Relation between Ga ordering and magnetostriction of Fe-Ga alloys studied by x-ray diffuse scattering
Creators
- 1. Iowa State Univ., Ames, IA (United States)
- 2. Ames National Laboratory, Ames, IA (United States)
Description
Transmission synchrotron diffraction was employed to characterize the Ga ordering in magnetostrictive Fe100-xGax alloys with Ga concentrations from 0 to 20.3 at.%. The experiments focused on the development of atomic short-range ordering (SRO) by analysis of the diffuse scattering appearing at superlattice positions of the D03 ordered alloy structure. No SRO was found for Ga concentrations less than 4 at. %. Between 13 and 20.3 at. %, D03-type SRO clusters are observed whose size increases with Ga concentration for both slow-cooled and quenched samples. Thermal quenching of the samples suppresses the cluster sizes when compared to slow-cooled samples of the same concentration. For quenched samples with large Ga concentration, Ga pairing is evidenced by growing B2-type correlations. At low concentrations, the presence of SRO appears to have little (if any) effect on the enhanced magnetostriction. However, the dramatic suppression of magnetostriction near ∼ 20 at. % Ga can be linked rapid growth of SRO just before the onset of long-range chemical order.
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review. B, Condensed Matter and Materials Physics
- Journal Volume
- 81
- Journal Issue
- 5
- Journal Page Range
- p. 054432
- ISSN
- 1098-0121
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 42026198
- Subject category
- S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY; S36: MATERIALS SCIENCE;
- Descriptors DEI
- ALLOYS; DIFFRACTION; DIFFUSE SCATTERING; MAGNETOSTRICTION; QUENCHING; SUPERLATTICES; SYNCHROTRONS
- Descriptors DEC
- ACCELERATORS; COHERENT SCATTERING; CYCLIC ACCELERATORS; DIFFRACTION; MAGNETIC PROPERTIES; PHYSICAL PROPERTIES; SCATTERING
Optional Information
- Notes
- 9 pages, doi 10.1103/PhysRevB.81.054432