The recent high precision measurement of W boson mass by CDF-II collaboration points to the contribution(s) of new physics beyond the Standard Model. One of the minimalistic ways to account for the anomalous W boson mass is by introducing a hyperchargeless real SU (2) L triplet scalar whose vacuum expectation value explicitly contributes to the W boson mass at the tree level while the Z boson mass remains the same. Such a triplet can be naturally embedded in a singlet-triplet scotogenic model for one loop neutrino mass generated by dark sector particles running in the loop. We discuss the detailed phenomenology of the model, obtaining the parameter space consistent with the CDF-II W boson mass measurements. The dark matter as well as the constraints comings from S, T , U parameters are also analyzed.

The CDF-II collaboration's recent high-precision measurement of W boson mass indicates new physics contribution(s) beyond the Standard Model. We investigate the possibility of the well-known canonical Scotogenic model, where dark matter particle running in the loop generates neutrino masses, to explain the CDF-II measurement. We show that the doublet scalar carrying a dark parity charge can account for the W boson mass anomaly through oblique S,T,U parameter corrections. For both scalar and fermionic dark matter possibilities, we simultaneously examine the constraints coming from a) neutrino mass, oscillation, neutrinoless double beta decay and lepton flavour violation experiments, b) from dark matter relic density and direct detection experiments c) from the oblique S,T,U parameter values consistent with CDF-II W boson measurement. We show that the canonical Scotogenic model can simultaneously explain all the aforementioned issues.