Classical space-time geometry in the IKKT matrix model
Harold C. Steinacker

TL;DR
This paper explores how classical 3+1-dimensional space-time geometries can emerge from the IKKT matrix model using covariant quantum spaces, providing a practical method and analyzing the impact of higher-spin contributions.
Contribution
It offers an explicit recipe for reconstructing generic classical geometries within the IKKT matrix model, including the role of fuzzy extra dimensions and higher-spin effects.
Findings
Higher-spin contributions do not significantly alter the physical content in the weak gravity regime.
The framework supports emergent gravity with an induced Einstein-Hilbert action.
Explicit construction methods for classical geometries are provided.
Abstract
We discuss the reconstruction of generic 3+1-dimensional space-time geometries from covariant quantum spaces as backgrounds in the IKKT matrix model. An explicit recipe to realize generic classical geometries is provided. Even though this typically entails some higher-spin contributions, these do not significantly modify the physical content of the model in the weak gravity regime. This justifies the framework for emergent gravity given by the semi-classical matrix model, supplemented by an induced Einstein-Hilbert action which arises in the presence of fuzzy extra dimensions.
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Taxonomy
TopicsNoncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories · Black Holes and Theoretical Physics
