CDF-II $W$ Boson Mass Anomaly in the Canonical Scotogenic Neutrino-Dark Matter Model
Aditya Batra, ShivaSankar K.A, Sanjoy Mandal, Hemant Prajapati, Rahul, Srivastava

TL;DR
This paper explores whether the canonical Scotogenic model can explain the CDF-II W boson mass anomaly, analyzing constraints from various experiments and identifying viable dark matter mass ranges.
Contribution
It demonstrates that the scalar dark matter in the model is ruled out at high masses but viable at intermediate masses, and shows fermionic dark matter can explain the anomaly within certain mass ranges.
Findings
Scalar dark matter above 500 GeV is ruled out by CDF-II data.
Intermediate scalar dark matter masses (54-76 GeV) remain viable.
Fermionic dark matter below 500 GeV can simultaneously satisfy all constraints.
Abstract
The CDF-II collaboration's recent high-precision measurement of boson mass indicates new physics contribution(s) beyond the Standard Model. We investigate the possibility of the well-known canonical Scotogenic model to explain the CDF-II measurement. The Scotogenic model is a popular scenario beyond the Standard Model that induces neutrino masses at the 1-loop level and includes a viable dark matter candidate, either scalar or fermionic. 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 LEP and LHC (c) from dark matter relic density and direct detection experiments (d) from the oblique parameter values consistent with CDF-II boson measurement. We demonstrate that the new CDF-II measurement rules out…
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Dark Matter and Cosmic Phenomena · Computational Physics and Python Applications
