Phys. Rev. B 76, 064504 (2007) [10 pages]Muon spin rotation measurements of the superfluid density in fresh and aged superconducting PuCoGa5Received 27 March 2007; published 6 August 2007 We have measured the temperature dependence and magnitude of the superfluid density ρs(T) via the magnetic field penetration depth λ(T) in PuCoGa5 (nominal critical temperature Tc0=18.5 K) using the muon spin rotation technique in order to investigate the symmetry of the order parameter, and to study the effects of aging on the superconducting properties of a radioactive material. The same single crystals were measured after 25 days (Tc=18.25 K) and 400 days (Tc=15.0 K) of aging at room temperature. Penetration depths λ(0)=265(5) and ⩾498(10) nm are derived for the fresh and aged samples, respectively. The temperature dependence of the superfluid density ρs(T)∕ρs(0)=λ(0)2∕λ(T)2 is well described in both materials by a model using d-wave gap symmetry. Within the context of a strong-coupling dirty d-wave model a zero-temperature gap value Δ0=3.0kBTc0 is obtained in the fresh sample for a scattering rate Γ=0.005πkBTc0, which is consistent with Abrikosov-Gor’kov (AG) pair-breaking theory. This Δ0 should be compared to the weak-coupling value for a clean d-wave gap Δ0=2.14kBTc0. In the aged sample the same model yields Δ0=2.4kBTc0 for Γ=0.010πkBTc0. This value of Γ is much less than required by the AG pair-breaking formalism. Furthermore, the aged ρs(0) is reduced by at least 70% compared to the fresh sample, which is also incompatible with ΔTc∕Tc0∼20%, according to AG theory. We conclude that the data in aged PuCoGa5 support the postulate that the scattering from radiation-induced defects is not in the limit of the AG theory of an order parameter which is spatially averaged over impurity sites, but rather in the limit of short-coherence-length superconductivity. We show that a model calculation consistent with this assumption fits ρs(T) in the aged sample rather well. © 2007 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevB.76.064504
DOI:
10.1103/PhysRevB.76.064504
PACS:
71.27.+a, 74.70.Tx, 61.80.−x, 76.75.+i
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