Magnetic transitions and isotropic versus anisotropic magnetic behaviour of [CH3NH3][M(HCOO)3] M = Mn2+, Co2+, Ni2+, Cu2+ metal-organic perovskites

被引:30
作者
Pato-Doldan, B. [1 ]
Gomez-Aguirre, L. C. [1 ]
Hansen, A. P. [2 ]
Mira, J. [3 ]
Castro-Garcia, S. [1 ]
Sanchez-Andujar, M. [1 ]
Senaris-Rodriguez, M. A. [1 ]
Zapf, V. S. [2 ]
Singleton, J. [2 ]
机构
[1] Univ A Coruna, Dept Fundamental Chem, Fac Sci, QuiMolMat Grp,CICA, Campus A Coruna, La Coruna 15071, Spain
[2] Los Alamos Natl Lab, Natl High Magnet Field Lab, Los Alamos, NM 87545 USA
[3] Univ Santiago de Compostela, Dept Appl Phys, Santiago 15782, Spain
基金
美国国家科学基金会;
关键词
PROMINENT DIELECTRIC ANOMALIES; NEGATIVE THERMAL-EXPANSION; WEAK FERROMAGNETISM; NEUTRON-DIFFRACTION; PHASE-TRANSITIONS; FRAMEWORKS; FERROELECTRICITY;
D O I
10.1039/c6tc03992h
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
Here we present an in-depth study of the magnetic properties of a family of metal organic perovskites ABX(3), [CH3NH3][M(HCOO)(3)] in which A = CH3NH3+ is the methylammonium cation, B = M is a divalent metal cation (Mn2+, Co2+, Ni2+ or Cu2+), and X is the formate anion (HCOO-). The magnetic properties have been measured on powdered samples and along the different orientations of mm-sized single crystals. They display spin-canted weak ferromagnetism with Neel temperatures of 8.0 K (Mn2+), 15.7 K (Co2+) and 34 K (Ni2+), which are inversely proportional to the ionic radii of the metal cations. The Cu2+ member displays low-dimensional magnetism as a result of orbital ordering of the Cu2+ d orbitals originating from a Jahn-Teller distortion. Pulsed-field magnetization experiments (fields of up to 60 T at temperatures down to 0.6 K) show that Mn2+, Co2+ and Ni2+ formates display cation-characteristic spin flop transitions. A saturation magnetization value of 5 mu(B) (at 12.5 T) was observed for Mn2+, meanwhile the Co2+ formate shows an orientation dependent quasi saturation (5.1 mu(B) at 21 T along [101] vs. 5.8 mu(B) at 26 T along [010]). The different isotropic/anisotropic behaviour can be explained by the orbital contribution to the magnetic response.
引用
收藏
页码:11164 / 11172
页数:9
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