The emergence of expanding space-time in a novel large-$N$ limit of the Lorentzian type IIB matrix model
Mitsuaki Hirasawa, Konstantinos N. Anagnostopoulos, Takehiro Azuma,, Kohta Hatakeyama, Jun Nishimura, Stratos Kovalkov Papadoudis, Asato Tsuchiya

TL;DR
This paper introduces a modified Lorentzian type IIB matrix model with a mass term and demonstrates through complex Langevin simulations that an expanding Lorentzian space-time emerges in the large-$N$ limit, offering insights into non-perturbative superstring theory.
Contribution
It proposes a novel large-$N$ limit with a vanishing mass term coefficient that results in emergent expanding Lorentzian space-time, addressing previous issues with Euclidean space-time appearance.
Findings
Emergence of expanding Lorentzian space-time in the modified model
Use of complex Langevin simulations to handle the sign problem
The model provides a promising non-perturbative approach to superstring theory
Abstract
The Lorentzian type IIB matrix model is a promising candidate for a non-perturbative formulation of superstring theory. However, it was found recently that a Euclidean space-time appears in the conventional large- limit. In this work, we add a Lorentz invariant mass term to the original model and consider a limit, in which the coefficient of the mass term vanishes at large . By performing complex Langevin simulations to overcome the sign problem, we observe the emergence of expanding space-time with the Lorentzian signature.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories
