Higher spin fluctuations on spinless 4D BTZ black hole
arXiv:1903.01399 · doi:10.1007/JHEP08(2019)171
Abstract
We construct linearized solutions to Vasiliev's four-dimensional higher spin gravity on warped which is an invariant non-rotating BTZ-like black hole with topology. The background can be obtained from by means of identifications along a Killing boost in the region where , or, equivalently, by gluing together two Bañados--Gomberoff--Martinez eternal black holes along their past and future space-like singularities (where 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 and of a commuting Killing boost . The resulting solution space has two main branches in which star commutes and anti-commutes, respectively, to Vasiliev's twisted-central closed two-form . Each branch decomposes further into two subsectors generated from ground states with zero momentum on . We examine the subsector in which anti-commutes to and the ground state is -invariant of which is broken by momenta on and by quasi-normal modes. We show that a set of -invariant modes (with units of momenta) are singularity-free as master fields living on a total bundle space, although the individual Fronsdal fields have membrane-like singularities at . We interpret our findings as an example where Vasiliev's theory completes singular classical Lorentzian geometries into smooth higher spin geometries.
v3: Revised and published on JHEP, with more references, main text 63 pages plus appendices (v2: Clarifications, table and references added, typos corrected)
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- Scalar Electrodynamics and Higgs Mechanism in the Unfolded Dynamics Approach
- All-Order Quartic Couplings in Highly Symmetric D-brane-Anti-D-brane Systems
- Higher-spin initial data in twistor space with complex stargenvalues