Magnetic properties of the (Mo2/3R1/3)2AlC (R=Ho,Dy) iMAX phases studied by x-ray magnetic circular dichroism and neutron diffraction

Maxime Barbier, Fabrice Wilhelm, Claire V. Colin, Christine Opagiste, Elsa Lhotel, Damir Pinek, Youngsoo Kim, Daniel Braithwaite, Eric Ressouche, Philippe Ohresser, Edwige Otero, Andrei Rogalev, and Thierry Ouisse
Phys. Rev. B 105, 174421 – Published 17 May 2022

Abstract

We report on the magnetic properties of single crystals of Ho- and Dy-based (Mo2/3R1/3)2AlC iMAX phases. In these nanolamellar compounds, where planes of R and Mo arranged in a skewed triangular lattice are separated by planes of Al and C, geometrical frustration and magnetic exchange interactions lead to complex magnetic properties. Temperature-dependent bulk magnetization, specific heat, and resistivity measurements reveal two magnetic phase transitions in Dy iMAX (15 and 12 K) and only one in Ho iMAX (8.5 K). Strong magnetic anisotropy and metamagnetic transitions with a step at 13 of saturation moment along the crystal a axis are observed in field-dependent bulk magnetization curves. X-ray magnetic circular dichroism measurements unveil induced moments on Mo and Al, and a quantitative estimation of the orbital and spin moments of Mo based on magneto-optical sum rules suggests an unusual interaction between the R 4f and the Mo 4d magnetic moments. Magnetic structures are derived from neutron diffraction measurements, revealing a zero-field incommensurate amplitude modulated order in both compounds, followed by an antiferromagnetic equal-moments structure at lower temperature for Dy iMAX. The bulk magnetization 13 step is found to be linked to the flip of one R moment out of three within the planes. Detailed phase diagrams for Ho and Dy iMAX are derived from these measurements.

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  • Received 24 January 2022
  • Accepted 2 May 2022

DOI:https://doi.org/10.1103/PhysRevB.105.174421

©2022 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Maxime Barbier1,2,*, Fabrice Wilhelm2,†, Claire V. Colin3, Christine Opagiste3, Elsa Lhotel3, Damir Pinek2, Youngsoo Kim4, Daniel Braithwaite4, Eric Ressouche5, Philippe Ohresser6, Edwige Otero6, Andrei Rogalev2, and Thierry Ouisse1,‡

  • 1Université Grenoble Alpes, Centre national de la recherche scientifique (CNRS), Grenoble INP, Laboratoire des Matériaux et du Génie Physique (LMGP), F-38000 Grenoble, France
  • 2European Synchrotron Radiation Facility (ESRF), 71 Avenue des Martyrs, CS 40220, 38043 Grenoble Cedex 9, France
  • 3Université Grenoble Alpes, Centre national de la recherche scientifique (CNRS), Grenoble INP, Institut Néel, F-38000 Grenoble, France
  • 4Université Grenoble Alpes, Grenoble INP, Commissariat à l’énergie atomique et aux énergies alternatives (CEA), Interdisciplinary Research Institute of Grenoble (IRIG), Quantum Photonics, Electronics and Engineering Laboratory (PHELIQS), F-38054, Grenoble, France
  • 5Université Grenoble Alpes, Grenoble INP, Commissariat à l’énergie atomique et aux énergies alternatives (CEA), Interdisciplinary Research Institute of Grenoble (IRIG)-Modeling and Exploration of Materials Laboratory (MEM), 38000 Grenoble, France
  • 6Synchrotron-SOLEIL, L’Orme des Merisiers, Saint-Aubin 91192, France

  • *Corresponding author: maxime.barbier@grenoble-inp.fr
  • Corresponding author: wilhelm@esrf.fr
  • Corresponding author: thierry.ouisse@grenoble-inp.fr

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Issue

Vol. 105, Iss. 17 — 1 May 2022

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