Naturally Stable Right-Handed Neutrino Dark Matter
P. S. Bhupal Dev, Rabindra N. Mohapatra, Yongchao Zhang

TL;DR
This paper introduces a non-supersymmetric left-right symmetric model with an exact Z2 symmetry that stabilizes the lightest right-handed neutrino, making it a natural dark matter candidate with distinctive collider and detection signatures.
Contribution
The model uniquely incorporates an automatic Z2 symmetry in a non-supersymmetric left-right framework, enabling stable right-handed neutrino dark matter with specific phenomenological predictions.
Findings
Dark matter mass lower bound around 1 TeV
Potential to relax unitarity bounds via entropy dilution
Predicted long-lived colored particles for collider searches
Abstract
We point out that a class of non-supersymmetric models based on the gauge group possesses an automatic, exact symmetry under which the fermions in the sector (called -sector) are odd and those in the standard model sector (called -sector) are even. This symmetry, which is different from the usual parity symmetry of the left-right symmetric models, persists in the lepton sector even after the gauge symmetry breaks down to . This keeps the lightest right-handed neutrino naturally stable, thereby allowing it to play the role of dark matter (DM) in the Universe. There are several differences between the usual left-right models and the model presented here: (i) our model can have two versions, one which has no parity symmetry so that the couplings…
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