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Tuesday, 27 March 2007, 14:00 in SSB7109
Prof. Shinji Mukohyama (University of Tokyo)
Cosmology with warped flux compactification
Inflation in the early universe and the accelerated expansion of the late-time universe are two major quasi de Sitter phases in the history of our universe. Thus, any candidates for the unified theory of nature must allow 4-dimensional de Sitter or/and quasi de Sitter solutions. It is only recent that a consistent 4-dimensional de Sitter solution was found in string theory by using warped flux compactification and branes. In this talk I would like to discuss cosmological applications of models of warped flux compactification.
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Modified by Andrei Frolov <frolov@sfu.ca> on 2023-11-01