With one scalar coupling tuned to about 10^-3, the minimal left-right symmetric model predicts a first-order phase transition whose gravitational waves could be seen by LISA and other planned space interferometers.
Probing Heavy-Light Neutrino Mixing in Left-Right Seesaw Models at the LHC
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abstract
We show that in TeV-scale left-right (L-R) symmetric seesaw models, there are new dominant contributions to the collider signals of heavy Majorana neutrinos arising from the heavy-light neutrino mixing, which directly probe the seesaw matrix in a certain class of models. We propose a way to distinguish this contribution from the widely discussed one that only probes the Majorana nature of the heavy right-handed neutrinos, by analyzing some simple kinematical variables. We find that in this class of L-R seesaw models the existing LHC data already yield slightly stronger constraints on the heavy-light neutrino mixing than those derived for standard seesaw models, and the improvement will be significant as more data are collected.
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Gravitational Waves as a Probe of Left-Right Symmetry Breaking
With one scalar coupling tuned to about 10^-3, the minimal left-right symmetric model predicts a first-order phase transition whose gravitational waves could be seen by LISA and other planned space interferometers.