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Let $A$ be subsystem of a larger system $A \cup B$, and $\psi$ be a typical state from the subspace of the Hilbert space ${\cal H}_{AB}$ satisfying an energy constraint.
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We can motivate the result by considering a spin state of the form ψ = ( 1 / 2 N ) ∑ exp ( i θ ( σ 1 , … , σ N ) ) | σ 1 , … , σ N ⟩ \psi=(1/2^{N})\sum\exp(i\theta(\sigma_{1},\dotsc,\sigma_{N}))\,|\sigma_{1},\dotsc,\sigma_{N}\rangle , where σ i = ± \sigma_{i}=\pm . Tracing over all but the first n n spins ( N ≫ n N\gg n ) yields an approximately diagonal density matrix ≈ 𝟏 / 2 n \approx{\bf 1}/2^{n} . The off-diagonal entries are small for generic (random) functions θ \theta due to cancellations. This example is only illustrative, however, because ψ \psi is not entirely typical – we have assumed equal probabilities for ψ \psi to be found in each | σ 1 , … , σ N ⟩ |\sigma_{1},\dotsc,\sigma_{N}\rangle state
Cited in the paper.
G. Westfall, private communication
Cited in the paper.
For an overview, including discussion of results on boundary thermalization, see CERN lectures by Takayanagi: http://www2.yukawa.kyoto-u.ac.jp/~tadashi.takayanagi/CERNEE.pdf
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S. Goldstein, T. Hara, H. Tasaki, New J. Phys. 17
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