Vacuum-Bounded States and the Entropy of Black Hole Evaporation
Ken D. Olum

TL;DR
This paper investigates the maximum entropy of vacuum-bounded states in a one-dimensional model, explores implications for black hole information loss, and finds that low-energy vacuum-bounded states can have unexpectedly high entropy.
Contribution
It introduces a numerical method to compute the maximum entropy of vacuum-bounded states and applies these results to black hole evaporation and information paradox.
Findings
Maximum entropy bounds for vacuum-bounded states at high energies.
Implication that black hole final explosions cannot emit large amounts of information.
At low energies, vacuum-bounded states can have much higher entropy than rigid box states.
Abstract
We call a state ``vacuum bounded'' if every measurement performed outside a specified interior region gives the same result as in the vacuum. We compute the maximum entropy of a vacuum-bounded state with a given energy for a one-dimensional model, with the aid of numerical calculations on a lattice. For large energies we show that a vacuum-bounded system with length and a given energy has entropy no more than , where is the entropy in a rigid box with the same size and energy. Assuming that the state resulting from the evaporation of a black hole is similar to a vacuum-bounded state, and that the similarity between vacuum-bounded and rigid box problems extends from 1 to 3 dimensions, we apply these results to the black hole information paradox. Under these assumptions we conclude that large amounts of information cannot be emitted in the final…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Quantum Electrodynamics and Casimir Effect
