Abstract
We have performed transverse-field (TF) and zero-field (ZF) measurements of (Bi2201) systems with , 0.4, 0.6, and 1.0, using ceramic specimens with modest -axis alignment and single-crystal specimens. The absence of static magnetic order has been confirmed in underdoped and optimally doped systems at , while only a very weak signature towards static magnetism has been found at in the system, which is a lightly hole-doped nonsuperconducting insulator. In the superconducting (, 0.4, and 0.2) systems, the relaxation rate in TF-, proportional to (superconducting carrier density and effective mass), followed a general trend found in other cuprate systems in a plot of vs . Assuming the in-plane effective mass for Bi2201 to be comparable to three to four times the bare electron mass as found in (LSCO) and (YBCO) systems, we obtain per Cu for the Bi2201 system. This carrier density is much smaller than the Hall number per Cu obtained at in high magnetic fields along the axis applied to suppress superconductivity. The present results of the superfluid density in Bi2201 are compared with those from other cuprate systems, including YBCO systems with very much reduced studied by microwave, , and inductance methods. Additional muon-spin-relaxation measurements have been performed on a single-crystal specimen of Bi2201 in a high transverse magnetic field of parallel to the axis, in order to search for the field-induced muon spin relaxation recently found in LSCO and some other high-temperature superconducting cuprate (HTSC) systems well above . The nearly temperature-independent and very small relaxation rate observed in Bi2201 above rules out a hypothesis that the field-induced relaxation is directly proportional to the magnitude of the Nernst coefficient, which is a measure of the strength of dynamic superconductivity. We also describe a procedure for angular averaging of in measurements using ceramic specimens with modest alignment of -axis orientations, together with the neutron-scattering results obtained for determining the orientation distribution of microcrystallites in the present ceramic specimens.
6 More- Received 8 February 2006
DOI:https://doi.org/10.1103/PhysRevB.75.054511
©2007 American Physical Society