The tachyon at the end of the universe
By John McGreevy, E. Silverstein. 2005
141 citations recorded by the source corpus.
We show that a tachyon condensate phase replaces the spacelike singularity in certain cosmological and black hole spacetimes in string theory. We analyze explicitly a set of examples with flat spatial slices in various dimensions which have a winding tachyon condensate, using worldsheet path integral methods from Liouville theory. In a vacuum with no excitations above the tachyon background in the would-be singular region, we analyze the production of closed strings in the resulting state in the bulk of spacetime. We find a thermal result reminiscent of the Hartle-Hawking state, with tunably small energy density. The amplitudes exhibit a self-consistent truncation of support to the weakly-coupled small-tachyon region of spacetime. We argue that the background is accordingly robust against back reaction, and that the resulting string theory amplitudes are perturbatively finite, indicating a resolution of the singularity and a mechanism to start or end time in string theory. Finally, we discuss the generalization of these methods to examples with positively curved spatial slices.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/461178c24dab3b68c19ab585d90bf0bba5866f16
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Citations in the corpus
- Probe branes, time-dependent couplings and thermalization in AdS/CFT (2010, unknown): “J H E P 0 7 ( 2 0 1 0 ) 0 7 1 theory dual [5–17].”
- AdS bubbles, entropy and closed string tachyons (2006, methodology): “We will also present the dual holographic computation4 [11] in supergravity.”
- A matrix big bang (2005, background): “See, however, the very recent paper [11], which claims that certain space-like singularities are replaced by a tachyon condensate phase within perturbative string theory.”