RUS  ENG
Full version
JOURNALS // Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki // Archive

Pis'ma v Zh. Èksper. Teoret. Fiz., 2014 Volume 100, Issue 6, Pages 423–428 (Mi jetpl4125)

This article is cited in 6 papers

CONDENSED MATTER

Pressure-induced antiferromagnet-ferromagnet transition and a change in the spin state of Co in La$_{0.5}$Ba$_{0.5}$CoO$_{2.8}$

D. P. Kozlenkoa, A. V. Rutkauskasa, N. T. Dangb, N. O. Golosovaa, S. E. Kichanova, L. S. Dubrovinskyc, H. P. Liermannd, W. Morgenrothd, B. N. Savenkoa

a Joint Institute for Nuclear Research, Dubna, Moskovskaya obl.
b Institute of Research and Developmen, Duy Tan University
c Bayerisches Geoinstitut, Universität Bayreuth
d Institute of Geosciences, University of Frankfurt

Abstract: The crystal and magnetic structures of anion-deficit cobaltite La$_{0.5}$Ba$_{0.5}$CoO$_{2.8}$ have been studied by the X-ray and neutron diffraction methods at high pressures up to 30 and 6 GPa, respectively. A structure transition from the cubic phase with symmetry Pm$\bar{3}$m to the tetragonal phase with symmetry P4/mmm has been observed in this compound at $P\approx3\,$. It is accompanied by the change of the ground antiferromagnetic state of the G type to the ferromagnetic state because of a change in the electronic configuration of Co$^{3+}$ ions. Possible mechanisms of the observed magnetic phase transition, as well as the role of the superexchange interactions between Co$^{3+}$ ions in various spin states in the formation of magnetic properties, have been discussed. Pressure-induced change in the magnetic state of La$_{0.5}$Ba$_{0.5}$CoO$_{2.8}$ significantly differs from related stoichiometric compounds La$_{0.5}$A$_{0.5}$CoO$_{3.0}$ (A = Sr, Ca), where the ground ferromagnetic state is formed and the sign of the pressure dependence of the Curie temperature depends on the element A.

Received: 11.07.2014

DOI: 10.7868/S0370274X14180064


 English version:
Journal of Experimental and Theoretical Physics Letters, 2014, 100:6, 380–384

Bibliographic databases:


© Steklov Math. Inst. of RAS, 2024