Spin Noise Spectroscopy of Herbertsmithite ZnCu<sub>3</sub>(OH)<sub>6</sub>Cl<sub>2</sub>
ORAL · Invited
Abstract
An emerging concept for identifying various types of spin liquid states, which are often altogether designated by the absence of order, is through their characteristic spin noise. This spin noise approach has been successfully demonstrated in the classical spin ice material Dy2Ti2O7 [1,2] and the spiral spin liquid material Ca10Cr7O28 [3]. Here we report the spin noise spectroscopy study of Herbertsmithite ZnCu3(OH)6Cl2 [4], an iconic quantum spin liquid candidate with S = 1/2 Cu2+ kagome layers whose exact spin ground state has remained controversial. While much effort has focused on the kagome layer, here we exploit spin dynamics of the interlayer Cu2+ “witness-spins” which, interacting primarily via the kagome layer, evidence its quantum dynamics.
To do so, we have developed a mK SQUID-based spin noise spectrometer with fT/√Hz-sensitivity and µs-time resolution to measure the magnetization noise M(t, T) in ZnCu3(OH)6Cl2. Below 400 mK, intense witness-spin fluctuations emerge over frequencies ranging 0.1 Hz < f < 1 kHz with a scale-invariant power spectral density SM(ω,T)∝1/ωα(T). We find a sharp transition at T* = 260 mK, indicated by a peak in both the noise variance and the µT-DC susceptibility. Below T*, the noise spectrum stabilizes as nearly 1/ω and the spin state enters an ultra-slow “aging” regime over at least 105 s. We theoretically explore spinon RKKY interactions between the witness-spins for consistency with all these phenomena.
[1] R. Dusad et al. Nature 571, 234 (2019)
[2] J. C. Dasini et al. arXiv:2408.00460 (2024)
[3] H. Takahashi & C.-C. Hsu et al. arXiv:2405.02075 (2024)
[4] H. Takahashi & J. Murphy et al. submitted (2024)
To do so, we have developed a mK SQUID-based spin noise spectrometer with fT/√Hz-sensitivity and µs-time resolution to measure the magnetization noise M(t, T) in ZnCu3(OH)6Cl2. Below 400 mK, intense witness-spin fluctuations emerge over frequencies ranging 0.1 Hz < f < 1 kHz with a scale-invariant power spectral density SM(ω,T)∝1/ωα(T). We find a sharp transition at T* = 260 mK, indicated by a peak in both the noise variance and the µT-DC susceptibility. Below T*, the noise spectrum stabilizes as nearly 1/ω and the spin state enters an ultra-slow “aging” regime over at least 105 s. We theoretically explore spinon RKKY interactions between the witness-spins for consistency with all these phenomena.
[1] R. Dusad et al. Nature 571, 234 (2019)
[2] J. C. Dasini et al. arXiv:2408.00460 (2024)
[3] H. Takahashi & C.-C. Hsu et al. arXiv:2405.02075 (2024)
[4] H. Takahashi & J. Murphy et al. submitted (2024)
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Presenters
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Hiroto Takahashi
University of Oxford
Authors
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Hiroto Takahashi
University of Oxford
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Jack Murphy
University College Cork
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Mitikorn Wood-Thanan
University of Bristol
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Pascal Puphal
Max Planck Institute for Solid State Research
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Fabian Jerzembeck
Max Planck Institute for Chemical Physics of Solids
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Chun-Chih Hsu
University of Oxford
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jonathan ward
University College Cork
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Masahiko Isobe
Max Planck Institute for Solid State Research
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Yosuke Matsumoto
Max Planck Institute for Solid State Research
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HIDENORI TAKAGI
Max Planck Institute for Solid State Physics
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Michael Ray Norman
Argonne National Laboratory
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Stephen Blundell
University of Oxford
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Felix Flicker
University of Bristol, Cardiff Univ of Wales
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Seamus Davis
University of Oxford, UC Cork, University of Oxford