The emergence of (3+1)-dimensional expanding spacetime from complex Langevin simulations of the Lorentzian type IIB matrix model with deformations

Abstract The Lorentzian type IIB matrix model is a promising candidate for a nonperturbative formulation of superstring theory. In this model, the eigenvalue distribution of the N × N bosonic matrices Aμ (μ = 0, …, 9) represents an emergent spacetime, which is determined by the dynamics of the model in the large-N limit. Here we perform numerical simulations of the model overcoming the sign problem by the complex Langevin method with the matrix size N up to 128. In order to avoid the singular drift problem due to the Pfaffian, which appears after integrating out the fermionic matrices, we deform the model in a manner inspired by the supersymmetric deformation, which is used to define the “polarized type IIB matrix model” in the Euclidean case. We find that the deformed model exhibits a phase in which (3+1)-dimensional expanding spacetime emerges with both space and time being smooth and real.

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Publication Details

Journal
Progress of Theoretical and Experimental Physics
Published
2026-08-14
DOI
https://doi.org/10.1093/ptep/ptag159
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00

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article

The emergence of (3+1)-dimensional expanding spacetime from complex Langevin simulations of the Lorentzian type IIB matrix model with deformations

Takehiro Azuma, Mitsuaki Hirasawa, Konstantinos N.Anagnostopoulos, Asato Tsuchiya et al.
Progress of Theoretical and Experimental Physics
Black Holes and Theoretical Physics
article

The emergence of (3+1)-dimensional expanding spacetime from complex Langevin simulations of the Lorentzian type IIB matrix model with deformations

Takehiro Azuma, Mitsuaki Hirasawa, Konstantinos N.Anagnostopoulos, Asato Tsuchiya, Jun Nishimura, Stratos Papadoudis
article en

Abstract

Abstract The Lorentzian type IIB matrix model is a promising candidate for a nonperturbative formulation of superstring theory. In this model, the eigenvalue distribution of the N × N bosonic matrices Aμ (μ = 0, …, 9) represents an emergent spacetime, which is determined by the dynamics of the model in the large-N limit. Here we perform numerical simulations of the model overcoming the sign problem by the complex Langevin method with the matrix size N up to 128. In order to avoid the singular drift problem due to the Pfaffian, which appears after integrating out the fermionic matrices, we deform the model in a manner inspired by the supersymmetric deformation, which is used to define the “polarized type IIB matrix model” in the Euclidean case. We find that the deformed model exhibits a phase in which (3+1)-dimensional expanding spacetime emerges with both space and time being smooth and real.

Progress of Theoretical and Experimental Physics
Setsunan University (JP), Shizuoka University (JP), High Energy Accelerator Research Organization (JP), National Technical University of Athens (GR), The Graduate University for Advanced Studies, SOKENDAI (JP), Istituto Nazionale di Fisica Nucleare, Sezione di Milano Bicocca (IT), University of Milano-Bicocca (IT)
Joint Institute for Computational Fundamental Science, Ministry of Education, Culture, Sports, Science and Technology, Hokkaido University, Yukawa Institute for Theoretical Physics, Kyoto University, Japan Society for the Promotion of Science, RIKEN
Sustainable cities and communities
Openalex Percentile: Top 60%
Black Holes and Theoretical Physics
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