Superconducting energy gap and c-axis plasma frequency of (Nd,Sm)O0.82F0.18FeAs superconductors from infrared ellipsometry
A. Dubroka, K. W. Kim, M. Roessle, V.K. Malik, R. H. Liu, G. Wu, X. H., Chen, and C. Bernhard

TL;DR
This study uses infrared ellipsometry to investigate the anisotropic superconducting properties of Nd and Sm-based pnictide superconductors, revealing a large energy gap and high anisotropy similar to cuprate high-temperature superconductors.
Contribution
First infrared ellipsometry measurements of the c-axis response in (Nd,Sm)O0.82F0.18FeAs superconductors, demonstrating strong anisotropy and a large superconducting energy gap.
Findings
c-axis plasma frequency upper limit ≤ 260 cm⁻¹
c-axis magnetic penetration depth ≥ 6 μm
anisotropy ratio λ_c/λ_ab ≥ 30
Abstract
We present ellipsometric measurements of the far-infrared dielectric response of polycrystalline samples of the new pnictide superconductor RO0.82F0.18FeAs (R=Nd and Sm). We find evidence that the electronic properties are strongly anisotropic such that the optical spectra are dominated by the weakly conducting c-axis response similar as in the cuprate high-temperature superconductors (HTSC). Accordingly, we obtain an upper limit of the c-axis superconducting plasma frequency of which corresponds to a lower limit of the c-axis magnetic penetration depth of and an anisotropy of as compared to nm from muon spin rotation [A. Drew {\it et al.}, arXiv:0805.1042]. Also in analogy to the cuprate HTSC, our spectra exhibit the signatures of a gap-like suppression of the conductivity…
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