https://doi.org/10.1140/epjp/s13360-025-06099-1
Regular Article
Two dark matter candidates in a doublet-triplet Higgs model
1
Instituto de Física, Universidad Nacional Autónoma de México, A.P. 20-364, C.P. 01000, CDMX, México
2
Departamento de Astronomía y Astrofísica, Facultad de Ciencias Espaciales, Universidad Nacional Autónoma de Honduras, Bulevar Suyapa, Tegucigalpa, M.D.C., Honduras
3
Departamento de Física, Facultad de Estudios Superiores Cuautitlán, Universidad Nacional Autónoma de México, 54770, Estado de México, México
4
Departamento de Física, Centro de Investigación y de Estudios Avanzados del IPN, Apdo. Postal 14-740 07000, Ciudad de México, México
Received:
16
January
2024
Accepted:
6
February
2025
Published online:
24
February
2025
We study a Standard Model extension that provides a bi-component dark matter scenario as well as a mechanism for the generation of left-handed neutrino masses. We extend the Standard Model scalar sector by adding an inert complex doublet with hypercharge
and a real inert
triplet with hypercharge
. These scalars provide suitable dark matter candidates belonging to two different dark sectors that are stabilised by the discrete symmetries
. We consider the contribution of both candidates to the total relic abundance in order to reduce the desert regions in the inert doublet and inert triplet models. In addition, we have added an active real scalar
triplet with hypercharge
in order to generate light neutrino Majorana masses through the type-II seesaw mechanism. We have analysed the dark matter phenomenology for the model and alongside with the neutrino mass generation.
Copyright comment Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
© The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2025
Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.