Gravitational time dilation in extended quantum systems: The case of light clocks in Schwarzschild spacetime

IF 4.2 Q2 QUANTUM SCIENCE & TECHNOLOGY
Tupac Bravo, D. Rätzel, I. Fuentes
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引用次数: 1

Abstract

The precision of optical atomic clocks is approaching a regime where they resolve gravitational time dilation on smaller scales than their own extensions. Hence, an accurate description of quantum clocks has to take their spatial extension into account. In this article, as a first step toward a fully relativistic description of extended quantum clocks, we investigate a quantized version of Einstein's light clock fixed at a constant distance from a large massive object like the Earth. The model consists of a quantum light field in a one-dimensional cavity in Schwarzschild spacetime, where the distance between the mirrors is fixed by a rigid rod. By comparing a vertical and a horizontal clock, we propose an operational way to define the clock time when the clock resolves gravitational time dilation on scales smaller than its extension. In particular, we show that the time measured by the vertical light clock is equivalent to the proper time defined at its center. We also derive fundamental bounds on the precision of these clocks for measurements of proper time and the Schwarzschild radius.
扩展量子系统中的引力时间膨胀:史瓦西时空中的光钟
光学原子钟的精度正在接近一种状态,即它们在比自身扩展更小的尺度上解决引力时间膨胀。因此,对量子钟的精确描述必须考虑到它们的空间扩展。在本文中,作为对扩展量子钟进行完全相对论性描述的第一步,我们研究了爱因斯坦光钟的量子化版本,光钟固定在与地球等大质量物体的恒定距离上。该模型由史瓦西时空中一维腔中的量子光场组成,其中镜子之间的距离由刚性杆固定。通过比较垂直时钟和水平时钟,我们提出了一种定义时钟时间的操作方法,当时钟在小于其扩展的尺度上解决引力时间膨胀时。特别地,我们证明了由垂直光钟测量的时间与在其中心定义的固有时是等价的。我们还推导了这些时钟测量固有时和史瓦西半径精度的基本界限。
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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