Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.11889/6937
Title: Dark matter in three-Higgs-doublet models with $S_3$ symmetry
Authors: Khater, W. 
Kunčinas, A. 
Ogreid, O. M. 
Osland, P. 
Rebelo, M. N. 
Keywords: High Energy Physics - Phenomenology
Issue Date: 16-Aug-2021
Journal: Journal of High Energy Physics (JHEP) 
Abstract: Models with two or more scalar doublets with discrete or global symmetries can have vacua with vanishing vacuum expectation values in the bases where symmetries are imposed. If a suitable symmetry stabilises such vacua, these models may lead to interesting dark matter candidates, provided that the symmetry prevents couplings among the dark matter candidates and the fermions. We analyse three-Higgs-doublet models with an underlying $S_3$ symmetry. These models have many distinct vacua with one or two vanishing vacuum expectation values which can be stabilised by a remnant of the $S_3$ symmetry which survived spontaneous symmetry breaking. We discuss all possible vacua in the context of $S_3$-symmetric three-Higgs-doublet models, allowing also for softly broken $S_3$, and explore one of the vacuum configurations in detail. In the case we explore, only one of the three Higgs doublets is inert. The other two are active, and therefore the active sector, in many aspects, behaves like a two-Higgs-doublet model. The way the fermions couple to the scalar sector is constrained by the $S_3$ symmetry and is such that the flavour structure of the model is solely governed by the $V_\text{CKM}$ matrix which, in our framework, is not constrained by the $S_3$ symmetry. This is a key requirement for models with minimal flavour violation. In our model there is no CP violation in the scalar sector. We study this model in detail giving the masses and couplings and identifying the range of parameters that are compatible with theoretical and experimental constraints, both from accelerator physics and from astrophysics.
Description: 50 pages, 14 figures, V2: typos fixed, some plots changed, V3: minor text edits, V4: version consistent with JHEP
URI: http://hdl.handle.net/20.500.11889/6937
DOI: http://arxiv.org/abs/2108.07026v4
10.1007/JHEP01(2022)120
http://arxiv.org/abs/2108.07026v4
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