Double exchange magnetic interaction and giant negative magnetoresistivityin the spin glass state of the new compound CuCr1.6Sb0.4S4

Citation
J. Warczewski et al., Double exchange magnetic interaction and giant negative magnetoresistivityin the spin glass state of the new compound CuCr1.6Sb0.4S4, J ALLOY COM, 319(1-2), 2001, pp. 7-13
Citations number
16
Categorie Soggetti
Apllied Physucs/Condensed Matter/Materiales Science
Journal title
JOURNAL OF ALLOYS AND COMPOUNDS
ISSN journal
09258388 → ACNP
Volume
319
Issue
1-2
Year of publication
2001
Pages
7 - 13
Database
ISI
SICI code
0925-8388(20010426)319:1-2<7:DEMIAG>2.0.ZU;2-N
Abstract
CuCr1.6Sb0.4S4 crystallizes in the spinel structure with the lattice parame ter a=9.9680(1) Angstrom and the anion parameter u = 0.3820(1). The very ha rd magnetization of the sample, the shape of the magnetization isotherms as well as the lack of magnetic saturation even in a field of B = 14 T indica te that the antiferromagnetic superexchange interaction dominates the long- range magnetic interactions between the magnetic moments localized on the c hromium ions. A high positive value of the paramagnetic Curie-Weiss tempera ture Theta (C-W) (equal to 318 K) testifies that the short-range interactio n is ferromagnetic and strong which means that in the corresponding microre gions the double exchange interaction is present and predominates. A sugges tion is made that these microregions behave like superparamagnetic clusters . As the result of the competition of the interactions mentioned above the sample under study reveals a spin glass state at low temperatures, which is confirmed by the temperature dependence of the magnetic susceptibility cur ves. The spin-freezing temperature is lower than 50 K. CuCr1.6Sb0.4S4 is a semiconductor with a giant negative magnetoresistivity equal to 74% at 38 T and 3 K. The driving force of this effect is the double exchange magnetic interaction. Three values for the activation energy were observed: E-1 = 0. 118 eV, E-2 = 0.004 eV and E-3 = 0.033 eV. These are most probably connecte d with the energy levels generated by the crystal field. (C) 2001 Elsevier Science BN. All rights reserved.