Gravitational Radiation of Rolling Tachyon
arXiv:hep-th/0209222 · doi:10.1088/1126-6708/2002/11/050
Abstract
In this paper we compute the radiation of the massless closed string states due to the non-vanishing coupling to the rolling open string tachyon with co-dimensions larger than 2, and discuss the effect of back reaction to the motion of the rolling tachyon. We find that for small string coupling, the tachyonic matter remains in the late time, but it will completely evaporate away over a short time of few string scales if the string coupling is huge. Comment on the implication of our results to the g-theorem of boundary conformal field theory is given.
17 pages, 1 figure; v2 correct typos, add references & acknowledgement; v3 final to appear on JHEP with minor comment and references added
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- Classical and Quantum D-branes in 2D String Theory
- Closed Strings as Imaginary D-branes
- Reheating the Universe after String Theory Inflation
- Open and Closed Strings from Unstable D-branes
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- Inflationary Attractor from Tachyonic Matter
- Warped Reheating in Multi-Throat Brane Inflation
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- Electromagnetic String Fluid in Rolling Tachyon
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- Time Evolution via S-branes
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- Twisting S-branes
- Comments on Half S-Branes
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- Predictions of Dynamically Emerging Brane Inflation Models
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