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三方系统中基于雷尼相对熵的纠缠一夫一妻制

Rényi relative entropy based monogamy of entanglement in tripartite systems.

作者信息

Mannaï Marwa, Sati Hisham, Byrnes Tim, Radhakrishnan Chandrashekar

机构信息

Center for Quantum and Topological Systems, NYUAD Research Institute, New York University, Abu Dhabi, UAE.

Mathematics, Division of Science, New York University Abu Dhabi (NYUAD), Abu Dhabi, UAE.

出版信息

Sci Rep. 2025 Jan 2;15(1):530. doi: 10.1038/s41598-024-84153-1.

DOI:10.1038/s41598-024-84153-1
PMID:39747288
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11695734/
Abstract

A comprehensive investigation of the entanglement characteristics is carried out on tripartite spin-1/2 systems, examining prototypical tripartite states, the thermal Heisenberg model, and the transverse field Ising model. The entanglement is computed using the Rényi relative entropy. In the traditional Rényi relative entropy, the generalization parameter α can take values only in the range [Formula: see text] due to the requirements of joint convexity of the measure. To use the Rényi relative entropy over a wider range of α, we use the sandwiched form which is jointly convex in the regime [Formula: see text]. In prototypical tripartite states, we find that GHZ states are monogamous, but surprisingly so are W states. On the other hand, star states exhibit polygamy, due to the higher level of purity of the bipartite subsystems. For spin models, we study the dependence of entanglement on various parameters such as temperature, spin-spin interaction, and anisotropy, and identify regions where entanglement is the largest. The Rényi parameter α scales the amount of entanglement in the system. The entanglement measure based on the traditional and the sandwiched Rényi relative entropies obey the Araki-Lieb-Thirring inequality. In the Heisenberg models, namely the XYZ, XXZ, and XY models, the system is always monogamous. However, in the transverse field Ising model, the state is initially polygamous and becomes monogamous with temperature and coupling.

摘要

我们对三方自旋 - 1/2 系统的纠缠特性进行了全面研究,考察了典型的三方态、热海森堡模型和横场伊辛模型。使用雷尼相对熵来计算纠缠。在传统的雷尼相对熵中,由于测度的联合凸性要求,泛化参数α只能在[公式:见文本]范围内取值。为了在更广泛的α范围内使用雷尼相对熵,我们使用在[公式:见文本]范围内联合凸的夹心形式。在典型的三方态中,我们发现 GHZ 态是一夫一妻制的,但令人惊讶的是 W 态也是如此。另一方面,星态表现出多配偶制,这是由于二分量子系统的纯度较高。对于自旋模型,我们研究了纠缠对温度、自旋 - 自旋相互作用和各向异性等各种参数的依赖性,并确定了纠缠最大的区域。雷尼参数α衡量了系统中的纠缠量。基于传统和夹心雷尼相对熵的纠缠测度服从荒木 - 利布 - Thirring 不等式。在海森堡模型,即 XYZ、XXZ 和 XY 模型中,系统总是一夫一妻制的。然而,在横场伊辛模型中,状态最初是多配偶制的,并且随着温度和耦合而变为一夫一妻制。

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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0840/11695734/d3e611683398/41598_2024_84153_Fig10_HTML.jpg
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