Holographic Timelike Entanglement and Subregion Complexity in Localized AdS3*S3*T4 Black Holes
- URL: http://arxiv.org/abs/2607.11641v1
- Date: Mon, 13 Jul 2026 14:57:41 GMT
- Title: Holographic Timelike Entanglement and Subregion Complexity in Localized AdS3*S3*T4 Black Holes
- Abstract summary: We study timelike entanglement entropy and timelike subregion complexity in localized black holes with AdS3*S3*T4 geometry.<n>We show that timelike Lorentzian observables probe localized-geometry effects that are absent in BTZ and in the leading large-$r$ description.
- Score: 3.4396122938297595
- License: http://creativecommons.org/licenses/by/4.0/
- Abstract: We study timelike entanglement entropy and timelike subregion complexity in localized black holes with asymptotic AdS3*S3*T4 geometry, focusing on the black-pole solution. Unlike the BTZ solution, the black pole exhibits a nontrivial dependence on the internal sphere through the functions $K_y(r,θ)$ and $G(r,θ)$. Both observables are constructed from spacelike and timelike Lorentzian branches, but they probe the geometry in different ways: timelike entanglement yields a complex lifted area, while timelike complexity gives a real, finite renormalized volume. We employ a localized timelike prescription in which the branch profile is built at an angular label $θ_0$ and subsequently lifted over the physical internal angle $θ$. In the large-$r$ regime, the leading angular dependence drops out, recovering the expected short-interval behaviour. In the exact black-pole geometry, the temporal families become non-monotonic, making a fixed-boundary-interval selection essential. As the boundary interval increases, the selected branches move inward and become sensitive to the localized cap-horizon transition region. These results demonstrate that timelike Lorentzian observables probe localized-geometry effects that are absent in BTZ and in the leading large-$r$ description.
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