paper

Inflationary Cosmology with Five Dimensional SO(10)

arXiv:hep-ph/0212331 · doi:10.1103/PhysRevD.69.046004

Abstract

We discuss inflationary cosmology in a five dimensional SO(10) model compactified on , which yields below the compactification scale. The gauge symmetry is preserved on one of the fixed points, while ``flipped'' is on the other fixed point. Inflation is associated with breaking, and is implemented through -term scalar potentials on the two fixed points. A brane-localized Einstein-Hilbert term allows both branes to have positive tensions during inflation. The scale of breaking is fixed from measurements to be around GeV, and the scalar spectral index . The inflaton field decays into right-handed neutrinos whose subsequent out of equilibrium decay yield the observed baryon asymmetry via leptogenesis.

1+19 pages, improved discussion of 5D cosmology, Version to appear in PRD

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