English

Axion Model with Intermediate Scale Fermionic Dark Matter

High Energy Physics - Phenomenology 2020-07-08 v2 Cosmology and Nongalactic Astrophysics

Abstract

We investigate a non-supersymmetric SO(10)×U(1)PQSO(10)\times U(1)_{\rm PQ} axion model in which the spontaneous breaking of U(1)PQU(1)_{\rm PQ} occurs after inflation, and the axion domain wall problem is resolved by employing the Lazarides-Shafi mechanism. This requires the introduction of two fermion 10-plets, such that the surviving discrete symmetry from the explicit U(1)PQU(1)_{\rm PQ} breaking by QCD instantons is reduced from Z12Z_{12} to Z4Z_4, where Z4Z_4 coincides with the center of SO(10)SO(10) (more precisely Spin(10)Spin(10)). An unbroken Z2Z_2 subgroup of Z4Z_4 yields intermediate scale topologically stable strings, as well as a stable electroweak doublet non-thermal dark matter candidate from the fermion 10-plets with mass comparable to or somewhat smaller than the axion decay constant faf_{\rm a}. We present an explicit realization with inflation taken into account and which also incorporates non-thermal leptogenesis. The fermion dark matter mass lies in the 3×1081010 GeV3\times 10^{8}-10^{10}~{\rm GeV} range and its contribution to the relic dark matter abundance can be comparable to that from the axion.

Keywords

Cite

@article{arxiv.2004.11560,
  title  = {Axion Model with Intermediate Scale Fermionic Dark Matter},
  author = {George Lazarides and Qaisar Shafi},
  journal= {arXiv preprint arXiv:2004.11560},
  year   = {2020}
}

Comments

9 pages, 5 figures included, version to be published in Phys. Lett. B

R2 v1 2026-06-23T15:04:10.129Z