Speaker
Description
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 ($\nu_R$), a Dirac fermion dark matter candidate ($\psi$) and a complex scalar ($\phi$), all of which are singlets under the SM gauge group. An additional $\mathbb{Z}_4$ symmetry has been introduced for the stability of dark matter candidate ψ 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 $\nu_R$, $\psi$ and $\phi$ while the latter maintains thermal contact via the Higgs portal interaction. The decoupling of $\nu_R$ occurs when $\phi$ loses its kinetic equilibrium with the SM plasma and thereafter all three $\mathbb{Z}_4$ charged particles form an equilibrium among themselves with a temperature $T_{\nu_R}$. The dark matter candidate $\psi$ 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 ($M_{\psi} \leq 10$ GeV) is already excluded by the Planck 2018 data for keeping $\nu_R$s in the thermal bath below a temperature of 600 MeV and thereby producing an excess contribution to N$_{\rm eff}$. 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 $\psi$ where direct detection experiments are still not capable enough for detection.
| Session | Astroparticle Physics and Cosmology |
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