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A multi-component SIMP model with $U(1)_X \rightarrow Z_2 \times Z_3$

Multi-component dark matter scenarios are studied in the model with U(1)$_{X}$ dark gauge symmetry that is broken into its product subgroup Z$_{2}$ × Z$_{3}$ á la Krauss-Wilczek mechanism. In this setup, there exist two types of dark matter fields, X and Y, distinguished by different Z$_{2}$ × Z$_{3...

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Autores principales: Choi, Soo-Min, Kim, Jinsu, Ko, Pyungwon, Li, Jinmian
Lenguaje:eng
Publicado: 2021
Materias:
Acceso en línea:https://dx.doi.org/10.1007/JHEP09(2021)028
http://cds.cern.ch/record/2754275
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author Choi, Soo-Min
Kim, Jinsu
Ko, Pyungwon
Li, Jinmian
author_facet Choi, Soo-Min
Kim, Jinsu
Ko, Pyungwon
Li, Jinmian
author_sort Choi, Soo-Min
collection CERN
description Multi-component dark matter scenarios are studied in the model with U(1)$_{X}$ dark gauge symmetry that is broken into its product subgroup Z$_{2}$ × Z$_{3}$ á la Krauss-Wilczek mechanism. In this setup, there exist two types of dark matter fields, X and Y, distinguished by different Z$_{2}$ × Z$_{3}$ charges. The real and imaginary parts of the Z$_{2}$-charged field, X$_{R}$ and X$_{I}$, get different masses from the U(1)$_{X}$ symmetry breaking. The field Y, which is another dark matter candidate due to the unbroken Z$_{3}$ symmetry, belongs to the Strongly Interacting Massive Particle (SIMP)-type dark matter. Both X$_{I}$ and X$_{R}$ may contribute to Y’s 3 → 2 annihilation processes, opening a new class of SIMP models with a local dark gauge symmetry. Depending on the mass difference between X$_{I}$ and X$_{R}$, we have either two-component or three-component dark matter scenarios. In particular two- or three-component SIMP scenarios can be realised not only for small mass difference between X and Y, but also for large mass hierarchy between them, which is a new and unique feature of the present model. We consider both theoretical and experimental constraints, and present four case studies of the multi-component dark matter scenarios.
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spelling cern-27542752023-10-04T07:38:39Zdoi:10.1007/JHEP09(2021)028http://cds.cern.ch/record/2754275engChoi, Soo-MinKim, JinsuKo, PyungwonLi, JinmianA multi-component SIMP model with $U(1)_X \rightarrow Z_2 \times Z_3$astro-ph.COAstrophysics and Astronomyhep-phParticle Physics - PhenomenologyMulti-component dark matter scenarios are studied in the model with U(1)$_{X}$ dark gauge symmetry that is broken into its product subgroup Z$_{2}$ × Z$_{3}$ á la Krauss-Wilczek mechanism. In this setup, there exist two types of dark matter fields, X and Y, distinguished by different Z$_{2}$ × Z$_{3}$ charges. The real and imaginary parts of the Z$_{2}$-charged field, X$_{R}$ and X$_{I}$, get different masses from the U(1)$_{X}$ symmetry breaking. The field Y, which is another dark matter candidate due to the unbroken Z$_{3}$ symmetry, belongs to the Strongly Interacting Massive Particle (SIMP)-type dark matter. Both X$_{I}$ and X$_{R}$ may contribute to Y’s 3 → 2 annihilation processes, opening a new class of SIMP models with a local dark gauge symmetry. Depending on the mass difference between X$_{I}$ and X$_{R}$, we have either two-component or three-component dark matter scenarios. In particular two- or three-component SIMP scenarios can be realised not only for small mass difference between X and Y, but also for large mass hierarchy between them, which is a new and unique feature of the present model. We consider both theoretical and experimental constraints, and present four case studies of the multi-component dark matter scenarios.Multi-component dark matter scenarios are studied in the model with $U(1)_X$ dark gauge symmetry that is broken into its product subgroup $Z_2 \times Z_3$á la Krauss-Wilczek mechanism. In this setup, there exist two types of dark matter fields, $X$ and $Y$, distinguished by different $Z_2 \times Z_3$ charges. The real and imaginary parts of the $Z_2$-charged field, $X_R$ and $X_I$, get different masses from the $U(1)_X$ symmetry breaking. The field $Y$, which is another dark matter candidate due to the unbroken $Z_3$ symmetry, belongs to the Strongly Interacting Massive Particle (SIMP)-type dark matter. Both $X_I$ and $X_R$ may contribute to $Y$'s $3\rightarrow 2$ annihilation processes, opening a new class of SIMP models with a local dark gauge symmetry. Depending on the mass difference between $X_I$ and $X_R$, we have either two-component or three-component dark matter scenarios. In particular two- or three-component SIMP scenarios can be realised not only for small mass difference between $X$ and $Y$, but also for large mass hierarchy between them, which is a new and unique feature of the present model. We consider both theoretical and experimental constraints, and present four case studies of the multi-component dark matter scenarios.arXiv:2103.05956TUM-HEP-1319/21CERN-TH-2021-030KIAS-P21008oai:cds.cern.ch:27542752021-03-10
spellingShingle astro-ph.CO
Astrophysics and Astronomy
hep-ph
Particle Physics - Phenomenology
Choi, Soo-Min
Kim, Jinsu
Ko, Pyungwon
Li, Jinmian
A multi-component SIMP model with $U(1)_X \rightarrow Z_2 \times Z_3$
title A multi-component SIMP model with $U(1)_X \rightarrow Z_2 \times Z_3$
title_full A multi-component SIMP model with $U(1)_X \rightarrow Z_2 \times Z_3$
title_fullStr A multi-component SIMP model with $U(1)_X \rightarrow Z_2 \times Z_3$
title_full_unstemmed A multi-component SIMP model with $U(1)_X \rightarrow Z_2 \times Z_3$
title_short A multi-component SIMP model with $U(1)_X \rightarrow Z_2 \times Z_3$
title_sort multi-component simp model with $u(1)_x \rightarrow z_2 \times z_3$
topic astro-ph.CO
Astrophysics and Astronomy
hep-ph
Particle Physics - Phenomenology
url https://dx.doi.org/10.1007/JHEP09(2021)028
http://cds.cern.ch/record/2754275
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