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Collider and dark matter searches in the inert doublet model from Peccei-Quinn symmetry

  • Alexandre Alves
  • Daniel A. Camargo
  • Alex G. Dias
  • Robinson Longas
  • Celso C. Nishi
  • Farinaldo S. QueirozEmail author
Open Access
Regular Article - Theoretical Physics

Abstract

Weakly Interacting Massive Particles (WIMPs) and axions are arguably the most compelling dark matter candidates in the literature. Could they coexist as dark matter particles? More importantly, can they be incorporated in a well motivated framework in agreement with experimental data? In this work, we show that this two component dark matter can be realized in the Inert Doublet Model in an elegant and natural manner by virtue of the spontaneous breaking of a Peccei-Quinn U(1) P Q symmetry into a residual \( {\mathbb{Z}}_2 \) symmetry. The WIMP stability is guaranteed by the \( {\mathbb{Z}}_2 \) symmetry and a new dark matter component, the axion, arises. There are two interesting outcomes: (i) vector-like quarks needed to implement the Peccei-Quinn symmetry in the model may act as a portal between the dark sector and the SM fields with a supersymmetry-type phenomenology at colliders; (ii) two-component Inert Doublet Model re-opens the phenomenologically interesting 100-500 GeV mass region. We show that the model can successfully realize a two component dark matter framework and at the same time avoid low and high energy physics constraints such as monojet and dijet plus missing energy, as well as indirect and direct dark matter detection bounds.

Keywords

Beyond Standard Model Cosmology of Theories beyond the SM Discrete Symmetries 

Notes

Open Access

This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.

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© The Author(s) 2016

Open AccessThis article is distributed under the terms of the Creative Commons Attribution 4.0 International License (https://creativecommons.org/licenses/by/4.0), which permits use, duplication, adaptation, distribution, and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.

Authors and Affiliations

  • Alexandre Alves
    • 1
  • Daniel A. Camargo
    • 2
  • Alex G. Dias
    • 2
  • Robinson Longas
    • 3
  • Celso C. Nishi
    • 4
  • Farinaldo S. Queiroz
    • 5
    Email author
  1. 1.Departamento de Ciências Exatas e da TerraUniversidade Federal de São PauloDiademaBrasil
  2. 2.Universidade Federal do ABC, Centro de Ciências Naturais e HumanasSanto AndréBrasil
  3. 3.Instituto de FísicaUniversidad de AntioquiaMedellínColombia
  4. 4.Universidade Federal do ABC, Centro de Matemática, Computação e Cognição NaturaisSanto AndréBrasil
  5. 5.Max-Planck-Institut fur KernphysikHeidelbergGermany

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