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Detailed study of the CePd2-xNixAl3 magnetic phase diagram around its critical concentration

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ARTÍCULO CIENTÍFICO

Autores

Sereni, J.G.
Pedrazzini, P.
Bauer, E.
Galatanu, A.
Aoki, Y.
Sato, H.

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Gerencia Física. Departamento Materia Condensada. División Bajas Temperaturas

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Afiliación

Fil: Sereni, J.G. Comisión Nacional de Energía Atómica. Instituto Balseiro. Laboratorio de Bajas Temperaturas; Argentina
Fil: Bauer, E. Technische Universität Wien; Austria
Fil: Pedrazzini, P. Comisión Nacional de Energía Atómica. Instituto Balseiro. Laboratorio de Bajas Temperaturas; Argentina; University of Geneva; Suiza
Fil: Galatanu, A. National Institute for Material Physics; Rumania
Fil: Aoki, Y. Tokyo Metropolitan University; Japón
Fil: Sato, H. Tokyo Metropolitan University; Japón

Sede CNEA

Centro Atómico Bariloche

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Idioma

eng

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Resumen

Thermal, magnetic and transport measurements on CePd2−xNixAl3 alloys within the 0≤x≤1 range are reported, including applied pressure (p) and magnetic field on some selected samples. The low temperature results indicate that long range antiferromagnetic order is robust up to x = 0.2, whereas between 0.25 and 0.5 magnetic fluctuations give rise to non-Fermi-liquid (NFL) behaviour. In this critical region, the low temperature specific heat can be described as due to two components, the major showing a NFL Cp /T = γ0 − γ1 √T dependence, while the minor one includes a decreasing fraction of short range order degrees of freedom. The latter is only observed close to the critical point, xcr≈0.35. Electrical resistivity (ρ) studies performed under pressure for x = 0.5 allow us to investigate the evolution of the NFL state around and beyond xcr, where the exponent of ρ ∝ T n increases from n = 1 (for p = 0) up to n = 2 (for p = 12 kbar). This exponent is also observed at normal pressure on the x = 1.0 sample, indicating the onset of the Fermi liquid behaviour. Doping and pressure effects are compared by fitting high temperature resistivity data employing a unique function which allows us to describe the evolution of the characteristic energy of this series along a large range of concentration and pressure.

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J G Sereni et al 2006 J. Phys.: Condens. Matter 18 3789

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