Reflected entropy in an evaporating black hole through non-isometric map
Bin Chen, Zhi-jun Yin

TL;DR
This paper investigates reflected entropy in evaporating black holes using a non-isometric holographic map, showing consistency with the Page curve and quantum extremal surface calculations, and exploring entanglement properties between various regions.
Contribution
It introduces a non-isometric holographic map model for evaporating black holes and analyzes reflected entropy, providing new insights into entanglement structure in quantum gravity.
Findings
Entanglement entropy matches quantum extremal surface results.
Reflected entropy calculations are consistent with existing effective descriptions.
The model reproduces the Page curve for evaporating black holes.
Abstract
The black hole information paradox has been an important problem in quantum gravity. In the study of evaporating black hole, it has been proposed that the holographic map between the semi-classical effective description in bulk and the fundamental description in boundary cannot be isometric. In this work, we would like to study the reflected entropy in an evaporating black hole model through non-isometric holographic map. We assume that the evaporating is slowly enough that it makes sense to ascribe a slowly varying temperature to the Hawking radiation. We then introduce a two-sided black hole model to canonically purify the semi-classical state. The holographic map to the fundamental description is non-isometric and defined by a Haar random unitary matrix. We show that the entanglement entropy of the radiation in the model matches the result read from the quantum extremal surface…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Experimental and Theoretical Physics Studies
