Contiguous 3d and 4f Magnetism: strongly correlated 3d electrons in YbFe2Al10

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dc.contributor.author Khuntia, P.
dc.contributor.author Peratheepan, P.
dc.contributor.author Strydom, A. M.
dc.contributor.author Utsumi, Y.
dc.contributor.author Tsuei, K. D.
dc.contributor.author Tjeng, L. H.
dc.contributor.author Steglich, F.
dc.contributor.author Baenitz, M.
dc.date.accessioned 2019-08-11T04:13:55Z
dc.date.available 2019-08-11T04:13:55Z
dc.date.issued 2014
dc.identifier.uri http://www.digital.lib.esn.ac.lk/handle/123456789/3966
dc.description.abstract We present magnetization, specific heat, and 27 Al NMR investigations on YbFe 2 Al 10 over a wide range in temperature and magnetic field. The magnetic susceptibility at low temperatures is strongly enhanced at weak magnetic fields, accompanied by a ln ( T 0 / T ) divergence of the low- T specific heat coefficient in zero field, which indicates a ground state of correlated electrons. From our hard-x-ray photoemission spectroscopy study, the Yb valence at 50 K is evaluated to be 2.38. The system displays valence fluctuating behavior in the low to intermediate temperature range, whereas above 400 K, Yb 3 + carries a full and stable moment, and Fe carries a moment of about 3.1 μ B . The enhanced value of the Sommerfeld-Wilson ratio and the dynamic scaling of the spin-lattice relaxation rate divided by T [ 27 ( 1 / T 1 T ) ] with static susceptibility suggests admixed ferromagnetic correlations. 27 ( 1 / T 1 T ) simultaneously tracks the valence fluctuations from the 4 f Yb ions in the high temperature range and field dependent antiferromagnetic correlations among partially Kondo screened Fe 3 d moments at low temperature; the latter evolve out of an Yb 4 f admixed conduction band. DOI: https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.113.216403 en_US
dc.language.iso en en_US
dc.publisher Physical Review en_US
dc.title Contiguous 3d and 4f Magnetism: strongly correlated 3d electrons in YbFe2Al10 en_US
dc.type Article en_US
dc.identifier.sslno 04 en_US
dc.identifier.doi https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.113.216403 en_US


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