Light Dirac neutrino portal dark matter with observable
arXiv:2103.05648 · doi:10.1088/1475-7516/2021/10/002
Abstract
We propose a Dirac neutrino portal dark matter scenario by minimally extending the particle content of the Standard Model (SM) with three right handed neutrinos (), a Dirac fermion dark matter candidate () and a complex scalar (), all of which are singlets under the SM gauge group. An additional symmetry has been introduced for the stability of dark matter candidate and also ensuring the Dirac nature of light neutrinos at the same time. Both the right handed neutrinos and the dark matter thermalise with the SM plasma due to a new Yukawa interaction involving , and while the latter maintains thermal contact via the Higgs portal interaction. The decoupling of occurs when loses its kinetic equilibrium with the SM plasma and thereafter all three charged particles form an equilibrium among themselves with a temperature . The dark matter candidate finally freezes out within the dark sector and preserves its relic abundance. We have found that in the present scenario, some portion of low mass dark matter ( GeV) is already excluded by the Planck 2018 data for keeping s in the thermal bath below a temperature of 600 MeV and thereby producing an excess contribution to . The next generation experiments like CMB-S4, SPT-3G etc. will have the required sensitivities to probe the entire model parameter space of this minimal scenario, especially the low mass range of where direct detection experiments are still not capable enough for detection.
39 pages, 7 figures, 1 table, a new discussion related to the decay of has been added in Appendix A, new figures are added, new references are added, conclusion remains unchanged, version accepted for publication in JCAP
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