Information Transfer with a Gravitating Bath

H. Geng, A. Karch, Carlos Perez-Pardavila, S. Raju, L. Randall, Marcos Riojas, Sanjit Shashi
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引用次数: 162

Abstract

Late-time dominance of entanglement islands plays a critical role in addressing the information paradox for black holes in AdS coupled to an asymptotic non-gravitational bath. A natural question is how this observation can be extended to gravitational systems. To gain insight into this question, we explore how this story is modified within the context of Karch-Randall braneworlds when we allow the asymptotic bath to couple to dynamical gravity. We find that because of the inability to separate degrees of freedom by spatial location when defining the radiation region, the entanglement entropy of radiation emitted into the bath is a time-independent constant, consistent with recent work on black hole information in asymptotically flat space. If we instead consider an entanglement entropy between two sectors of a specific division of the Hilbert space, we then find non-trivial time-dependence, with the Page time a monotonically decreasing function of the brane angle -- provided both branes are below a particular angle. However, the properties of the entropy depend discontinuously on this angle, which is the first example of such discontinuous behavior for an AdS brane in AdS space.
用重力浴传递信息
纠缠岛的晚时间优势在解决渐近非引力槽耦合AdS中黑洞的信息悖论中起着关键作用。一个自然的问题是如何将这一观察推广到引力系统。为了深入了解这个问题,我们探索当我们允许渐近浴与动态重力耦合时,如何在Karch-Randall膜世界的背景下修改这个故事。我们发现,在定义辐射区域时,由于无法通过空间位置来分离自由度,因此发射到槽中的辐射的纠缠熵是一个与时间无关的常数,这与最近关于渐近平坦空间中黑洞信息的研究一致。如果我们转而考虑希尔伯特空间特定划分的两个扇区之间的纠缠熵,我们就会发现非平凡的时间依赖性,Page时间是膜角的单调递减函数——前提是两个膜都低于特定角度。然而,熵的性质不连续地依赖于这个角度,这是AdS空间中AdS膜的这种不连续行为的第一个例子。
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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