English

F-term Inflation and Leptogenesis with 5D SO(10)

High Energy Physics - Phenomenology 2007-05-23 v2

Abstract

We discuss a five dimensional inflationary scenario based on a supersymmetric SO(10) model compactified on S1/(Z2×Z2)S^1/(Z_2\times Z_2'). Inflation is implemented through scalar potentials on four dimensional branes, and a brane-localized Einstein-Hilbert term is essential to make both brane vacuum energies positive during inflation. The orbifold boundary conditions break the SO(10) gauge symmetry to SU(4)c×SU(2)L×SU(2)RSU(4)_c\times SU(2)_L\times SU(2)_R (H\equiv H). The inflationary scenario yields δT/T(M/MPlanck)2\delta T/T\propto (M/M_{\rm Planck})^2, which fixes MM, the symmetry breaking scale of HH to be close to the SUSY GUT scale of 101610^{16} GeV. The scalar spectral index nn is 0.980.990.98-0.99, and the tensor to scalar ratio rr is \lapproxeq104\lapproxeq 10^{-4}. The inflaton decay into the lightest right handed neutrinos yields the observed baryon asymmetry via leptogenesis.

Keywords

Cite

@article{arxiv.hep-ph/0308158,
  title  = {F-term Inflation and Leptogenesis with 5D SO(10)},
  author = {Bumseok Kyae},
  journal= {arXiv preprint arXiv:hep-ph/0308158},
  year   = {2007}
}

Comments

Contribution to the Proceedings of SUGRA20, International Conference 20 Years of SUGRA and Search for SUSY and Unification, Northeastern University, Boston, March 2003

R2 v1 2026-07-22T13:49:31.664Z