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Islands in cosmology

Thomas Hartman, Yikun Jiang, Edgar Shaghoulian

2020Journal of High Energy Physics160 citationsDOIOpen Access PDF

Abstract

A bstract A quantum extremal island suggests that a region of spacetime is encoded in the quantum state of another system, like the encoding of the black hole interior in Hawking radiation. We study conditions for islands to appear in general spacetimes, with or without black holes. They must violate Bekenstein’s area bound in a precise sense, and the boundary of an island must satisfy several other information-theoretic inequalities. These conditions combine to impose very strong restrictions, which we apply to cosmological models. We find several examples of islands in crunching universes. In particular, in the four-dimensional FRW cosmology with radiation and a negative cosmological constant, there is an island near the turning point when the geometry begins to recollapse. In a two-dimensional model of JT gravity in de Sitter spacetime, there are islands inside crunches that are encoded at future infinity or inside bubbles of Minkowski spacetime. Finally, we discuss simple tensor network toy models for islands in cosmology and black holes.

Topics & Concepts

PhysicsCosmologyMinkowski spaceFriedmann–Lemaître–Robertson–Walker metricTheoretical physicsQuantum cosmologyBlack hole (networking)Quantum gravitySpacetimeHawking radiationWhite holeDe Sitter universeLoop quantum cosmologyClassical mechanicsMathematical physicsPhysical cosmologyTensor (intrinsic definition)Cosmological constantBoundary (topology)Quantum field theory in curved spacetimede Sitter–Schwarzschild metricHawkingQuantum stateBlack hole information paradoxQuantum geometrySimple (philosophy)QuantumQuantum mechanicsLoop quantum gravityMicro black holeDe Sitter spaceBlack Holes and Theoretical PhysicsNoncommutative and Quantum Gravity TheoriesAdvanced Operator Algebra Research
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