Fundamental Complement of a Gravitating Region
Raphael Bousso, Sami Kaya

TL;DR
This paper introduces the concept of a fundamental complement for gravitating regions in spacetime, refining entanglement wedge definitions and exploring their properties across various cosmological models, including de Sitter and AdS spaces.
Contribution
It defines the fundamental complement of a gravitating region and demonstrates how entanglement wedges relate to these complements in general spacetimes.
Findings
The fundamental complement $ ilde{a}$ is the smallest wedge containing all infinite world lines in the spacelike complement of $a$.
Entanglement wedge $e(a)$ is the spacelike complement of $e( ilde a)$ in the bulk.
De Sitter space is not trivially reconstructible, unlike Big Bang cosmologies.
Abstract
Any gravitating region in any spacetime gives rise to a generalized entanglement wedge, the hologram . Holograms exhibit properties expected of fundamental operator algebras, such as strong subadditivity, nesting, and no-cloning. But the entanglement wedge EW of an AdS boundary region with commutant satisfies an additional condition, complementarity: EW is the spacelike complement of EW in the bulk. Here we identify an analogue of the boundary commutant in general spacetimes: given a gravitating region , its \emph{fundamental complement} is the smallest wedge that contains all infinite world lines contained in the spacelike complement of . We refine the definition of by requiring that it be spacelike to . We prove that is the spacelike complement of when the latter is computed…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories
