arXiv · hep-th/0303087
Closed String Tachyon Condensation and Worldsheet Inflation
Abstract
Closed string tachyon condensation in spacetime generates potentials on the worldsheet that model two-dimensional inflationary cosmology. These models illustrate and elucidate a variety of aspects of inflation, in particular the generation of quantum fluctuations and their back-reaction on geometry. We exhibit a class of Liouville gravity models coupled to matter that can exhibit, for example: (a) pure de Sitter gravity; (b) slow-roll inflation; (c) topological inflation; and (d) graceful exit into an FRW phase. The models also provide a quantitative testing ground for ideas about the origin of inflation, such as the various `no-boundary/tunnelling' proposals, and the `eternal/chaotic' inflationary scenario. We suggest an alternative mechanism for quantum creation of cosmological spacetimes which, in the context of the model, provides a natural explanation for why the typical FRW cosmology at large scales underwent a period of inflation at small scale.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Bruno Carneiro da Cunha, Emil J. Martinec. 2003-04-14. Closed String Tachyon Condensation and Worldsheet Inflation. https://doi.org/10.1103/physrevd.68.063502
Cite the original work for its findings. Save a collection to share your selection of sources.