Abstract

We derive the universal terms of entanglement entropy for 6d CFTs by applying the holographic and the field theoretical approaches, respectively. Our formulas are conformal invariant and agree with the results of [34,35]. Remarkably, we find that the holographic and the field theoretical results match exactly for the $C^2$ and $Ck^2$ terms. Here $C$ and $k$ denote the Weyl tensor and the extrinsic curvature, respectively. As for the $k^4$ terms, we meet the splitting problem of the conical metrics. The splitting problem in the bulk can be fixed by equations of motion. As for the splitting on the boundary, we assume the general forms and find that there indeed exists suitable splitting which can make the holographic and the field theoretical $k^4$ terms match. Since we have much more equations than the free parameters, the match for $k^4$ terms is non-trivial.

Highlights

  • Holographic entanglement entropyWe briefly review the derivations of holographic entanglement entropy (HEE) for the general higher curvature gravity [10]

  • See [14,15,16,17,18,19] for the study of holographic entanglement entropy and the differential entropy of a holographic hole [20,21,22,23]

  • As we have mentioned in the above sub-section, the splittings of the conical metrics cannot be avoided in order to derive consistent results for the universal terms of EE

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Summary

Holographic entanglement entropy

We briefly review the derivations of holographic entanglement entropy (HEE) for the general higher curvature gravity [10]. As we find, this ansatz yields inconsistent results for the universal terms of EE for 6d CFTs [12], i.e., two gravitational actions with the same holographic Weyl anomaly give different universal terms of EE. To resolve this inconsistency, we proposes the following regularizations. How to split M into M0 and M1 (M denotes T and Q) is the so-called the splitting problem It appears because one cannot distinguish r2 and r2n in the expansions of the conical metric. As we shall show in the sub-section, this is the case at least for Einstein gravity

The splitting problem
Approach based on PBH transformation
Fefferman-Graham expansion
Schwimmer-Theisen approach
Example: higher curvature gravity
Holographic method
Logarithmic terms of EE from a smart-constructed action
F1 and F2
Logarithmic terms of EE from a general action
Field theoretical method
For ds2
Conclusions
A Universal relations from extremal entropy condition
B The conformal invariance of F3
C Weyl tensor
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