17–24 Jul 2024
Prague
Europe/Prague timezone

Neutrino Masses from a Hybrid Type I + III Inverse Seesaw Mechanism in $U(1)_{R-L}$-symmetric MSSM

20 Jul 2024, 11:15
15m
Panorama

Panorama

Parallel session talk 02. Neutrino Physics Neutrino Physics

Speaker

Cem Murat Ayber (Carleton University)

Description

We show that, in a $U(1)_{R-L}$-symmetric SUSY model, the pseudo-Dirac bino and wino can give rise to three light neutrino masses through effective operators, generated at the messenger scale between a SUSY breaking hidden sector and the visible sector. The neutrino-bino/wino mixing follows a hybrid type I+III inverse seesaw pattern. The light neutrino masses are governed by the ratio of the $U(1)_{R-L}$-breaking gravitino mass, $m_{3/2}$, and the messenger scale $\Lambda_M$. The charged component of the $SU(2)_L$-triplet, here the lightest charginos, mix with the charged leptons and generate FCNC at tree level. We find that resulting LFV observables yield a lower bound on the messenger scale, $\Lambda_M\gtrsim(500-1000)~{\rm TeV}$ for a simplified hybrid mixing scenario. We identify interesting mixing structures for certain $U(1)_{R-L}$-breaking singlino/tripletino Majorana masses. We describe the rich collider phenomenology expected in this neutrino-mass generation mechanism.

Alternate track 03. Beyond the Standard Model
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Author

Cem Murat Ayber (Carleton University)

Co-author

Presentation materials