Entanglement dynamics in κ-deformed spacetime

IF 6.4 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Science China Physics, Mechanics & Astronomy Pub Date : 2024-08-16 DOI:10.1007/s11433-023-2419-7
Xiaobao Liu, Zehua Tian, Jiliang Jing
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Abstract

We treat two identical and mutually independent two-level atoms that are coupled to a quantum field as an open quantum system. The master equation that governs their evolution is derived by tracing over the degree of freedom of the field. With this, we compare the entanglement dynamics of the two atoms moving with different trajectories in κ-deformed and Minkowski spacetimes. Notably, when the environment-induced interatomic interaction does not exist, the entanglement dynamics of two static atoms in κ-deformed spacetime are reduced to that in Minkowski spacetime in the case that the spacetime deformation parameter κ is sufficiently large as theoretically predicted. However, if the atoms undergo relativistic motion, regardless of whether inertial or non-inertial, their entanglement dynamics in κ-deformed spacetime behave differently from that in Minkowski spacetime even when κ is large. We investigate various types of entanglement behavior, such as decay and generation, and discuss how different relativistic motions, such as uniform motion in a straight line and circular motion, amplify the differences in the entanglement dynamics between the κ-deformed and Minkowski spacetime cases. In addition, when the environment-induced interatomic interaction is considered, we find that it may also enhance the differences in the entanglement dynamics between these two spacetimes. Thus, in principle, one can tell whether she/he is in κ-deformed or Minkowski spacetime by checking the entanglement behavior between two atoms in certain circumstances.

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κ变形时空中的纠缠动力学
我们将与量子场耦合的两个相同且相互独立的两级原子视为一个开放的量子系统。通过追踪场的自由度,我们得出了支配它们演化的主方程。据此,我们比较了在κ-变形和闵科夫斯基时空中以不同轨迹运动的两个原子的纠缠动力学。值得注意的是,当环境诱导的原子间相互作用不存在时,在时空变形参数κ足够大的情况下,两个静态原子在κ-变形时空中的纠缠动力学会被还原为在闵科夫斯基时空中的纠缠动力学,正如理论预测的那样。然而,如果原子发生相对论运动,不管是惯性运动还是非惯性运动,即使κ很大,它们在κ变形时空中的纠缠动力学表现也与在闵科夫斯基时空中的不同。我们研究了各种类型的纠缠行为,如衰减和生成,并讨论了不同的相对论运动,如直线匀速运动和圆周运动,是如何放大κ-变形时空和闵科夫斯基时空中纠缠动力学的差异的。此外,当考虑到环境诱导的原子间相互作用时,我们发现它也会增强这两种时空之间的纠缠动力学差异。因此,原则上,人们可以通过检查两个原子在某些情况下的纠缠行为来判断自己是处于κ-变形时空还是闵科夫斯基时空。
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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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