Spherically symmetric solutions of higher-spin gravity in the IKKT matrix model
arXiv:2112.08204 · doi:10.1016/j.nuclphysb.2022.115843
Abstract
We present a systematic study of spherically symmetric vacuum solutions of the IKKT matrix model, within the framework of semi-classical covariant quantum geometries. All asymptotically flat solutions of the equations of motion of the frame are found explicitly. They reproduce the linearized Schwarzschild geometry for large but deviate from it at the non-linear level, and include contributions from dilaton and axion. They are pertinent to the pre-gravity theory arising on classical brane solutions within the classical matrix model, before taking into account the Einstein-Hilbert term induced by quantum effects. We also address the problem of reconstructing matrix configurations corresponding to some given frame, and show that this problem can always be solved at the geometrical level of the underlying higher spin theory, ignoring possible higher spin modes.
35 pages, 21 figures
References in corpus (6)
- Complex Langevin analysis of the space-time structure in the Lorentzian type IIB matrix model
- Gravity as a Quantum Effect on Quantum Space-Time
- 4D Higher Spin Black Holes with Nonlinear Scalar Fluctuations
- Field Equations of Massless Fields in the New Interpretation of the Matrix Model
- Factorization of the Effective Action in the IIB Matrix Model
- Curved Superspaces and Local Supersymmetry in Supermatrix Model