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      AdS Bubbles, Entropy and Closed String Tachyons

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          Abstract

          We study the conjectured connection between AdS bubbles (AdS solitons) and closed string tachyon condensations. We confirm that the entanglement entropy, which measures the degree of freedom, decreases under the tachyon condensation. The entropies in supergravity and free Yang-Mills agree with each other remarkably. Next we consider the tachyon condensation on the AdS twisted circle and argue that its endpoint is given by the twisted AdS bubble, defined by the double Wick rotation of rotating black 3-brane solutions. We calculated the Casimir energy and entropy and checked the agreements between the gauge and gravity results. Finally we show an infinite boost of a null linear dilaton theory with a tachyon wall (or bubble), leads to a solvable time-dependent background with a bulk tachyon condensation. This is the simplest example of spacetimes with null boundaries in string theory.

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          Quantum source of entropy for black holes

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            The Inside Story: Quasilocal Tachyons and Black Holes

            We analyze the fate of excitations in regions of closed string tachyon condensate, a question crucial for understanding unitarity in a class of black holes in string theory. First we introduce a simple new example of {\it quasilocal} tachyon condensation in a globally stable AdS/CFT background, and review tachyons' appearance in black hole physics. Then we calculate forces on particles and fields in a tachyon phase using a field theoretic model with spatially localized exponentially growing time dependent masses. This model reveals two features, both supporting unitary evolution in the bulk of spacetime. First, the growing energy of fields sourced by sets of (real and virtual) particles in the tachyon phase yields outward forces on them, leaving behind only combinations which do not source any fields. Secondly, requiring the consistency of perturbative string theory imposes cancellation of a BRST anomaly, which also yields a restricted set of states. Each of these effects supports the notion of a black hole final state arising from string-theoretic dynamics replacing the black hole singularity.
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              Author and article information

              Journal
              2006-11-02
              2006-11-11
              Article
              10.1088/1126-6708/2007/01/090
              hep-th/0611035
              34cfaf11-9a63-44fb-bc1d-70c6c885d1c6
              History
              Custom metadata
              KUNS-2050
              JHEP 0701:090,2007
              45 pages, 6 figures, harvmac, eq.(2.16) corrected, references added
              hep-th gr-qc

              General relativity & Quantum cosmology,High energy & Particle physics
              General relativity & Quantum cosmology, High energy & Particle physics

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