2013
DOI: 10.1007/jhep04(2013)022
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Towards the fast scrambling conjecture

Abstract: Many proposed quantum mechanical models of black holes include highly nonlocal interactions. The time required for thermalization to occur in such models should reflect the relaxation times associated with classical black holes in general relativity. Moreover, the time required for a particularly strong form of thermalization to occur, sometimes known as scrambling, determines the time scale on which black holes should start to release information. It has been conjectured that black holes scramble in a time lo… Show more

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Cited by 396 publications
(474 citation statements)
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“…Also, as shown in the previous section, notice that any other entanglement entropy associated to other subsystems reach the entanglement plateaux at this time scale as well. At this point, we want to remark that this result, if correct, furnish a counterexample of the mean field bound presented in [36]. In ref.…”
Section: Jhep08(2016)081mentioning
confidence: 57%
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“…Also, as shown in the previous section, notice that any other entanglement entropy associated to other subsystems reach the entanglement plateaux at this time scale as well. At this point, we want to remark that this result, if correct, furnish a counterexample of the mean field bound presented in [36]. In ref.…”
Section: Jhep08(2016)081mentioning
confidence: 57%
“…We want to stress again that the lower bounds presented in ref. [36] seem not to be valid generically. The breakdown of the mean field approximation, or analogously the breakdown of the factorization of the initial state (3.5), occurs on a time scale given by t = 1/R, independent of the system size, see (3.6).…”
Section: Jhep08(2016)081mentioning
confidence: 92%
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