Spinflation

D. Easson, R. Gregory, D. Mota, Gianmassimo Tasinato, I. Zavala

Research output: Contribution to journalArticlepeer-review

81 Downloads (Pure)

Abstract

We study the cosmological implications of including angular motion in the DBI brane inflation scenario. The non-canonical kinetic terms of the Dirac-Born-Infeld action give an interesting alternative to slow roll inflation, and cycling branes can drive periods of accelerated expansion in the Universe. We present explicit numerical solutions demonstrating brane inflation in the Klebanov-Strassler throat. We find that demanding sufficient inflation takes place in the throat is in conflict with keeping the brane's total energy low enough so that local gravitational backreaction on the Calabi-Yau manifold can be safely ignored. We deduce that spinflation (brane inflation with angular momentum) can ease this tension by providing extra e-foldings at the start of inflation. Cosmological expansion rapidly damps the angular momentum causing an exit to a more conventional brane inflation scenario. Finally, we set up a general framework for cosmological perturbation theory in this scenario, where we have multi-field non-standard kinetic term inflation.
Original languageEnglish
Pages (from-to)010
Number of pages1
JournalJournal of Cosmology and Astroparticle Physics
Volume2008
Issue number2
DOIs
Publication statusPublished - Feb 2008

Fingerprint

Dive into the research topics of 'Spinflation'. Together they form a unique fingerprint.

Cite this