Covariant cosmological quantum space-time, higher-spin and gravity in the IKKT matrix model
From MaRDI portal
Publication:2317713
DOI10.1007/JHEP07(2019)010zbMath1418.83019arXiv1901.03522WikidataQ125748356 ScholiaQ125748356MaRDI QIDQ2317713
Harold C. Steinacker, Marcus Sperling
Publication date: 12 August 2019
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1901.03522
Two-dimensional field theories, conformal field theories, etc. in quantum mechanics (81T40) Quantization of the gravitational field (83C45) Space-time singularities, cosmic censorship, etc. (83C75) Methods of noncommutative geometry in general relativity (83C65) Astrophysical cosmology (85A40)
Related Items
Gravity as a quantum effect on quantum space-time ⋮ Cosmic time evolution and propagator from a Yang–Mills matrix model ⋮ Spherically symmetric solutions of higher-spin gravity in the IKKT matrix model ⋮ One-loop effective action of the IKKT model for cosmological backgrounds ⋮ Spinorial higher-spin gauge theory from IKKT model in Euclidean and Minkowski signatures ⋮ A twistorial description of the IKKT-matrix model ⋮ Infinite distances in multicritical CFTs and higher-spin holography ⋮ One-loop effective action and emergent gravity on quantum spaces in the IKKT matrix model ⋮ The fuzzy BTZ ⋮ Four-dimensional gravity on a covariant noncommutative space ⋮ Scalar modes and the linearized Schwarzschild solution on a quantized FLRW space-time in Yang–Mills matrix models ⋮ On the quantum structure of space-time, gravity, and higher spin in matrix models ⋮ Exploring the gravity sector of emergent higher-spin gravity: effective action and a solution ⋮ Higher-spin gravity and torsion on quantized space-time in matrix models ⋮ Complex Langevin analysis of the spontaneous breaking of 10D rotational symmetry in the Euclidean IKKT matrix model ⋮ $Sp(4; \mathbb{R})$ squeezing for Bloch four-hyperboloid via the non-compact Hopf map ⋮ Quantum (matrix) geometry and quasi-coherent states
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