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Phys. Rev. B 77, 224412 (2008) [5 pages]

Magnetic structure and orbital state of Ca3Ru2O7 investigated by resonant x-ray diffraction

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B. Bohnenbuck1, I. Zegkinoglou1, J. Strempfer2, C. Schüßler-Langeheine3, C. S. Nelson4, Ph. Leininger1, H.-H. Wu3, E. Schierle5, J. C. Lang6, G. Srajer6, S. I. Ikeda7, Y. Yoshida7, K. Iwata8, S. Katano8, N. Kikugawa9, and B. Keimer1
1Max -Planck -Institut für Festkörperforschung, Heisenbergstr. 1, 70569 Stuttgart, Germany
2Hamburger Synchrotronstrahlungslabor (HASYLAB) at DESY, Notkestr. 85, 22603 Hamburg, Germany
3II. Physikalisches Institut, Universität zu Köln, Zülpicher Straße 77, 50937 Köln, Germany
4National Synchrotron Light Source, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
5Hahn-Meitner-Institut (HMI) at BESSY, Albert Einstein Straße 15, 12489 Berlin, Germany
6Advanced Photon Source, Argonne National Laboratory, Argonne, Illinois 60439, USA
7National Institute of Advanced Industrial Science and Technology, Tsukuba, Ibaraki 305-8568, Japan
8Faculty of Science, Saitama University, Saitama 338-8570, Japan
9National Institute for Material Science, Tsukuba, Ibaraki 305-0047, Japan

Received 14 March 2008; published 5 June 2008

Resonant x-ray diffraction at the L2- and L3-absorption edges of Ru has been used to investigate the magnetic structure of Ca3Ru2O7, a material with a bilayer perovskite structure that undergoes a transition from a high-temperature metallic to a low-temperature insulating phase at 48 K. In the insulating phase, magnetic Bragg reflections characteristic of A-type antiferromagnetic order (that is, ferromagnetic RuO2 bilayers coupled antiferromagnetically along the c-axis) were identified. The azimuthal-angle dependence of the diffracted intensity implies that the magnetic moments are aligned along the b-axis in the RuO2 planes. In the metallic phase, the A-type magnetic order persists up to the Néel temperature of 56 K, but the sublattice magnetization decreases by a factor of ∼1.7 and rotates by 90° within the planes. Resonant signals characteristic of uniform or staggered orbital order were not found within the experimental sensitivity, probably reflecting a weak orbital polarization in the insulating state.

© 2008 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.77.224412
DOI:
10.1103/PhysRevB.77.224412
PACS:
78.70.Ck, 75.50.Ee