Magnetism of NaYbS2: From finite temperatures to ground state

IF 6.4 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY
Weizhen Zhuo, Zheng Zhang, Mingtai Xie, Anmin Zhang, Jianting Ji, Feng Jin, Qingming Zhang
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Abstract

Rare-earth chalcogenide compounds ARECh2 (A = alkali or monovalent metal, RE = rare earth, Ch = O, S, Se, Te) are a large family of quantum spin liquid (QSL) candidate materials. NaYbS2 is a representative member of the family. Several key issues on NaYbS2, particularly how to determine the highly anisotropic spin Hamiltonian and describe the magnetism at finite temperatures and the ground state, remain to be addressed. In this paper, we conducted an in-depth and comprehensive study on the magnetism of NaYbS2 from finite temperatures to the ground state. Firstly, we successfully detected three crystalline electric field (CEF) excitation energy levels using low-temperature Raman scattering technique. Combining them with the CEF theory and magnetization data, we worked out the CEF parameters, CEF energy levels, and CEF wavefunctions. We further determined a characteristic temperature of ∼40 K, above which the magnetism is dominated by CEF excitations while below which the spin-exchange interactions play a main role. The characteristic temperature has been confirmed by the temperature-dependent electron spin resonance (ESR) linewidth. Low-temperature ESR experiments on the dilute magnetic doped crystal of NaYb0.1Lu0.9S2 further helped us to determine the accurate g-factor. Next, we quantitatively obtained the spin-exchange interactions in the spin Hamiltonian by consistently simulating the magnetization and specific heat data. Finally, the above studies allow us to explore the ground state magnetism of NaYbS2 by using the density matrix renormalization group. We combined numerical calculations and experimental results to demonstrate that the ground state of NaYbS2 is a Dirac-like QSL.

NaYbS2 的磁性:从有限温度到基态
稀土瑀化合物 ARECh2(A = 碱金属或一价金属,RE = 稀土,Ch = O、S、Se、Te)是一个庞大的量子自旋液体(QSL)候选材料家族。NaYbS2 是该家族的代表成员。关于 NaYbS2 的几个关键问题,特别是如何确定高度各向异性的自旋哈密顿,以及如何描述有限温度下的磁性和基态,仍有待解决。在本文中,我们对 NaYbS2 从有限温度到基态的磁性进行了深入而全面的研究。首先,我们利用低温拉曼散射技术成功探测到了三个晶体电场(CEF)激发能级。结合 CEF 理论和磁化数据,我们计算出了 CEF 参数、CEF 能级和 CEF 波函数。我们进一步确定了一个 ∼40 K 的特征温度,在此温度之上,磁性主要由 CEF 激发所主导,而在此温度之下,自旋交换相互作用则起主要作用。随温度变化的电子自旋共振(ESR)线宽证实了这一特征温度。在稀磁掺杂的 NaYb0.1Lu0.9S2 晶体上进行的低温 ESR 实验进一步帮助我们确定了精确的 g 因子。接下来,我们通过持续模拟磁化和比热数据,定量地获得了自旋哈密顿中的自旋交换相互作用。最后,通过上述研究,我们利用密度矩阵重正化群探索了 NaYbS2 的基态磁性。我们将数值计算与实验结果相结合,证明了 NaYbS2 的基态是一种类似于狄拉克的 QSL。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Science China Physics, Mechanics & Astronomy
Science China Physics, Mechanics & Astronomy PHYSICS, MULTIDISCIPLINARY-
CiteScore
10.30
自引率
6.20%
发文量
4047
审稿时长
3 months
期刊介绍: Science China Physics, Mechanics & Astronomy, an academic journal cosponsored by the Chinese Academy of Sciences and the National Natural Science Foundation of China, and published by Science China Press, is committed to publishing high-quality, original results in both basic and applied research. Science China Physics, Mechanics & Astronomy, is published in both print and electronic forms. It is indexed by Science Citation Index. Categories of articles: Reviews summarize representative results and achievements in a particular topic or an area, comment on the current state of research, and advise on the research directions. The author’s own opinion and related discussion is requested. Research papers report on important original results in all areas of physics, mechanics and astronomy. Brief reports present short reports in a timely manner of the latest important results.
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