Brane Inflation : String Theory viewed from the Cosmos
S.-H. Henry Tye

TL;DR
Brane inflation, a string theory-based early universe model, predicts observable signatures like cosmic strings and non-Gaussianities, with current data constraining its parameters and offering potential validation of string theory.
Contribution
This paper discusses the naturalness, robustness, and cosmological predictions of brane inflation within string theory, highlighting potential observable signatures and current constraints.
Findings
Potential detection of cosmic superstrings via gravitational waves.
Stringy features like non-Gaussianity and tensor modes could be observed.
Cosmological data constrains brane inflation parameters.
Abstract
Brane inflation is a specific realization of the inflationary universe scenario in the early universe within the brane world framework in string theory. The naturalness and robustness of this realistic scenario is explained. Its predictions on the cosmological observables in the cosmic microwave background radiation, especially possible distinct stringy features, such as large non-Gaussianity or large tensor mode that deviates from that predicted in the slow roll scenario, are discussed. Stringy KK modes as hidden dark matter is also a possibility. Another generic consequence of brane inflation is the production of cosmic strings towards the end of inflation. These cosmic strings are nothing but superstrings stretched to cosmological sizes. The properties of these cosmic superstrings and their subsequent cosmological evolution into a scaling network open up their possible detections in…
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Taxonomy
TopicsCosmology and Gravitation Theories · Solar and Space Plasma Dynamics · Black Holes and Theoretical Physics
