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Geodesic Stability for Kehagias-Sfetsos Black Hole in Hořava-Lifshitz Gravity via Lyapunov Exponents

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Abstract

By computing the Lyapunov exponent, which is the inverse of the instability time scale associated with this geodesic motion we show that for a general Kehagias-Sfetsos (KS) solution, there is two region of space which in both of them the equatorial timelike geodesics are stable via Lyapunov measure of stability.

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Authors and Affiliations

  1. Department of Science of Bijar, University of Kurdistan, Bijar, Iran

    M. R. Setare

  2. Physics Department, Faculty of Science, Tarbiat Moalem University, Tehran, Iran

    D. Momeni

Authors
  1. M. R. Setare
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  2. D. Momeni
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Correspondence to D. Momeni.

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Setare, M.R., Momeni, D. Geodesic Stability for Kehagias-Sfetsos Black Hole in Hořava-Lifshitz Gravity via Lyapunov Exponents. Int J Theor Phys 50, 106–113 (2011). https://doi.org/10.1007/s10773-010-0498-8

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  • DOI: https://doi.org/10.1007/s10773-010-0498-8

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