English

Majorana Fermion Dark Matter in Minimally Extended Left-Right Symmetric Model

High Energy Physics - Phenomenology 2021-03-17 v1 Cosmology and Nongalactic Astrophysics High Energy Physics - Experiment

Abstract

We present a minimal extension of the left-right symmetric model based on the gauge group SU(3)c×SU(2)L×SU(2)R×U(1)BL×U(1)XSU(3)_{c} \times SU(2)_{L} \times SU(2)_{R} \times U(1)_{B-L} \times U(1)_{X}, in which a vector-like fermion pair (ζL\zeta_L and ζR\zeta_R) charged under the U(1)BL×U(1)XU(1)_{B-L} \times U(1)_X symmetry is introduced. Associated with the symmetry breaking of the gauge group SU(2)R×U(1)BL×U(1)XSU(2)_{R} \times U(1)_{B-L} \times U(1)_{X} down to the Standard Model (SM) hypercharge U(1)YU(1)_Y, Majorana masses for ζL,R\zeta_{L, R} are generated and the lightest mass eigenstate plays a role of the dark matter (DM) in our universe by its communication with the SM particles through a new neutral gauge boson "XX". We consider various phenomenological constraints of this DM scenario, such as the observed DM relic density, the LHC Run-2 constraints from the search for a narrow resonance, and the perturbativity of the gauge couplings below the Planck scale. Combining all constraints, we identify the allowed parameter region which turns out to be very narrow. A significant portion of the currently allowed parameter region will be tested by the High-Luminosity LHC experiments.

Keywords

Cite

@article{arxiv.2103.08873,
  title  = {Majorana Fermion Dark Matter in Minimally Extended Left-Right Symmetric Model},
  author = {M. J. Neves and Nobuchika Okada and Satomi Okada},
  journal= {arXiv preprint arXiv:2103.08873},
  year   = {2021}
}

Comments

23 pages, 6 figures