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arXiv · 2312.10311

Symmetry breaking of $3$-dimensional AdS in holographic semiclassical gravity

Akihiro Ishibashi·Kengo Maeda·Takashi Okamura
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Abstract

We show that $3$-dimensional AdS spacetime can be semiclassically unstable due to strongly interacting quantum field effects. In our previous paper, we have pointed out the possibility of such an instability of AdS$_3$ by inspecting linear perturbations of the (covering space of) static BTZ black hole with AdS${}_4$ gravity dual in the context of holographic semiclassical problems. In the present paper, we further study this issue from thermodynamic viewpoint by constructing asymptotically AdS$_3$ semiclassical solutions and computing free energies of the solutions. We find two asymptotically AdS${}_3$ solutions to the semiclassical Einstein equations with non-vanishing source term: the one whose free energy is smaller than that of the BTZ with vanishing source term and the other whose free energy is smaller than that of the global AdS$_3$ with no horizon (thus manifestly zero-temperature background). The instability found in this paper implies the breakdown of the maximal symmetries of AdS$_3$, and its origin is different from the well-known semiclassical linear instability since our holographic semiclassical Einstein equations in $3$-dimensions do not involve higher order derivative terms.

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Akihiro Ishibashi, Kengo Maeda, Takashi Okamura. 2023-12-16. Symmetry breaking of $3$-dimensional AdS in holographic semiclassical gravity. https://arxiv.org/abs/2312.10311

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