PuCoGa5: Dazed and confused superconducting 5f electrons?

Eric D. Bauer

Los Alamos National Laboratory

 

The discovery of superconductivity in PuCoGa5 with a transition temperature of Tc = 18.5 K has generated renewed interest in Pu-based intermetallic compounds [1]. PuCoGa5, and its superconducting cousin PuRhGa5 (Tc=8.7 K), have the same crystal structure as a growing class of tetragonal CemTnIn2m+3n (T=Co, Rh, Ir) heavy fermion superconductors, suggesting that the structure plays a key role in generating superconductivity in these materials. The Pu 5f electrons in PuCoGa5 appear to be neither fully localized nor fully itinerant; elements of both kinds of behavior manifest themselves in photoemission measurements [2] and in physical properties such as an enhanced electronic specific heat coefficient  ~ 100 mJ/mol-K2 consistent with moderately heavy fermion behavior. Nuclear magnetic resonance measurements [3] provide strong evidence for unconventional d-wave superconductivity that is mediated by magnetic (spin) fluctuations rather than by phonons in the case of conventional superconductors such as Al. While similar measurements have firmly established that the CeTIn5 compounds are unconventional d-wave superconductors, most probably mediated by antiferromagnetic spin fluctuations, it is less clear what the origin of superconductivity is in PuCoGa5. In this talk, I will discuss recent measurements on PuCoGa5 that elucidate the nature of superconductivity, spin fluctuations, and its 5f electrons.

 

[1] J. L. Sarrao et al., Nature 420, 297 (2002).

[2] J. J. Joyce et al., Phys. Rev. Lett. 91, 176401 (2003).

[3] N. J. Curro et al., Nature 434, 622 (2005).