2007
DOI: 10.1088/1126-6708/2007/12/027
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The arrow of time, black holes, and quantum mixing of largeNYang-Mills theories

Abstract: Quantum gravity in an AdS spacetime is described by an SU (N ) Yang-Mills theory on a sphere, a bounded many-body system. We argue that in the high temperature phase the theory is intrinsically non-perturbative in the large N limit. At any nonzero value of the 't Hooft coupling λ, an exponentially large (in N 2 ) number of free theory states of wide energy range (of order N ) mix under the interaction. As a result the planar perturbation theory breaks down. We argue that an arrow of time emerges and the dual s… Show more

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Cited by 68 publications
(102 citation statements)
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“…So even after coarse graining, the allowed values of ω seem to take effectively a continuous spectrum. See also the discussion in [55].…”
Section: Jhep10(2013)212mentioning
confidence: 97%
“…So even after coarse graining, the allowed values of ω seem to take effectively a continuous spectrum. See also the discussion in [55].…”
Section: Jhep10(2013)212mentioning
confidence: 97%
“…On the field theory side, one thus has the statement that, to all orders in 1/N , the two-point function decays to JHEP05(2016)048 Figure 1. The basic graphical unit of the Hamiltonian (2.2) studied in [4]. i i j Figure 2.…”
Section: Thermalizationmentioning
confidence: 99%
“…This late time breakdown of perturbation theory was studied in the context of matrix quantum mechanics in [4]. Reducing Yang-Mills on a sphere in terms of spherical harmonics, one obtains a Hamiltonian whose essential features can be captured by considering just two interacting matrices.…”
Section: Thermalizationmentioning
confidence: 99%
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“…Usually, simple, weakly coupled physical states in string theory are associated with gauge invariant composite operators of low dimension in the boundary field theory, rather than with the underlying DOF. The high temperature free energy is dominated by operators of very high dimension, which have dense spectrum of dimensions corresponding to the spectrum of a chaotic Hamiltonian [32]. Furthermore, as we will see in a moment, a typical theory with a large number of almost free fields cannot have a c.c.…”
Section: Ads/cftmentioning
confidence: 93%