General Relativity in IIB matrix model

A bstract The matrix models are non-perturbative formulations of string theory, from which many believe that spacetime arises. The matrix fluctuations around the spacetime thus created should represent both matter and gravitational fields. In this paper, we discuss how the gravitational field emerges from the IIB matrix model. In particular, we consider how diffeomorphism invariance arises and how unitarity is guaranteed in this theory. Specifically, we consider matrices as bilocal fields and discuss how the Lorentz-invariant vacuum and low-energy excitations around it can be expressed. We then discuss how the conditions for the theory to be unitary can be written in terms of bilocal fields. We argue that in the low-energy limit, the bilocal fields are reduced to local fields consisting of a finite number of massless fields and an infinite number of massive fields, satisfying unitarity.

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Publication Details

Journal
Journal of High Energy Physics
Published
2026-02-05
DOI
https://doi.org/10.1007/jhep02(2026)070
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00

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article

General Relativity in IIB matrix model

Harold Steinacker, Hikaru KAWAI, P. T. Ho
Journal of High Energy Physics
Black Holes and Theoretical Physics
article

General Relativity in IIB matrix model

Harold Steinacker, Hikaru KAWAI, P. T. Ho
article en

Abstract

A bstract The matrix models are non-perturbative formulations of string theory, from which many believe that spacetime arises. The matrix fluctuations around the spacetime thus created should represent both matter and gravitational fields. In this paper, we discuss how the gravitational field emerges from the IIB matrix model. In particular, we consider how diffeomorphism invariance arises and how unitarity is guaranteed in this theory. Specifically, we consider matrices as bilocal fields and discuss how the Lorentz-invariant vacuum and low-energy excitations around it can be expressed. We then discuss how the conditions for the theory to be unitary can be written in terms of bilocal fields. We argue that in the low-energy limit, the bilocal fields are reduced to local fields consisting of a finite number of massless fields and an infinite number of massive fields, satisfying unitarity.

Journal of High Energy PhysicsVol. 2026(2)
University of Vienna (AT), National Taiwan University (TW), National Center for Theoretical Sciences (TW), Osaka Metropolitan University (JP)
Austrian Science Fund, National Taiwan University, National Science and Technology Council, Japan Society for the Promotion of Science
Affordable and clean energy
Openalex Percentile: Top 62%
Black Holes and Theoretical Physics
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