English

Supersymmetric Models For Gauge Inflation

High Energy Physics - Phenomenology 2008-11-26 v3 Astrophysics High Energy Physics - Theory

Abstract

We present possible realizations of gauge inflation arising from a 5D N=1{\cal N}=1 supersymmetric U(1) model, where the extra dimension is compactified on a circle. A one-loop inflaton effective 4D potential is generated, with the inflaton being a 'Wilson-line field'. It relies on a SUSY breaking. We first consider SUSY breaking to occur spontaneously within a 'no-scale' model by a non zero FF-term of the radion superfield which transmits SUSY breaking into the 'visible' sector. As an alternative, we study DD-term SUSY breaking originating directly from the 5D gauge supermultiplet. Together with the usual KK resummation method, we present a calculation with the world-line formalism. The latter allows one to get the resulting effective potential directly as a sum over all winding modes. For both presented scenarios, the generated effective potentials have suitable forms for realizing successful inflation, i.e. are flat enough and give the needed number of e{\rm e}-foldings. In addition, there is a natural way to get strongly suppressed values for the potentials, which then could be associated with dark energy/quintessence.

Keywords

Cite

@article{arxiv.hep-ph/0305230,
  title  = {Supersymmetric Models For Gauge Inflation},
  author = {R. Hofmann and F. Paccetti Correia and M. G. Schmidt and Z. Tavartkiladze},
  journal= {arXiv preprint arXiv:hep-ph/0305230},
  year   = {2008}
}

Comments

LaTeX, 16 pages, typos corrected and refs. added

R2 v1 2026-07-22T13:48:06.537Z