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• W2596758519 startingPage "2881" @default.
• W2596758519 abstract "If a system falls through a black hole horizon, then its information is lost to an observer at infinity. But we argue that the accessible information is lost before the horizon is crossed. The temperature of the hole limits information carrying signals from a system that has fallen too close to the horizon. Extremal holes have T = 0, but there is a minimum energy required to emit a quantum in the short proper time left before the horizon is crossed. If we attempt to bring the system back to infinity for observation, then acceleration radiation destroys the information. All three considerations give a critical distance from the horizon [Formula: see text], where r H is the horizon radius and ΔE is the energy scale characterizing the system. For systems in string theory where we pack information as densely as possible, this acceleration constraint is found to have a geometric interpretation. These estimates suggest that in theories of gravity we should measure information not as a quantity contained inside a given system, but in terms of how much of that information can be reliably accessed by another observer." @default.
• W2596758519 created "2017-03-23" @default.
• W2596758519 creator A5016809443 @default.
• W2596758519 date "2011-12-31" @default.
• W2596758519 modified "2023-09-25" @default.
• W2596758519 title "EFFECTIVE INFORMATION LOSS OUTSIDE THE HORIZON" @default.
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• W2596758519 doi "https://doi.org/10.1142/s0218271811020767" @default.
• W2596758519 hasPublicationYear "2011" @default.
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