How many 1-loop neutrino mass models are there?

Author:

Arbeláez Carolina,Cepedello RicardoORCID,Helo Juan Carlos,Hirsch Martin,Kovalenko Sergey

Abstract

Abstract It is well-known that at tree-level the d = 5 Weinberg operator can be generated in exactly three different ways, the famous seesaw models. In this paper we study the related question of how many phenomenologically consistent 1-loop models one can construct at d=5. First, we discuss that there are two possible classes of 1-loop neutrino mass models, that allow avoiding stable charged relics: (i) models with dark matter candidates and (ii) models with “exits”. Here, we define “exits” as particles that can decay into standard model fields. Considering 1-loop models with new scalars and fermions, we find in the dark matter class a total of (115+203) models, while in the exit class we find (38+368) models. Here, 115 is the number of DM models, which require a stabilizing symmetry, while 203 is the number of models which contain a dark matter candidate, which maybe accidentally stable. In the exit class the 38 refers to models, for which one (or two) of the internal particles in the loop is a SM field, while the 368 models contain only fields beyond the SM (BSM) in the neutrino mass diagram. We then study the RGE evolution of the gauge couplings in all our 1-loop models. Many of the models in our list lead to Landau poles in some gauge coupling at rather low energies and there is exactly one model which unifies the gauge couplings at energies above 1015 GeV in a numerically acceptable way.

Publisher

Springer Science and Business Media LLC

Subject

Nuclear and High Energy Physics

Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Radiative neutrino masses and the Cohen-Kaplan-Nelson bound;Journal of High Energy Physics;2023-11-13

2. Phenomenological and cosmological implications of a scotogenic three-loop neutrino mass model;Journal of High Energy Physics;2023-03-06

3. Mapping the SMEFT to discoverable models;Journal of High Energy Physics;2022-09-27

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