D-brane Inflation
G. Dvali, Q. Shafi, S. Solganik

TL;DR
This paper presents a calculable model of brane inflation where parallel D-branes attract each other, leading to a slow-roll inflationary phase with specific spectral index and reheating mechanisms.
Contribution
It introduces a concrete brane inflation scenario with detailed calculations of inflation dynamics and observable predictions, advancing the understanding of string-inspired cosmology.
Findings
Spectral index approximately 0.97
Effective compactification scale around 10^{12} GeV
Reheating via brane collision and annihilation
Abstract
We discuss a calculable version of brane inflation, in which a set of parallel D-brane and anti-D-brane worlds, initially displaced in extra dimension, slowly attract each other. In the effective four-dimensional theory this slow motion of branes translates into a slow-roll of a scalar field (proportional to their separation) with a flat potential that drives inflation. The number of possible e-foldings is severely constrained. The scalar spectral index is found to be 0.97, while the effective compactification scale is of order GeV. Reheating of the Universe is provided by collision and subsequent annihilation of branes.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Geophysics and Gravity Measurements
