Cited 2 time in
Cited 2 time in
Page curves for tripartite systems
- Page curves for tripartite systems
- Hwang, Junha; Lee, Deok Sang; Nho, Dongju; Oh, Jeonghun; Park, Hyosub; Yeom, Dong-Han; Zoe, Heeseung
- DGIST Authors
- Hwang, Junha; Lee, Deok Sang; Nho, Dongju; Oh, Jeonghun; Park, Hyosub; Zoe, Heeseung
- Issue Date
- Classical and Quantum Gravity, 34(14)
- Article Type
- Black Hole Complementarity; Black Hole Information; Black Hole Remnants; Entanglement Entropy; Evolution; False Vacuum Bubbles; Information; Information Theory; Mixed States; Pure States
- We investigate information flow and Page curves for tripartite systems. We prepare a tripartite system (say, A, B, and C) of a given number of states and calculate information and entropy contents by assuming random states. Initially, every particle was in A (this means a black hole), and as time goes on, particles move to either B (this means Hawking radiation) or C (this means a broadly defined remnant, including a non-local transport of information, the last burst, an interior large volume, or a bubble universe, etc). If the final number of states of the remnant is smaller than that of Hawking radiation, then information will be stored by both the radiation and the mutual information between the radiation and the remnant, while the remnant itself does not contain information. On the other hand, if the final number of states of the remnant is greater than that of Hawking radiation, then the radiation contains negligible information, while the remnant and the mutual information between the radiation and the remnant contain information. Unless the number of states of the remnant is large enough compared to the entropy of the black hole, Hawking radiation must contain information; and we meet the menace of black hole complementarity again. Therefore, this contrasts the tension between various assumptions and candidates of the resolution of the information loss problem. © 2017 IOP Publishing Ltd.
- Institute of Physics Publishing
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