Holographic entanglement in spin network states: A focused review

IF 4.2 Q2 QUANTUM SCIENCE & TECHNOLOGY
Eugenia Colafranceschi, G. Adesso
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引用次数: 7

Abstract

In the long-standing quest to reconcile gravity with quantum mechanics, profound connections have been unveiled between concepts traditionally pertaining to a quantum information theory, such as entanglement, and constitutive features of gravity, like holography. Developing and promoting these connections from the conceptual to the operational level unlock access to a powerful set of tools which can be pivotal toward the formulation of a consistent theory of quantum gravity. Here, we review recent progress on the role and applications of quantum informational methods, in particular tensor networks, for quantum gravity models. We focus on spin network states dual to finite regions of space, represented as entanglement graphs in the group field theory approach to quantum gravity, and illustrate how techniques from random tensor networks can be exploited to investigate their holographic properties. In particular, spin network states can be interpreted as maps from bulk to boundary, whose holographic behavior increases with the inhomogeneity of their geometric data (up to becoming proper quantum channels). The entanglement entropy of boundary states, which are obtained by feeding such maps with suitable bulk states, is then proved to follow a bulk area law with corrections due to the entanglement of the bulk state. We further review how exceeding a certain threshold of bulk entanglement leads to the emergence of a black hole-like region, revealing intriguing perspectives for quantum cosmology.
自旋网络态的全息纠缠:重点综述
在长期寻求调和引力与量子力学的过程中,传统上与量子信息理论有关的概念(如纠缠)与引力的本构特征(如全息)之间的深刻联系已经显现。发展和促进这些从概念到操作层面的联系,可以获得一套强大的工具,这些工具对制定一致的量子引力理论至关重要。在这里,我们回顾了量子信息方法,特别是张量网络在量子引力模型中的作用和应用的最新进展。我们专注于空间有限区域的对偶自旋网络状态,在量子引力的群场论方法中用纠缠图表示,并说明如何利用随机张量网络的技术来研究它们的全息特性。特别是,自旋网络状态可以被解释为从体到边界的映射,其全息行为随着几何数据的不均匀性而增加(直到成为合适的量子通道)。然后,通过向这些映射提供合适的体态获得的边界态的纠缠熵,被证明遵循体面积定律,并由于体态的纠缠而进行校正。我们进一步回顾了体纠缠超过一定阈值是如何导致类黑洞区域出现的,揭示了量子宇宙学的有趣视角。
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
CiteScore
9.90
自引率
0.00%
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