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Quantum chaos, thermalization, and entanglement generation in real-time simulations of the Banks-Fischler-Shenker-Susskind matrix model

Quantum chaos, thermalization, and entanglement generation in real-time simulations of the Banks-Fischler-Shenker-Susskind matrix model
Quantum chaos, thermalization, and entanglement generation in real-time simulations of the Banks-Fischler-Shenker-Susskind matrix model

We study numerically the onset of chaos and thermalization in the Banks-Fischler-Shenker-Susskind (BFSS) matrix model with and without fermions, considering Lyapunov exponents, entanglement generation, and quasinormal ringing. We approximate the real-time dynamics in terms of the most general Gaussian density matrices with parameters which obey self-consistent equations of motion, thus extending the applicability of real-time simulations beyond the classical limit. Initial values of these Gaussian density matrices are optimized to be as close as possible to the thermal equilibrium state of the system. Thus attempting to bridge between the low-energy regime with a calculable holographic description and the classical regime at high energies, we find that quantum corrections to classical dynamics tend to decrease the Lyapunov exponents, which is essential for consistency with the Maldacena-Shenker-Stanford bound at low temperatures. The entanglement entropy is found to exhibit an expected "scrambling" behavior - rapid initial growth followed by saturation. At least at high temperatures the entanglement saturation time appears to be governed by classical Lyapunov exponents. Decay of quasinormal modes is found to be characterized by the shortest timescale of all. We also find that while the bosonic matrix model becomes nonchaotic in the low-temperature regime, for the full BFSS model with fermions the leading Lyapunov exponent, entanglement saturation time, and decay rate of quasinormal modes all remain finite and nonzero down to the lowest temperatures.

2470-0010
Buividovich, P. V.
4025fae9-7881-4c25-8dbc-c1fae911d464
Hanada, M.
a3ad894b-9d7d-4954-923e-e177e5c7f54a
Schäfer, A.
38a20c26-b85f-49f4-93cb-011c99a6cf42
Buividovich, P. V.
4025fae9-7881-4c25-8dbc-c1fae911d464
Hanada, M.
a3ad894b-9d7d-4954-923e-e177e5c7f54a
Schäfer, A.
38a20c26-b85f-49f4-93cb-011c99a6cf42

Buividovich, P. V., Hanada, M. and Schäfer, A. (2019) Quantum chaos, thermalization, and entanglement generation in real-time simulations of the Banks-Fischler-Shenker-Susskind matrix model. Physical Review D, 99 (4), [046011]. (doi:10.1103/PhysRevD.99.046011).

Record type: Article

Abstract

We study numerically the onset of chaos and thermalization in the Banks-Fischler-Shenker-Susskind (BFSS) matrix model with and without fermions, considering Lyapunov exponents, entanglement generation, and quasinormal ringing. We approximate the real-time dynamics in terms of the most general Gaussian density matrices with parameters which obey self-consistent equations of motion, thus extending the applicability of real-time simulations beyond the classical limit. Initial values of these Gaussian density matrices are optimized to be as close as possible to the thermal equilibrium state of the system. Thus attempting to bridge between the low-energy regime with a calculable holographic description and the classical regime at high energies, we find that quantum corrections to classical dynamics tend to decrease the Lyapunov exponents, which is essential for consistency with the Maldacena-Shenker-Stanford bound at low temperatures. The entanglement entropy is found to exhibit an expected "scrambling" behavior - rapid initial growth followed by saturation. At least at high temperatures the entanglement saturation time appears to be governed by classical Lyapunov exponents. Decay of quasinormal modes is found to be characterized by the shortest timescale of all. We also find that while the bosonic matrix model becomes nonchaotic in the low-temperature regime, for the full BFSS model with fermions the leading Lyapunov exponent, entanglement saturation time, and decay rate of quasinormal modes all remain finite and nonzero down to the lowest temperatures.

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PhysRevD.99.046011 - Version of Record
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Accepted/In Press date: 15 February 2019
e-pub ahead of print date: 19 February 2019

Identifiers

Local EPrints ID: 429017
URI: http://eprints.soton.ac.uk/id/eprint/429017
ISSN: 2470-0010
PURE UUID: 78707839-cc53-4aa7-89a3-0d5637d65112

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Date deposited: 19 Mar 2019 17:30
Last modified: 17 Mar 2024 12:21

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Contributors

Author: P. V. Buividovich
Author: M. Hanada
Author: A. Schäfer

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