November 2009

Journal

Magnetic Anisotropy in the Fe(II)Fe(III) Bimetallic Oxalates

By:
Fishman, Randy S; Reboredo, Fernando A
Journal Name:
Physical Review B
Page Number:
14421-1-14421-10
Volume:
77
Issue Number:
14
Publication Date:
November 2009
View DOI Listing:
https://doi.org/10.1103/PhysRevB.77.144421

Abstract

Bimetallic oxalates are layered molecule-based magnets with transition metals M(II) and M'(III) coupled by the oxalate bridges ox=C2O4 in an open honeycomb structure. Fe(II)Fe(III) bimetallic compounds with spins S = 2 and S′ = 5/2 ferrimagnetically order below a transition temperature Tc that ranges from 30 to 48 K, depending on the cation between the layers. In small magnetic fields, several of these compounds exhibit "giant negative magnetization" below a compensation temperature of about 0.62 Tc. By studying the behavior of the orbital-doublet ground state produced by a C3-symmetric crystal field, we construct a reduced Hamiltonian that contains both exchange and spin-orbit interactions. This Hamiltonian is used to explain all of the important behavior of the Fe(II)Fe(III) bimetallic oxalates, including the stability of magnetic order in well-separated two-dimensional layers and the magnetic compensation in compounds with high transition temperatures. Fitting the parameters of this reduced Hamiltonian, we estimate that the z component of the orbital angular momentum of the ground-state doublet in compounds exhibiting magnetic compensation is about 0.27 and that the antiferromagnetic exchange coupling Jc between the Fe(II) and Fe(III) spins is about 0.45 meV. In a magnetic field perpendicular to the bimetallic layers, a spin-flop transition is predicted at a field of about 3Jc/μB ≈ 25 T. A Holstein-Primakoff 1/S and 1/S′ expansion is used to evaluate the spin-wave spectrum and to estimate the spin-wave gap sw ≈ 1.65 meV in compounds that exhibit magnetic compensation. This significant spin-wave gap explains the stability of magnetic order in well-separated bimetallic layers. We predict that the negative magnetization can be optically reversed by near-infrared light. Breaking the C3 symmetry about each of the Fe(II) ions either through a cation-induced distortion or uni-axial strain in the plane of the bimetallic layer is expected to increase the magnetic compensation temperature.


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