Islands in Schwarzschild black holes
Koji Hashimoto, Norihiro Iizuka, Yoshinori Matsuo
Abstract
A bstract We study the Page curve for asymptotically flat eternal Schwarzschild black holes in four and higher spacetime dimensions. Before the Page time, the entanglement entropy grows linearly in time. After the Page time, the entanglement entropy of a given region outside the black hole is largely modified by the emergence of an island, which extends to the outer vicinity of the event horizon. As a result, it remains a constant value which reproduces the Bekenstein-Hawking entropy, consistent with the finiteness of the von Neumann entropy for an eternal black hole.
Topics & Concepts
PhysicsSchwarzschild radiusEntropy (arrow of time)Quantum entanglementBlack hole (networking)SpacetimeBlack hole thermodynamicsWhite holeSchwarzschild metricMathematical physicsVon Neumann entropyEvent horizonFuzzballTheoretical physicsMicro black holePhoton sphereQuantum mechanicsCharged black holeHawking radiationBoltzmann's entropy formulaExtremal black holeBlack Holes and Theoretical PhysicsNoncommutative and Quantum Gravity TheoriesCosmology and Gravitation Theories