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We study the Lorentzian version of the type IIB matrix model as a nonperturbative formulation of superstring theory in (9+1)-dimensions. Monte Carlo results show that not only space but also time emerges dynamically in this model.…

High Energy Physics - Theory · Physics 2015-06-11 Jun Nishimura

Recently we have shown by Monte Carlo simulation that expanding (3+1)-dimensional universe appears dynamically from a Lorentzian matrix model for type IIB superstring theory in (9+1)-dimensions. The mechanism for the spontaneous breaking of…

High Energy Physics - Theory · Physics 2015-05-30 Sang-Woo Kim , Jun Nishimura , Asato Tsuchiya

The type IIB matrix model is a conjectured nonperturbative formulation of superstring theory. Recent studies on the Lorentzian version of the model have shown that only three out of nine spatial directions start to expand after some…

High Energy Physics - Lattice · Physics 2016-11-30 Yuta Ito , Jun Nishimura , Asato Tsuchiya

The emergence of (3+1)-dimensional expanding space-time in the Lorentzian type IIB matrix model is an intriguing phenomenon which was observed in Monte Carlo studies of this model. In particular, this may be taken as a support to the…

High Energy Physics - Theory · Physics 2019-10-17 Toshihiro Aoki , Mitsuaki Hirasawa , Yuta Ito , Jun Nishimura , Asato Tsuchiya

Recently we have studied the Lorentzian version of the IIB matrix model as a nonperturbative formulation of superstring theory. By Monte Carlo simulation, we have shown that the notion of time ---as well as space---emerges dynamically from…

High Energy Physics - Theory · Physics 2015-06-11 Sang-Woo Kim , Jun Nishimura , Asato Tsuchiya

The type IIB matrix model is one of the most promising candidates for a nonperturbative formulation of superstring theory. In particular, its Lorentzian version was shown to exhibit an interesting real-time dynamics such as the spontaneous…

High Energy Physics - Theory · Physics 2017-04-26 Yuta Ito , Jun Nishimura , Asato Tsuchiya

The type IIB matrix model is a promising candidate for a nonperturbative formulation of superstring theory. In the Lorentzian version, in particular, the emergence of (3+1)D expanding space-time was observed by Monte Carlo studies of this…

High Energy Physics - Lattice · Physics 2020-06-02 Jun Nishimura

Recent studies on the Lorentzian version of the type IIB matrix model show that (3+1)D expanding universe emerges dynamically from (9+1)D space-time predicted by superstring theory. Here we study a bosonic matrix model obtained by omitting…

High Energy Physics - Theory · Physics 2016-01-20 Yuta Ito , Jun Nishimura , Asato Tsuchiya

We review recent developments in the type IIB matrix model, which was conjectured to be a nonperturbative formulation of superstring theory. In the first part we review the recent results for the Euclidean model, which suggest that SO(10)…

High Energy Physics - Theory · Physics 2016-01-20 Jun Nishimura

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 $N\times N$ bosonic matrices $A_\mu$ $(\mu = 0 , \ldots , 9)$…

The type IIB matrix model is a conjectured nonperturbative formulation of superstring theory. Recently the Lorentzian version of the model has been studied by Monte Carlo simulation, and it has been shown that only three out of nine spatial…

High Energy Physics - Lattice · Physics 2013-11-25 Yuta Ito , Sang-Woo Kim , Jun Nishimura , Asato Tsuchiya

Recently we have shown that (3+1)-dimensional expanding universe appears dynamically and uniquely from the Lorentzian version of the IIB matrix model, which is considered as a nonperturbative formulation of superstring theory. Similarly, it…

High Energy Physics - Theory · Physics 2016-06-21 Jun Nishimura , Asato Tsuchiya

The type IIB matrix model is a promising candidate for a nonperturbative formulation of superstring theory. As such, it is expected to explain the origin of space--time and matter at the same time. This has been partially demonstrated by…

High Energy Physics - Theory · Physics 2022-02-01 Kohta Hatakeyama , Akira Matsumoto , Jun Nishimura , Asato Tsuchiya , Atis Yosprakob

The Lorentzian type IIB matrix model is a promising candidate for a non-perturbative formulation of superstring theory. In previous studies, Monte Carlo calculations provided interesting results indicating the spontaneous breaking of SO(9)…

We propose a new method for studying the early universe in the Lorentzian version of the IIB matrix model, which is considered to be a nonperturbative formulation of superstring theory. This method is based on the idea of renormalization…

High Energy Physics - Theory · Physics 2016-06-21 Yuta Ito , Sang-Woo Kim , Yuki Koizuka , Jun Nishimura , Asato Tsuchiya

We present evidence that recent numerical results from the reduced classical equations of the Lorentzian IIB matrix model can be interpreted as corresponding to the emergence of an expanding universe. In addition, we propose an effective…

General Relativity and Quantum Cosmology · Physics 2020-10-27 F. R. Klinkhamer

The IKKT matrix model (or the type IIB matrix model) is known as a promising candidate for a nonperturbative formulation of superstring theory in ten dimensions. As a most attractive feature, the model admits the emergence of…

High Energy Physics - Theory · Physics 2022-05-11 Jun Nishimura

The Lorentzian type IIB matrix model is a promising candidate for a nonperturbative formulation of superstring theory. Recently we performed complex Langevin simulations by adding a Lorentz invariant mass term as an IR regulator and found a…

The Lorentzian type IIB matrix model is a promising candidate for a non-perturbative formulation of superstring theory. However, it was recently found that a Euclidean space-time appears in the conventional large-$N$ limit. In this work, we…

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-$N$ limit. In this work, we…

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