Timelike and gravitational anomalous entanglement from the inner horizon
Qiang Wen, Mingshuai Xu, Haocheng Zhong

TL;DR
This paper explores the properties of the inner RT surface in AdS$_3$/CFT$_2$, revealing its connection to timelike entanglement entropy, and examines how gravitational anomalies modify holographic entanglement measures.
Contribution
It introduces a new interpretation of the inner RT surface, linking it to timelike entanglement entropy and gravitational anomalies in TMG, expanding understanding of holographic entanglement.
Findings
Inner RT surface corresponds to the real part of holographic timelike entanglement entropy.
Inner RT surface's correction reproduces the entanglement entropy correction in TMG.
Inner EWCS represents the mixed state correlation in the presence of gravitational anomalies.
Abstract
In the context of the AdS/CFT, the boundary causal development and the entanglement wedge of any boundary spacelike interval can be mapped to a thermal CFT and a Rindler respectively via certain boundary and bulk Rindler transformations. Nevertheless, the Rindler mapping is not confined in the entanglement wedges. While the outer horizon of the Rindler is mapped to the RT surface, we also identify the pre-image of the inner horizon in the original AdS, which we call the inner RT surface. In this paper we give some new physical interpretation for the inner RT surface. First, the inner RT surface breaks into two pieces which anchor on the two tips of the causal development. Furthermore, we can take the two tips as the endpoints of a certain timelike interval and the inner RT surface is exactly the spacelike geodesic…
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Taxonomy
TopicsCosmology and Gravitation Theories · Computational Physics and Python Applications · Relativity and Gravitational Theory
