Radiative origin of neutrino masses

[en] Mechanisms for Majorana neutrino mass generation can be classified according to the level at which the Weinberg operator is generated. The different possibilities can be sorted in “canonical” tree-level and loop-induced realizations, the latter being motivated by their potential experimental testability. Here, we discuss the one- and two-loop cases, paying special attention to systematic classification schemes, whose aim is that of constructing a full picture for neutrino mass generation

Disciplines :

Physics

Author, co-author :

Aristizabal Sierra, Diego ; Université de Liège > Département d'astrophys., géophysique et océanographie (AGO) > Inter. fondamentales en physique et astrophysique (IFPA)

Language :

English

Title :

Radiative origin of neutrino masses

Publication date :

November 2015

Journal title :

Acta Physica Polonica B

ISSN :

0587-4254

eISSN :

1509-5770

Publisher :

Institute of Physics Jagiellonian University, Krakow, Poland

Volume :

Pages :

2311

Peer reviewed :

Peer Reviewed verified by ORBi

Available on ORBi :

since 18 January 2016

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