Ultrasound investigation of Ce2Zr2O7 at low temperatures and in high magnetic fields.

ORAL

Abstract

Through careful controlling the atmosphere during the growth of Ce2Zr2O7 we have been able to stabilize Ce3+ and prevent the formation of non-magnetic Ce4+.1 This allows us to study the interesting case of doublet-octupole moment on a pyrochlore lattice. In the pyrochlore structure the Ce3+ J = 5/2 multiplet is split by crystal field interactions resulting in wave functions for the ground state Kramers doublet which correspond to a linear combination of mJ = ±3/2 states. A generic model for these unusual doublets supports two distinct symmetry enriched U(1) QSL ground states in the corresponding quantum spin ice regimes.2 We measured ultrasound down to 20 mK and in magnetic fields of up to 10 T with the field applied along the [111] direction for transversal and longitudinal modes. In zero field we observe a softening of the modes for temperatures below 0.8 K, which is an indication for quantum fluctuations. At 20 mK, an increase of the magnetic field leads to decrease of the sound velocity and the curves show hysteresis which is reminiscent of the behaviour observed in Dy2Ti2O7 and Ho2Ti2O7.

1. H. Otobe et al., J. Phys. Chem. Solids 66, p.329 (2005).
2. Y.D. Li and G. Chen, Phys. Rev. B 95, p.041106(R) (2017).

Presenters

  • Andrea Bianchi

    Département de physique, Université de Montréal, Montréal, QC, H3T 3J7, Canada, Universite de Montreal

Authors

  • Andrea Bianchi

    Département de physique, Université de Montréal, Montréal, QC, H3T 3J7, Canada, Universite de Montreal

  • Jérémie Dudemain

    Département de physique, Université de Montréal, Montréal, QC, H3T 3J7, Canada, Universite de Montreal

  • Jonathan Gaudet

    Department of Physics and Astronomy, McMaster University, Johns Hopkins University, Baltimore, MD 21218, Institute for Quantum Matter and Department of Physics and Astronomy, Johns Hopkins University, Physics and Astronomy, Johns Hopkins University, IQM, Johns Hopkins University

  • Evan Smith

    Department of Physics and Astronomy, McMaster University, Hamilton, Ontario, Canada L8S 4M1, McMaster University, Department of Physics and Astronomy, McMaster University, Physics and Astronomy, McMaster University

  • Bruce Gaulin

    Department of Physics and Astronomy, McMaster University, McMaster University, Department of Physics and Astronomy, McMaster University, Hamilton, Ontario, Canada L8S 4M1, Physics and Astronomy, McMaster University

  • Yulia Gritsenko

    Hochfeld-Magnetlabor Dresden, Helmholtz-Zentrum Dresden-Rossendorf

  • Sergei Zherlitsyn

    Hochfeld-Magnetlabor Dresden, Helmholtz-Zentrum Dresden-Rossendorf

  • Joachim Wosnitza

    Dresden High Magnetic Field Laboratory, Helmholtz-Zentrum Dresden-Rossendorf, Hochfeld-Magnetlabor Dresden, Helmholtz-Zentrum Dresden-Rossendorf