Abstract

By fast Lyapunov indicator (FLI), we study the chaotic dynamics of closed string around charged black brane with hyperscaling violation (HV). The Hawking temperature, Lifshitz dynamical exponent and HV exponent together affect the chaotic dynamics of this system. The temperature plays the role of driving the closed string to escape to infinity. There is a threshold value z∗ = 2, below which the string is captured by the black brane no matter where the string is placed at the beginning. However, when z > 2, the string escapes to infinity if it is placed near the black brane at the beginning, but if the initial position of string is far away from the black brane, it oscillates around the black brane till eternity, which is a quasi-periodic motion. HV exponent plays the role of driving the string falling into the black brane. With the increase of HV exponent θ, the falling velocity becomes faster. We find that when we heat the system with large HV exponent, the chaotic system does not essentially changes. It indicates that the HV exponent plays a very important role in determining the state of the chaotic system. Also we study the effect from the winding number of the string. The study indicates that the chaotic dynamics of the string is insensitive to the winding number.

Highlights

  • Introduction of numerical methodA reliable numerical technique is very essential to solve the EOMs of a closed string

  • By fast Lyapunov indicator (FLI), we study the chaotic dynamics of closed string around charged black brane with hyperscaling violation (HV)

  • When z > 2, the string escapes to infinity if it is placed near the black brane at the beginning, but if the initial position of string is far away from the black brane, it oscillates around the black brane till eternity, which is a quasi-periodic motion

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Summary

The role of the temperature

We find that even when the closed string is at the position being close to the black brane (here, we take r0 = 10), the string escapes to infinity rapidly as the temperature is further increased (see the figure 3). We plot the FLIs for r0 = 10 (right plot in figure 4), which clearly exhibits the two behaviors of closed string: escaping to infinity or being captured by the black brane depending on the temperature of the black brane. The escaping or falling velocity is rapid for r0 = 10 These observations are consistent with that in the time evolution and the phase space.

The effect from Lifshitz dynamical exponent
The effect from HV exponent
The effect of the winding number
Conclusions and discussions
Full Text
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