Abstract
Abstract
We argue that the Schwarzschild-de Sitter black hole entropy formula does not imply that the entanglement spectrum of the vacuum density matrix of de Sitter space is flat. Specifically, we show that the expectation value of a random projection operator of dimension d ≫ 1, on a Hilbert space of dimension D ≫ d and in a density matrix ρ = e–K with strictly positive spectrum, is $$ \frac{d}{D}\left(1+o\left(\frac{1}{\sqrt{d}}\right)\right) $$
d
D
1
+
o
1
d
, independent of the spectrum of the density matrix. In addition, for a suitable class of spectra the asymptotic estimates Tr (ρK) ~ ln D – o(1) and Tr [ρ(K – 〈K〉)2] = a〈K〉 are compatible for any order one constant a. We discuss a simple family of matrix models and projections that can replicate such modular Hamiltonians and the SdS entropy formula.
Publisher
Springer Science and Business Media LLC
Subject
Nuclear and High Energy Physics
Cited by
4 articles.
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