Brany Liouville Inflation
John Ellis (CERN), N.E. Mavromatos (King's Coll. Lon.), D.V., Nanopoulos (TAMU), A. Sakharov (CERN, ETH)

TL;DR
This paper proposes a string theory-based inflation model driven by the Liouville field, connecting brane dynamics with cosmological observations and suggesting a small, evolving vacuum energy component.
Contribution
It introduces a novel inflationary model using non-critical supersymmetric string theory with brane dynamics, constrained by cosmic microwave background and gamma-ray burst data.
Findings
Model parameters fixed by WMAP data
Consistent with gamma-ray burst light propagation constraints
Suggests a small, relaxing vacuum energy component
Abstract
We present a specific model for cosmological inflation driven by the Liouville field in a non-critical supersymmetric string framework, in which the departure from criticality is due to open strings stretched between the two moving Type-II 5-branes. We use WMAP and other data on fluctuations in the cosmic microwave background to fix parameters of the model, such as the relative separation and velocity of the 5-branes, respecting also the constraints imposed by data on light propagation from distant gamma-ray bursters. The model also suggests a small, relaxing component in the present vacuum energy that may accommodate the breaking of supersymmetry.
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