English

Low scale Dirac leptogenesis and dark matter with observable $\Delta N_{\rm eff}$

High Energy Physics - Phenomenology 2022-06-15 v2 Cosmology and Nongalactic Astrophysics

Abstract

We propose a gauged BLB-L extension of the standard model (SM) where light neutrinos are of Dirac type by virtue of tiny Yukawa couplings with the SM Higgs. To achieve leptogenesis, we include additional heavy Majorana fermions without introducing any BLB-L violation by two units. An additional scalar doublet with appropriate BLB-L charge can allow heavy fermion coupling with the SM leptons so that out of equilibrium decay of the former can lead to generation of lepton asymmetry. Due to the BLB-L gauge interactions of the decaying fermion, the criteria of successful Dirac leptogenesis can also constrain the gauge sector couplings so as to keep the corresponding washout processes under control. The same BLB-L gauge sector parameter space can also be constrained from dark matter requirements if the latter is assumed to be a SM singlet particle with non-zero BLB-L charge. The same BLB-L gauge interactions also lead to additional thermalised relativistic degrees of freedom ΔNeff\Delta N_{\rm eff} from light Dirac neutrinos which are tightly constrained by Planck 2018 data. While there exists parameter space from the criteria of successful low scale Dirac leptogenesis, dark matter and ΔNeff\Delta N_{\rm eff} even after incorporating the latest collider bounds, all the currently allowed parameters can be probed by future measurements of ΔNeff\Delta N_{\rm eff}.

Keywords

Cite

@article{arxiv.2101.02092,
  title  = {Low scale Dirac leptogenesis and dark matter with observable $\Delta N_{\rm eff}$},
  author = {Devabrat Mahanta and Debasish Borah},
  journal= {arXiv preprint arXiv:2101.02092},
  year   = {2022}
}

Comments

39 pages, 10 figures, Version that matches the one accepted in EPJC