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PreprintCC BY 4.0arXiv

Quantum spacetime and gravity from the IKKT matrix model: an invitation

Abstract

This is a concise and compact introduction to a framework for spacetime, gravity, and fundamental physics based on the IKKT matrix model, focusing on conceptual and structural aspects. The approach rests on nontrivial vacua or matrix backgrounds, which serve as 3+1-dimensional noncommutative spacetime. We discuss a specific class of backgrounds describing expanding homogeneous and isotropic FLRW spacetime, which provide a solution of the one-loop effective action with finitely many dof per volume. Perturbations of the background give rise to fields propagating on spacetime governed by a weakly-coupled gauge theory, as well as a nonstandard description of (quantum) gravity leading to some IR modifications. Maximal supersymmetry of the model is essential to ensure effective locality.

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BibTeX
@misc{steinacker2026quantum,
  title = {{Quantum spacetime and gravity from the IKKT matrix model: an invitation}},
  author = {Harold C. Steinacker},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.08955},
  eprint = {2609.08955},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.08955},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Quantum spacetime and gravity from the IKKT matrix model: an invitation
AU  - Harold C. Steinacker
PY  - 2026
DA  - 2026/09/08
PB  - arXiv
DO  - 10.48550/arxiv.2609.08955
UR  - https://arxiv.org/abs/2609.08955
AB  - This is a concise and compact introduction to a framework for spacetime, gravity, and fundamental physics based on the IKKT matrix model, focusing on conceptual and structural aspects. The approach rests on nontrivial vacua or matrix backgrounds, which serve as 3+1-dimensional noncommutative spacetime. We discuss a specific class of backgrounds describing expanding homogeneous and isotropic FLRW spacetime, which provide a solution of the one-loop effective action with finitely many dof per volume. Perturbations of the background give rise to fields propagating on spacetime governed by a weakly-coupled gauge theory, as well as a nonstandard description of (quantum) gravity leading to some IR modifications. Maximal supersymmetry of the model is essential to ensure effective locality.
ER  -