# Higher spin fluctuations on spinless 4D BTZ black hole

**Authors:** Rodrigo Aros, Carlo Iazeolla, Per Sundell, Yihao Yin

arXiv: 1903.01399 · 2019-09-04

## TL;DR

This paper constructs and analyzes linearized solutions in four-dimensional higher spin gravity on a BTZ-like black hole background, revealing how higher spin fields can smooth out classical singularities.

## Contribution

It introduces new solutions in Vasiliev's higher spin gravity on warped AdS3 backgrounds, demonstrating how higher spin fields can resolve classical singularities.

## Key findings

- Higher spin fluctuations are constructed on a BTZ-like black hole background.
- Certain higher spin modes are shown to be singularity-free as master fields.
- Higher spin fields can smooth out classical singularities in Lorentzian geometries.

## Abstract

We construct linearized solutions to Vasiliev's four-dimensional higher spin gravity on warped $AdS_3 \times_\xi S^1$ which is an $Sp(2)\times U(1)$ invariant non-rotating BTZ-like black hole with $\mathbb{R}^2\times T^2$ topology. The background can be obtained from $AdS_4$ by means of identifications along a Killing boost $K$ in the region where $\xi^2\equiv K^2\geqslant 0$, or, equivalently, by gluing together two Ba\~nados--Gomberoff--Martinez eternal black holes along their past and future space-like singularities (where $\xi$ vanishes) as to create a periodic (non-Killing) time. The fluctuations are constructed from gauge functions and initial data obtained by quantizing inverted harmonic oscillators providing an oscillator realization of $K$ and of a commuting Killing boost $\widetilde K$. The resulting solution space has two main branches in which $K$ star commutes and anti-commutes, respectively, to Vasiliev's twisted-central closed two-form $J$. Each branch decomposes further into two subsectors generated from ground states with zero momentum on $S^1$. We examine the subsector in which $K$ anti-commutes to $J$ and the ground state is $U(1)_K\times U(1)_{\widetilde K}$-invariant of which $U(1)_K$ is broken by momenta on $S^1$ and $U(1)_{\widetilde K}$ by quasi-normal modes. We show that a set of $U(1)_{\widetilde K}$-invariant modes (with $n$ units of $S^1$ momenta) are singularity-free as master fields living on a total bundle space, although the individual Fronsdal fields have membrane-like singularities at $\widetilde K^2=1$. We interpret our findings as an example where Vasiliev's theory completes singular classical Lorentzian geometries into smooth higher spin geometries.

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## Figures

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## References

94 references — full list in the complete paper: https://tomesphere.com/paper/1903.01399/full.md

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Source: https://tomesphere.com/paper/1903.01399