Observable ${\rm \Delta{N_{eff}}}$ in Dirac Scotogenic Model

TL;DR

This paper explores how future CMB experiments can detect signatures of the Dirac scotogenic model through measurements of extra relativistic degrees of freedom, linking dark matter, neutrino mass, and cosmological observations.

Contribution

It demonstrates that the parameter space of the Dirac scotogenic model can be probed via ${ m riangle N_{eff}}$ measurements, connecting dark matter, neutrino physics, and cosmology.

Findings

Future CMB experiments can test the model's parameter space.

Large Yukawa couplings can thermalize right-handed neutrinos.

Complementary signals include charged lepton flavor violation and collider signatures.

Abstract

We study the possibility of probing the radiative Dirac seesaw model with dark sector particles going inside the loop, popularly referred to as the Dirac scotogenic model via measurements of effective relativistic degrees of freedom ${\rm \Delta{N_{eff}}}$ at cosmic microwave background (CMB) experiments. The loop suppression and additional free parameters involved in neutrino mass generation allow large ($\sim\mathcal{O}(1))$ coupling of light Dirac neutrinos with the dark sector particles. Such large Yukawa coupling not only dictates the relic abundance of heavy fermion singlet dark matter but also can lead to the thermalisation of the right chiral part of Dirac neutrinos, generating additional relativistic degrees of freedom ${\rm \Delta{N_{eff}}}$. We find that the parameter space consistent with dark matter phenomenology and neutrino mass bounds can also be probed at future cosmic microwave background experiments like CMB-S4 via precision measurements of ${\rm \Delta{N_{eff}}}$. The same parameter space, while leading to loop-suppressed direct detection cross-section of dark matter outside future sensitivities, can also have other interesting and complementary observational prospects via charged lepton flavour violation and collider signatures.