Cosmology of the tachyon in brane inflation

Louis Leblond, Sarah Shandera

Research output: Contribution to journalArticle

21 Citations (Scopus)

Abstract

In certain implementations of the brane inflationary paradigm, the exit from inflation occurs when the branes annihilate through tachyon condensation. We investigate various cosmological effects produced by this tachyonic era. We find that only a very small region of the parameter space (corresponding to slow roll with tiny inflaton mass) allows for the tachyon to contribute some e-folds to inflation. In addition, non-adiabatic density perturbations are generated at the end of inflation. When the brane is moving relativistically this contribution can be of the same order as fluctuations produced 55 e-folds before the end of inflation. The additional contribution is exactly scale invariant and enhances the tensor/scalar ratio. Additional non-Gaussianities will also be generated, sharpening current constraints on Dirac-Born-Infeld-type models which already predict a significantly non-Gaussian signal.

Original languageEnglish (US)
Article number009
JournalJournal of Cosmology and Astroparticle Physics
Issue number1
DOIs
StatePublished - Jan 1 2007

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cosmology
condensation
tensors
scalars
perturbation

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics

Cite this

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Cosmology of the tachyon in brane inflation. / Leblond, Louis; Shandera, Sarah.

In: Journal of Cosmology and Astroparticle Physics, No. 1, 009, 01.01.2007.

Research output: Contribution to journalArticle

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