Generalized Rindler Wedge and Holographic Observer Concordance
Xin-Xiang Ju, Wen-Bin Pan, Ya-Wen Sun, Yuan-Tai Wang

TL;DR
This paper introduces a new way to define gravitational subsystems using accelerating observers and their horizons, establishing a holographic framework that links observer-based partitions to holographic dualities and entanglement entropy.
Contribution
It defines generalized Rindler wedges based on spacelike surfaces satisfying a global convexity condition, linking observer horizons to holographic duality and entanglement entropy.
Findings
Entanglement entropy proportional to the surface area of Rindler-convex regions
Holographic interpretation of generalized Rindler wedges supported by multiple evidence
Establishment of a holographic observer concordance framework
Abstract
Defining gravitational subsystems has long been challenging due to the lack of the conventional notion of locality in gravity. In this work, we define gravitational subsystems from the observable spacetime subregions of a set of well-defined accelerating observers. We study the most general horizons of accelerating observers and find that in a general spacetime, only spacelike surfaces satisfying a global condition could become horizons of well-defined accelerating observers, which we name the Rindler-convexity condition. The entanglement entropy associated with a Rindler-convex region is proportional to the area of the enclosing surface. The subregions defined from this observer perspective is named the generalized Rindler wedge. This provides a physical origin for defining gravitational subsystems associated with one type of Type III von Neumann subalgebra. We propose the holographic…
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Taxonomy
TopicsCosmology and Gravitation Theories · Advanced Differential Geometry Research · Geometric Analysis and Curvature Flows
