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    Multistage spin correlations in the s=12 stuffed hyper-star lattice Li2Cu2(MoO4)3

    J. Khatua1, Taeyun Kim1, G. Senthil Murugan2,3,*, S. M. Kumawat4, C.-L. Huang4, Yugo Oshima5, Hiroyuki Nojiri6, Gerald Morris7, Sarah R. Dunsiger7 et al.

    Heung-Sik Kim8, K. Sritharan2, Shankar Mani2, R. Sankar2,†, and Kwang-Yong Choi1,‡

    • 1Department of Physics, Sungkyunkwan University, Suwon 16419, Republic of Korea
    • 2Institute of Physics, Academia Sinica, Taipei 11529, Taiwan
    • 3Department of Physics, St. Joseph's College of Engineering, OMR, Chennai 600 119, India
    • 4Department of Physics and Center for Quantum Frontiers of Research and Technology (QFort), National Cheng Kung University, Tainan 70101, Taiwan
    • 5RIKEN Pioneering Research Institute, Wako, Saitama 351-0198, Japan
    • 6Institute for Materials Research, Tohoku University, Sendai 980-8577, Japan
    • 7Centre for Molecular and Materials Science, TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
    • 8Department of Energy Technology, Korea Institute of Energy Technology, Naju-si 58217, Republic of Korea

    • *Contact author: nanosen@gmail.com
    • †Contact author: sankarndf@gmail.com
    • ‡Contact author: choisky99@skku.edu

    Phys. Rev. B 113, 104441 – Published 24 March, 2026

    DOI: https://doi.org/10.1103/nv1l-dgv9

    Abstract

    The star lattice, which can be visualized as a honeycomb network with each vertex replaced by a triangle, provides a rare platform for realizing exotic quantum states such as quantum spin liquids and disorder-driven random-singlet (RS) states. Herein, we investigate the ground-state properties of the three-dimensional (3D) stuffed hyper-star lattice Li2Cu2(MoO4)3, which exhibits a crossover from short-range spin correlations to a disorder-driven RS-like state below T*∼15.8K. Thermodynamic and microscopic measurements capture this crossover through a change in the power-law behavior of various observables, from ∼T0.25 for T>T* to ∼T−0.50 for T<T*. Upon further cooling, a quasifrozen state emerges near Tf=0.32K, likely associated with weakly coupled spin chains within the hyper-star spin network. Our results underscore the crucial role of orphan spins and weak residual interactions in stabilizing a disorder-driven quantum-disordered state in three dimensions.

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