Complex magnetic order in the decorated spin-chain system Rb2Mn3(MoO4)3(OH)2

Yaohua Liu, Liurukara D. Sanjeewa, V. Ovidiu Garlea, Tiffany M. Smith Pellizzeri, Joseph W. Kolis, Athena S. Sefat

Research output: Contribution to journalArticlepeer-review

7 Scopus citations

Abstract

The macroscopic magnetic properties and microscopic magnetic structure of Rb2Mn3(MoO4)3(OH)2 (space group Pnma) are investigated by magnetization, heat capacity, and single-crystal neutron diffraction measurements. The compound's crystal structure contains bond-alternating [Mn3O11]∞ chains along the b axis, formed by isosceles triangles of Mn ions occupying two crystallographically nonequivalent sites (the Mn1 site on the base and Mn2 site on the vertex). These chains are only weakly linked to each other by nonmagnetic oxyanions. Both superconducting quantum interference device magnetometry and neutron diffraction experiments show two successive magnetic transitions as a function of temperature. On cooling, it transitions from a paramagnetic phase into an incommensurate phase below 4.5 K with a magnetic wave vector near k1=(0,0.46,0). An additional commensurate antiferromagnetically ordered component arises with k2=(0,0,0), forming a complex magnetic structure below 3.5 K with two different propagation vectors of different stars. On further cooling, the incommensurate wave vector undergoes a lock-in transition below 2.3 K. The experimental results suggest that the magnetic superspace group is Pnma.1′(0b0)s0ss for the single-k incommensurate phase and is Pn′ma(0b0)00s for the two-k magnetic phase. We propose a simplified magnetic structure model taking into account the major ordered contributions, where the commensurate k2 defines the ordering of the c-axis component of the Mn1 magnetic moment, while the incommensurate k1 describes the ordering of the ab-plane components of both Mn1 and Mn2 moments into elliptical cycloids.

Original languageEnglish
Article number064423
JournalPhysical Review B
Volume101
Issue number6
DOIs
StatePublished - Feb 1 2020

Funding

Y.L. sincerely acknowledges Dr. Chakoumakos (ORNL) for providing suggestions to improve the manuscript, and he is also indebted to lecturers at the 5th School on Representational Analysis and Magnetic Structures (University of Maryland, College Park, 2015) and the Workshop on Symmetry and Superspace Approach to Modulated Crystal Structures (Oak Ridge, 2019). A portion of this research used resources at the Spallation Neutron Source, a DOE Office of Science User Facility operated by the Oak Ridge National Laboratory. Work at ORNL was partially supported by the US Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division. We are indebted to the NSF for Grant No. DMR-1808371 for support of the synthesis work. This work has been partially supported by US DOE Grant No. DE-FG02-13ER41967. ORNL is managed by UT-Battelle, LLC, under Contract No. DE-AC05-00OR22725 for the US Department of Energy. The US Government retains, and the publisher, by accepting the article for publication, acknowledges that the US Government retains a nonexclusive, paid-up, irrevocable, worldwide license to publish or reproduce the published form of this manuscript, or allow others to do so, for US Government purposes.

FundersFunder number
National Science FoundationDMR-1808371
U.S. Department of EnergyDE-FG02-13ER41967
Directorate for Mathematical and Physical Sciences1808371
Office of Science
Basic Energy Sciences
Oak Ridge National LaboratoryDE-AC05-00OR22725
Division of Materials Sciences and Engineering

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