English

Heavier $W$ boson, dark matter and gravitational waves from strings in an $SO(10)$ axion model

High Energy Physics - Phenomenology 2022-09-08 v2 Cosmology and Nongalactic Astrophysics

Abstract

Inspired by the recent determination of the WW-boson mass by the CDF collaboration, we revisit an SO(10)SO(10) axion model in which a scalar SU(2)LSU(2)_L triplet field with zero hypercharge is known to acquire a non-zero VEV through its mixing with the Standard Model Higgs doublet. The triplet VEV provides a sizable contribution to the WW mass, which helps in significantly lowering the 7σ7\sigma discrepancy between the Standard Model prediction and the higher CDF value for mWm_W. We show that the relatively light triplet mass ((150)\sim (1-50) TeV) is compatible with gauge coupling unification and observable proton decay. An unbroken Z2Z_2 gauge symmetry, coupled with the presence of two fermionic 1010-plets required to resolve the axion domain wall problem, means that both axions and a stable intermediate mass (1091010\sim 10^9-10^{10} GeV) fermion are plausible dark matter candidates. We also display the gravitational wave spectrum from the intermediate scale topologically stable cosmic strings predicted by the model.

Keywords

Cite

@article{arxiv.2205.04824,
  title  = {Heavier $W$ boson, dark matter and gravitational waves from strings in an $SO(10)$ axion model},
  author = {George Lazarides and Rinku Maji and Rishav Roshan and Qaisar Shafi},
  journal= {arXiv preprint arXiv:2205.04824},
  year   = {2022}
}

Comments

20 pages, 6 figures, published version