English

Axions, WIMPs, proton decay and observable $r$ in $SO(10)$

High Energy Physics - Phenomenology 2023-04-19 v1

Abstract

We explore some experimentally testable predictions of an SO(10)SO(10) axion model which includes two 10-plets of fermions in order to resolve the axion domain wall problem. The axion symmetry can be safely broken after inflation, so that the isocurvature perturbations associated with the axion field are negligibly small. An unbroken gauge Z2Z_2 symmetry in SO(10)SO(10) ensures the presence of a stable WIMP-like dark matter, a linear combination of the electroweak doublets in the fermion 10-plets and an SO(10)SO(10) singlet fermion with mass 62.5  GeV  (1  TeV)\sim 62.5 \; {\rm GeV}\; (1 \; {\rm TeV}) when it is mostly the singlet (doublet) fermion, that co-exists with axion dark matter. We also discuss gauge coupling unification, proton decay, inflation with non-minimal coupling to gravity and leptogenesis. With the identification of the SM singlet Higgs field in the 126126 representation of SO(10)SO(10) as inflaton, the magnetic monopoles are inflated away, and we find 0.963ns0.9650.963 \lesssim n_s \lesssim 0.965 and 0.003r0.0360.003 \lesssim r \lesssim 0.036, where nsn_s and rr denote the scalar spectral index and tensor-to-scalar ratio, respectively. These predictions can be tested in future experiments such as CMB-S4.

Keywords

Cite

@article{arxiv.2207.10538,
  title  = {Axions, WIMPs, proton decay and observable $r$ in $SO(10)$},
  author = {Nobuchika Okada and Digesh Raut and Qaisar Shafi},
  journal= {arXiv preprint arXiv:2207.10538},
  year   = {2023}
}

Comments

21 pages, 6 figures