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Brane tachyon dynamics
Authors:Hongsheng Zhang  Xin-Zhou Li  Hyerim Noh
Affiliation:1. Shanghai United Center for Astrophysics (SUCA), Shanghai Normal University, 100 Guilin Road, Shanghai 200234, PR China;2. Korea Astronomy and Space Science Institute, Daejeon 305-348, Republic of Korea;3. Department of Astronomy, Beijing Normal University, Beijing 100875, PR China
Abstract:The dynamics of a tachyon attached to a Dvali, Gabadadze and Porrati (DGP) brane is investigated. Exponential potential and inverse power law potential are explored, respectively. The quasi-attractor behavior, for which the universe will eventually go into a phase similar to the slow-roll inflation, is discovered in both cases of exponential potential and inverse power law potential. The equation of state (EOS) of the virtual dark energy for a single scalar can cross the phantom divide in the branch θ=−1θ=1 for both potentials, while the EOS of the virtual dark energy for a single scalar cannot cross this divide in the branch θ=1θ=1.
Keywords:Brane   Tachyon   Dark energy
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