</i><sub>c</sub>.These results present strong evidence that both phases of Re<sub>3</sub>W are weak coupling Bardeen-Cooper-Schrieffer superconductors.</br>Another interesting finding is that both phases of Re<sub>3</sub>W could easily form an ideal point-contact junction (i.e.,inelastic scatterings at the interface can be ignored) with a normal metal tip.This is manifested as an extremely small broadening factor (<i>Γ</i>) used in the fitting process,and indicates a clean (and possibly transparent) interface.Keeping this in mind,we can assume that the effective barrier (<i>Z</i>) at the interface mainly comes from the mismatch between the Fermi velocity of the superconductor and that of the normal metal,which can be estimated from the formula <i>Z</i><sup>2</sup>=(1-<i>r</i>)<sup>2</sup>/4<i>r</i>,where <i>r</i> is the ratio between those two Fermi velocities.From this formula,we can obtain the Fermi velocity of Re<sub>3</sub>W by using the known value of Au's Fermi velocity and the fitting parameter <i>Z</i> for the Re<sub>3</sub>W/Au point contacts.It is interesting to find that the chemical property of Re<sub>3</sub>W is stable in the atmospheric environment.Even if the samples are exposed to the atmospheric environment for nearly six months,the inelastic scatterings are still very weak,and the superconducting properties are unchanged.</br>Such an exceptional performance of Re<sub>3</sub>W can be utilized to study the physical properties of its counter electrode in a point contact.As an attempt,we build a point contact between Re<sub>3</sub>W and a ferromagnetic Ni tip,and measure its Andreev reflection spectra which are then fitted with a modified BTK model by considering spin polarization.The determined spin polarization of Ni is in good agreement with previously reported result. Moreover,using the Fermi velocities of Re<sub>3</sub>W and Ni,we can calculate the effective barrier to be around 0.3 in the Re<sub>3</sub>W/Ni interface,which coincides with the fitting parameter <i>Z</i>.These results self-consistently demonstrate the validity of the determination of Re<sub>3</sub>W's Fermi velocity and the cleanness/transparency of the studied point-contact interface.
The 112-type (Ca, RE)FeAs2 (RE=rare earth) superconductors are very special among the iron-based superconductors for their particular crystal structures with arsenic chain configuration and attractive electronic phase diagram with the coexistence of superconductivity and antiferromagnetism upon carrier doping, while the chemical phases are absent for the low doping level or undoped parent compound. Here we report the single crystal growth method and physical characterizations for the newly discovered Eu 112 type parent compound EuFeAs2. The single crystal of EuFeAs2 is grown by high temperature solution method through using CsCl as the flux under the constant temperature of 800℃ with the molar ratio of the starting materials Eu:Fe:As:CsCl=1:1:4:18. The as-grown crystal is shinyplatelike piece with a typical size of 1 mm1 mm0.2 mm, and quite stable in air. The chemical composition of EuFeAs2 crystal is confirmed by energy-dispersive X-ray spectroscopy. The single crystal X-ray diffraction analysis at room temperature indicates that EuFeAs2 crystallizes into an orthorhombic crystal structure with the space group Imm2 (No. 44), and the refined lattice parameters are a=21.285(9) , b=3.9082(10) , c=3.9752(9) , which are different from those of the Ca 112 compound, but similar to those of unique zigzag As-As chain configuration presented in the layered crystal structure. Electrical resistivity measurements show three anomalies near 110 K, 98 K, and 46 K. The former two anomalies with relatively high temperature imply that the structural and antiferromagnetic transitions are related to Fe2+ sublattice, which is similar to other iron-based parent compounds. The low temperature anomaly at 46 K is attributed to the antiferromagnetic transition of Eu2+ sublattice, which is also confirmed by the corresponding transition observed in the direct current magnetic susceptibility measurement. The magnetic susceptibility of EuFeAs2 exhibits obvious anisotropy blow 46 K when the magnetic field is parallel or perpendicular to the bc plane, while the exact orientation of the Eu2+ moment needs further studying. The discovery of EuFeAs2 provides a new platform for further studying the unique crystal structure and electronic state phase diagrams in the 112-type iron-based superconducting family, and may shed new light on the correlations between superconductivity and magnetism.
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