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I will discuss several possible choices for the mass scale M of the Majorana leptons, complementing the Standard Model to describe neutrino masses and oscillations. Depending on M, they can or cannot accommodate eV neutrino anomalies, lead to baryogenesis, provide the dark matter candidate, ensure the stability of the Higgs mass against radiative corrections, and be directly searched at some experiments.
Joanna Malgorzata Wanczyk, Jan Steggemann, Konstantin Androsov
Aurelio Bay, Mikhail Chapochnikov, Guido Haefeli, Olivier Schneider, Sun Hee Kim, Lesya Shchutska, Paul Théodore Gabriel Pablo De Bryas Dexmiers d'Archiac, Inar Timiryasov, Anna Mascellani, Carina Trippl, Serhii Cholak, Elena Graverini, Ettore Zaffaroni, Jan Steggemann, Konstantin Androsov, Anni Matilda Kauniskangas, Federico Ronchetti, Zhibin Yang
Anna Mascellani, Jan Steggemann, Konstantin Androsov