Fits to non-supersymmetric SO(10) models with type I and II seesaw mechanisms using renormalization group evolution

Journal: Journal of High Energy Physics

Published: 2019-06-18

DOI: 10.1007/jhep06(2019)085

Affiliations: 3

Authors: 2

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AlbaNova University Center - Stockholm Center for Physics, Astronomy and Biotechnology (AlbaNova), Sweden 0.42
Oskar Klein Centre for Cosmoparticle Physics (OKC), Sweden 0.42
Science Institute, University of Iceland, Iceland 0.17