Electronic phase separation due to magnetic polaron formation in the semimetallic ferromagnet EuB6 - A weakly-nonlinear-transport study
- Author(s): Amyan, A
- Das, P
- Müller, J
- Fisk, Z
- et al.
Published Web Locationhttps://doi.org/10.3938/jkps.62.1489
We report measurements of weakly nonlinear electronic transport, as measured by third-harmonic voltage generation V , in the low-carrier density semimetallic ferromagnet EuB , which exhibits an unusual magnetic ordering with two consecutive transitions at T = 15.6K and T = 12.5K. In contrast to the linear resistivity, the third-harmonic voltage is sensitive to the microgeometry of the electronic system. Our measurements provide evidence for magnetically-driven electronic phase separation consistent with the picture of percolation of magnetic polarons (MP), which form highly conducting magnetically ordered clusters in a paramagnetic and less conducting background. Upon cooling in zero magnetic field through the ferromagnetic transition, the dramatic drop in the linear resistivity at the upper transition T coincides with the onset of nonlinearity, and upon further cooling is followed by a pronounced peak in V at the lower transition T . Likewise, in the paramagnetic regime, a drop of the material's magnetoresistance R(H) precedes a magnetic-fieldinduced peak in nonlinear transport. A striking observation is a linear temperature dependence of V . We suggest a picture where at the upper transition T the coalescing MP form a conducting path giving rise to a strong decrease in the resistance. The MP formation sets in at around T* ∼ 35K below which these entities are isolated and strongly fluctuating, while growing in number. The MP then start to form links at T , where percolative electronic transport is observed. The MP merge and start forming a continuum at the threshold T . In the paramagnetic temperature regime T < T < T*, MP percolation is induced by a magnetic field, and the threshold accompanied by charge carrier delocalization occurs at a single critical magnetization. © 2013 The Korean Physical Society. 3ω 6 c1 c2 c1 3ω c2 3ω c1 c1 c2 c1 peak