Spatially flat cosmological quantum spacetimes

TL;DR

This paper constructs a broad class of spatially flat quantum cosmological spacetimes within the IKKT matrix model framework, exploring their algebraic structure, higher spin modes, and gauge symmetries in the semi-classical regime.

Contribution

It introduces a large class of spatially flat quantum spacetimes, details their algebraic and semi-classical properties, and discusses gauge transformations and potential integration into the IKKT model.

Findings

Construction of new spatially flat quantum spacetimes

Analysis of their algebraic and semi-classical structures

Introduction of approximate diffeomorphisms and gauge relations

Abstract

We recently described a cosmological quantum spacetime of vanishing spatial curvature, which can be considered as background for the IKKT matrix model, assuming that the resulting gauge theory couples weakly. Building on this example, we construct a large class of spatially flat cosmological quantum spacetimes. We also elaborate on various details of their algebraic and semi-classical structure as well as the higher spin modes present in these models. In particular, we introduce the notion of approximate diffeomorphisms on the cosmological quantum spacetimes that stem from gauge transformations of the underlying matrix model, and investigate how different gauges are related in the semi-classical regime by approximate diffeomorphisms. Finally, we briefly outline how the described quantum spacetimes could be incorporated into the full IKKT model.