Abstract

We consider the extension of the standard model by dark fields with an Abelian spontaneously broken gauge symmetry in a hidden dark matter scenario. The dimension-four gauge-invariant terms include a kinetic mixing term and a Higgs mixing term, and we show that, after spontaneous symmetry breaking, the tree-level relation $M^{2}_{W}=M^{2}_{\tilde{Z}} \cos ^{2} \tilde{\theta }_{w}$ holds and permits us to write the mixing angle induced by the kinetic mixing in the neutral massive gauge boson sector, θζ, in terms of the values of MZ, the weak mixing angle, and of the mass of the physical dark gauge boson ZD. At the loop level, a similar relation is obtained in the $\overline{MS}$ scheme. Using the result extracted from the global fit to electroweak precision data for the ratio $\rho _{0}=M^{2}_{W}/\hat{c}^{2}_{Z} M^{2}_{Z}\hat{\rho }$, we obtain the lower bound $M_{Z_{D}}\gt M_{Z}$ for the dark gauge boson mass at the $94\%$ confidence level. We argue that this lower bound holds in the general case of theories for physics beyond the standard model with an extra U(1) gauge factor subgroup, whenever the extended Higgs potential respects custodial symmetry.

Details

Title
Kinetic mixing, custodial symmetry, and a lower bound on the mass of a dark gauge boson
Author
Napsuciale, M 1 ; Rodríguez, S 2 ; Hernández-Arellano, H 1 

 Departamento de Física, Universidad de Guanajuato , Lomas del Campestre 103, Fraccionamiento Lomas del Campestre, León, Guanajuato México , 37150 
 Facultad de Ciencias Físico-Matemáticas , Universidad Autónoma de Coahuila, Edificio A, Unidad Camporredondo, 25000, Saltillo Coahuila México 
Publication year
2022
Publication date
Sep 2022
Publisher
Oxford University Press
e-ISSN
20503911
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
3171492846
Copyright
© The Author(s) 2022. Published by Oxford University Press on behalf of the Physical Society of Japan. This work is published under https://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.