2022
DOI: 10.1016/j.physletb.2022.136949
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Chaotic dynamics of a suspended string in a gravitational background with magnetic field

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Cited by 8 publications
(20 citation statements)
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“…As we will later see, the Lyapunov exponent indeed behaves differently in both frames when a magnetic field is present. This should be contrasted with [95], in which calculations are based on the model of [97] where no dilaton field is present and the String and Einstein frame metrics thus coincide. To be more precise, the used metric solves the Einstein equations of motion up to the first non-trivial order in a 1/r expansion, as seminally presented in [98].…”
Section: A Magnetized Emd Gravity Modelmentioning
confidence: 99%
See 1 more Smart Citation
“…As we will later see, the Lyapunov exponent indeed behaves differently in both frames when a magnetic field is present. This should be contrasted with [95], in which calculations are based on the model of [97] where no dilaton field is present and the String and Einstein frame metrics thus coincide. To be more precise, the used metric solves the Einstein equations of motion up to the first non-trivial order in a 1/r expansion, as seminally presented in [98].…”
Section: A Magnetized Emd Gravity Modelmentioning
confidence: 99%
“…In a previous work, the role of magnetic field on the chaotic dynamics of the string has been scrutinised in [95]. In our paper, we build upon their work to continue the study of a magnetic field on the chaotic dynamics of a hanging string in two different frames i.e.…”
Section: Introductionmentioning
confidence: 99%
“…We study the effects of chemical potential, related to a baryon reservoir, and of a magnetic field on the chaotic behaviour of a strongly coupled Q Q pair in a finite temperature background [1,2]. Such systems can be investigated through holographic methods analyzing the dynamics of an open string hanging in the bulk in presence of a black hole (BH).…”
Section: Introductionmentioning
confidence: 99%
“…where µ is the chemical potential and µ c a critical value, can be checked. To test the bounds we consider the Q Q pair in a finite temperature and baryon density background [1], and with a constant and uniform magnetic field at finite temperature [2]. This allows us to test the generalized bound Eq.…”
Section: Introductionmentioning
confidence: 99%
“…The Lyapunov exponent for certain trajectories is bounded by the surface gravity at the horizon of the spherically symmetric static black hole [12]. This relation has been studied further and challenged in several setups [13,14,15,16,17]. In another relevant direction it has been also proposed an interesting correspondence between the operator growth in chaotic theories, the complexity and the radial momenta of the particles falling in the AdS black hole, for example in [18,19,20,21,22].…”
Section: Introductionmentioning
confidence: 99%