Feasibility to probe the dynamical scotogenic model at the LHC
Gustavo Ardila-Tafurth, Andrés Flórez, Cristian Rodríguez, Maud Sarazin, Óscar Zapata
TL;DR
This work assesses the collider feasibility of the dynamical scotogenic model, which links neutrino masses and dark matter through a global U(1)$_L$ symmetry and a Z$_2$-odd dark sector. By performing an MCMC scan that honors neutrino data, Higgs invisible decays, and DM constraints, the authors identify viable compressed-spectrum regions and evaluate Drell–Yan and Vector Boson Fusion production at the LHC. They find that fermionic DM can be probed via DY at the HL-LHC for masses between 100 and 220 GeV, while VBF channels remain below reach for both DM candidates; scalar DM prospects are generally poor at the LHC but may benefit modestly from FCC-hh energies. Overall, the DY channel provides the best collider sensitivity to fermionic DM in this framework, with future higher-energy machines offering incremental gains in specific mass ranges.
Abstract
We perform a feasibility study to probe dark matter (DM) production at the LHC within a global $U(1)_L$ scotogenic model. The study is conducted using the Markov Chain Monte Carlo numerical method, considering the viable parameter space of the model allowed by experimental constraints such as neutrino oscillation data, the Higgs to invisible branching fraction, and DM observables. The production of scalar and fermionic DM candidates, predicted by the model, is then studied under the LHC conditions for different luminosity scenarios imposing compressed mass spectra conditions between the lightest fermion and the $\mathbb{Z}_2$ odd scalars. We studied two production mechanisms, Drell-Yan and Vector Boson Fusion. It was found that the Drell-Yan mechanism gives better detection prospects for fermionic DM masses between 100-220~\textrm{GeV} at high luminosity scenarios.
