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Chemical pressure effect on superconductivity of BiS2-based Ce1-xNdxO1-yFyBiS2 and Nd1-zSmzO1-yFyBiS2

We have systematically investigated the crystal structure and the magnetic properties of BiS2-based superconductor Ce1-xNdxO1-yFyBiS2 (x = 0 - 1.0, y = 0.3, 0.5 and 0.7) and Nd1-zSmzO1-yFyBiS2 (x = 0 - 0.8, y = 0.3, 0.5 and 0.7). In the REOBiS2 system, both crystal structure and physical properties are tunable by mixing the RE (RE = rare earth) site with Ce, Nd and Sm due to the difference of ionic radius of RE. In the Ce1-xNdxO1-yFyBiS2 system, bulk superconductivity is observed for x = 1.0 with y = 0.3 and x = 0.5 - 1.0 with y = 0.5. The transition temperature (Tc) increases with increasing Nd concentration. The highest Tc is 4.8 K for x = 1.0 with y = 0.5 in the Ce1-xNdxO1-yFyBiS2 system. By the Nd substitution for Ce, lattice contraction along the a axis is generated while the c axis does not show a remarkable dependence on Nd concentration. The lattice constant of c decreases with increasing F concentration. Furthermore, we found that the Nd site can be replaced by smaller Sm ions up to z = 0.8 in Nd1-zSmzO1-yFyBiS2. Bulk superconductivity is observed within z = 0 - 0.8 for y = 0.3 and z = 0 - 0.6 for y = 0.5. The Tc increases with increasing Sm concentration. The highest Tc is 5.6 K for z = 0.8 with y = 0.3. With increasing Sm concentration, the lattice constant of a decreases while the lattice constants of c does not show a remarkable dependence on Sm concentration. We found that the chemical pressure generated by systematic solution of the RE site in the blocking layer commonly induces lattice contraction along the a axis in Ce1-xNdxO1-yFyBiS2 and Nd1-zSmzO1-yFyBiS2. The obtained results indicate that both optimal F concentration and uniaxial lattice contraction along the a axis generated by chemical pressure are essential for the inducement of bulk superconductivity in the REO1-yFyBiS2 system.