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Successive magnetic transitions of the pseudo-ternary compounds Ho1R Rh2Si2 (R=Y, La)
- Source :
- Physica B: Condensed Matter. 536:379-383
- Publication Year :
- 2018
- Publisher :
- Elsevier BV, 2018.
-
Abstract
- Magnetic measurements on the pseudo-ternary compounds Ho 1- x R x Rh 2 Si 2 (R = Y or La = Y or La) were performed in order to get information on the origin of “the successive component-separated magnetic transitions” which appear in HoRh 2 Si 2 . The lattice parameters a and c remain almost constant during changes to Y composition x , while they increase with increasing La composition x . The c / a ratios are also constant in the Y-system, and they increase with increasing x in the La-system especially for above around x = 0.4. The transition temperatures, T N1 = 29.1 K, T t = 27.3 K and T N2 =12.1 K at x = 0, decrease with increasing x . The rates of decrease for T N1 and T N2 in the Y-system accord with those in the La system below x = 0.4. The critical compositions for T N1 and T N2 are determined to be x N1 = 0.88 and x N2 = 0.59 in the La-system, respectively, and x N1 = 0.98 and x N2 = 0.75 in the Y-system. In both the systems, “the successive component-separated magnetic transitions” appear for the wide x regions. The magnetic ordered state persists in very dilute Ho-compounds in spite of much weak magnetic interactions. The effective magnetic moments are almost constant for the ordered compounds; μ eff = 10.6 ± 0.30 μ B /Ho. These behaviors are strange, indicating a strong correlation exists in these systems.
- Subjects :
- Magnetic measurements
Materials science
Magnetic moment
Condensed matter physics
Condensed Matter Physics
Magnetic phase diagram
Electronic, Optical and Magnetic Materials
Magnetic transitions
Crystallography
Lattice constant
Lattice (order)
Electrical and Electronic Engineering
Magnetic interaction
Ternary operation
Subjects
Details
- ISSN :
- 09214526
- Volume :
- 536
- Database :
- OpenAIRE
- Journal :
- Physica B: Condensed Matter
- Accession number :
- edsair.doi...........b540d1cac68417b72a6b1b943dcd026e
- Full Text :
- https://doi.org/10.1016/j.physb.2017.09.066