Incipient Orbital Order in Half-Metallic Ba{sub 2}FeReO{sub 6}
Journal Article
·
· Physical Review Letters
- Instituto de Fisica 'Gleb Wataghin', UNICAMP, C.P. 6165, 13083-970, Campinas, Sao Paulo (Brazil)
- European Synchrotron Radiation Facility, F-38043, Grenoble (France)
- NIST Center for Neutron Research, National Institute of Standards and Technology, Gaithersburg, Maryland 20899 (United States)
- Center for Superconductivity Research, University of Maryland, College Park, Maryland 20742 (United States)
- Solid State and Structural Chemistry Unit, Indian Institute of Science, Bangalore 560012 (India)
Largely unquenched Re 5d orbital magnetic moments in half-metallic Ba{sub 2}FeReO{sub 6} drive a symmetry lowering transition from a cubic paramagnet to a compressed tetragonal (c/a<1) ferrimagnet below T{sub C}{approx}305 K, with a giant linear magnetoelastic constant and the spins lying spontaneously along the unique tetragonal axis. The large orbital magnetization and degree of structural deformation indicate proximity to a metal-insulator transition. These results point to an incipient orbitally ordered state in the metallic ferrimagnetic phase.
- OSTI ID:
- 20861587
- Journal Information:
- Physical Review Letters, Journal Name: Physical Review Letters Journal Issue: 1 Vol. 98; ISSN 0031-9007; ISSN PRLTAO
- Country of Publication:
- United States
- Language:
- English
Similar Records
Neutron scattering investigation of rhenium orbital ordering in the double perovskite
Magnetic and orbital ordering in the spinel MnV{sub 2}O{sub 4}.
Tuning magnetic coercivity with external pressure in iron-rhenium based ferrimagnetic double perovskites
Journal Article
·
Tue Dec 18 19:00:00 EST 2018
· Physical Review B
·
OSTI ID:1509565
Magnetic and orbital ordering in the spinel MnV{sub 2}O{sub 4}.
Journal Article
·
Thu Feb 14 23:00:00 EST 2008
· Phys. Rev. Lett.
·
OSTI ID:925378
Tuning magnetic coercivity with external pressure in iron-rhenium based ferrimagnetic double perovskites
Journal Article
·
Wed Aug 01 20:00:00 EDT 2018
· Physical Review B
·
OSTI ID:1465770