Abstract

We analytically study phase transitions of holographic charged Rényi entropies in two gravitational systems dual to the mathcal{N} = 4 super-Yang-Mills theory at finite density and zero temperature. The first system is the Reissner-Nordström-AdS5 black hole, which has finite entropy at zero temperature. The second system is a charged dilatonic black hole in AdS5, which has zero entropy at zero temperature. Hyperbolic black holes are employed to calculate the Rényi entropies with the entangling surface being a sphere. We perturb each system by a charged scalar field, and look for a zero mode signaling the instability of the extremal hyperbolic black hole. Zero modes as well as the leading order of the full retarded Green’s function are analytically solved for both systems, in contrast to previous studies in which only the IR (near horizon) instability was analytically treated.

Highlights

  • We perturb each system by a charged scalar field, and look for a zero mode signaling the instability of the extremal hyperbolic black hole

  • We review the relation between Rényi entropies and hyperbolic black holes very briefly, but it is sufficient for the purpose of this paper

  • We have analytically solved the zero modes triggering the instability in two systems of charged hyperbolic black holes at zero temperature

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Summary

From Rényi entropies to hyperbolic black holes

We review the relation between Rényi entropies and hyperbolic black holes very briefly, but it is sufficient for the purpose of this paper. Phase transitions of Rényi entropies with the entangling surface being a sphere are studied in terms of hyperbolic black holes. The reduced density matrix for the subsystem A is ρA = TrBρ. The charged Rényi entropy is defined by [6]. Where μ is the entanglement chemical potential, and QA measures the amount of charge in the subsystem A, and NA(μ) ≡ Tr[ρAeμQA] is a normalization factor. Suppose we want to calculate the Rényi entropies of a CFT with a gravity dual, and the entangling surface is a sphere of radius R. The Rényi entropy is related to the free energy of a hyperbolic black hole: Sn(μ).

Hyperbolic RN-AdS5 black hole
Matching the IR and UV data
Two types of instabilities
Adding a double-trace deformation
Hyperbolic 2-charge black hole in AdS5
Discussion
A Fermi surfaces from the Gubser-Rocha-axions model
B Mathematical notes
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