Island for Gravitationally Prepared State and Pseudo Entanglement Wedge
Masamichi Miyaji

TL;DR
This paper explores a generalized spacetime with finite initial boundary, analyzing entanglement entropy and introducing the concept of pseudo entanglement wedges, which extend entanglement wedge reconstruction in holography.
Contribution
It introduces the pseudo entanglement wedge concept, generalizes entanglement entropy bounds with islands, and studies the reconstruction of bulk matter in spacetimes with finite initial boundaries.
Findings
Entanglement entropy is bounded by the boundary area of the island.
A necessary condition for initial states to satisfy strong sub-additivity.
Reconstruction of bulk matter transition matrix is exponentially hard, extending Python's lunch conjecture.
Abstract
We consider spacetime initiated by a finite-sized initial boundary as a generalization of the Hartle-Hawking no-boundary state. We study entanglement entropy of matter state prepared by such spacetime. We find that the entanglement entropy for large subregion is given either by the initial state entanglement or the entanglement island, preventing the entropy to grow arbitrarily large. Consequently, the entanglement entropy is always bounded from above by the boundary area of the island, leading to an entropy bound in terms of the island. The island is located in the analytically continued spacetime, either at the bra or the ket part of the spacetime in Schwinger-Keldysh formalism. The entanglement entropy is given by an average of pseudo generalized entropy for each entanglement island. We find a necessary condition of the initial state to be consistent with the strong…
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