Tensor gauge boson dark matter extension of the electroweak sector

Abstract The existence of dark matter is explained by a new, massive, neutral, non-symmetric, rank-2 tensor gauge boson ( $$\hbox {Z}_{{\upmu \upnu }}$$ Z μ ν -boson). The $$\hbox {Z}_{{\upmu \upnu }}$$ Z μ ν -boson can be predicted by the tensor gauge boson extension of the Electro Weak (EW) theory...

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Main Author: Elias Koorambas
Format: Article
Language:English
Published: SpringerOpen 2023-07-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-023-11791-6
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author Elias Koorambas
author_facet Elias Koorambas
author_sort Elias Koorambas
collection DOAJ
description Abstract The existence of dark matter is explained by a new, massive, neutral, non-symmetric, rank-2 tensor gauge boson ( $$\hbox {Z}_{{\upmu \upnu }}$$ Z μ ν -boson). The $$\hbox {Z}_{{\upmu \upnu }}$$ Z μ ν -boson can be predicted by the tensor gauge boson extension of the Electro Weak (EW) theory, proposed by Savvidy (Phys Lett B 625:341, 2005). The non-symmetric rank-2 tensor $$\hbox {Z}_{{\upmu \upnu }}$$ Z μ ν can be decomposed into a symmetric ( $$\hbox {Z}_{{(\upmu \upnu )}})$$ Z ( μ ν ) ) and anti-symmetric ( $$\hbox {Z}_{{[\upmu \upnu ]}})$$ Z [ μ ν ] ) part. Based on the non-Lagrangian formulation for the free sector of the $$\hbox {R}_{\textrm{2}}$$ R 2 -theory proposed recently by Criado et al. (Phys Rev D 102:125031, arXiv:2010.02224 , 2020), our massive anti-symmetric tensor field $$\hbox {Z}_{{[\upmu \upnu ]}}$$ Z [ μ ν ] corresponds to the massive symmetric spinor field $$\hbox {Z}_{{\upalpha \upbeta \upgamma \updelta }}$$ Z α β γ δ in the (2,0) irrep. For the massive $$\hbox {Z}_{{\upalpha \upbeta \upgamma \updelta }}$$ Z α β γ δ with the $$\hbox {Z}_{\textrm{2}}$$ Z 2 -symmetric Higgs portal couplings to a Standard Model (SM) particle, we compute the self-annihilation cross-section of the $$\hbox {Z}_{{\upalpha \upbeta \upgamma \updelta }}$$ Z α β γ δ dark matter and calculate its relic abundance. We also study the SM-SM particle scattering due to the exchange of the massive- $$\hbox {Z}_{{(\upmu \upnu )}}$$ Z ( μ ν ) symmetric field at a high energy scale. This proposition may have far reaching applications in astrophysics and cosmology.
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spelling doaj.art-493c315044714a31828267b0032b285c2023-09-10T11:22:35ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522023-07-018371910.1140/epjc/s10052-023-11791-6Tensor gauge boson dark matter extension of the electroweak sectorElias Koorambas0Computational Applications, Group, Division of Applied Technologies, National Center for Science and Research ‘Demokritos’Abstract The existence of dark matter is explained by a new, massive, neutral, non-symmetric, rank-2 tensor gauge boson ( $$\hbox {Z}_{{\upmu \upnu }}$$ Z μ ν -boson). The $$\hbox {Z}_{{\upmu \upnu }}$$ Z μ ν -boson can be predicted by the tensor gauge boson extension of the Electro Weak (EW) theory, proposed by Savvidy (Phys Lett B 625:341, 2005). The non-symmetric rank-2 tensor $$\hbox {Z}_{{\upmu \upnu }}$$ Z μ ν can be decomposed into a symmetric ( $$\hbox {Z}_{{(\upmu \upnu )}})$$ Z ( μ ν ) ) and anti-symmetric ( $$\hbox {Z}_{{[\upmu \upnu ]}})$$ Z [ μ ν ] ) part. Based on the non-Lagrangian formulation for the free sector of the $$\hbox {R}_{\textrm{2}}$$ R 2 -theory proposed recently by Criado et al. (Phys Rev D 102:125031, arXiv:2010.02224 , 2020), our massive anti-symmetric tensor field $$\hbox {Z}_{{[\upmu \upnu ]}}$$ Z [ μ ν ] corresponds to the massive symmetric spinor field $$\hbox {Z}_{{\upalpha \upbeta \upgamma \updelta }}$$ Z α β γ δ in the (2,0) irrep. For the massive $$\hbox {Z}_{{\upalpha \upbeta \upgamma \updelta }}$$ Z α β γ δ with the $$\hbox {Z}_{\textrm{2}}$$ Z 2 -symmetric Higgs portal couplings to a Standard Model (SM) particle, we compute the self-annihilation cross-section of the $$\hbox {Z}_{{\upalpha \upbeta \upgamma \updelta }}$$ Z α β γ δ dark matter and calculate its relic abundance. We also study the SM-SM particle scattering due to the exchange of the massive- $$\hbox {Z}_{{(\upmu \upnu )}}$$ Z ( μ ν ) symmetric field at a high energy scale. This proposition may have far reaching applications in astrophysics and cosmology.https://doi.org/10.1140/epjc/s10052-023-11791-6
spellingShingle Elias Koorambas
Tensor gauge boson dark matter extension of the electroweak sector
European Physical Journal C: Particles and Fields
title Tensor gauge boson dark matter extension of the electroweak sector
title_full Tensor gauge boson dark matter extension of the electroweak sector
title_fullStr Tensor gauge boson dark matter extension of the electroweak sector
title_full_unstemmed Tensor gauge boson dark matter extension of the electroweak sector
title_short Tensor gauge boson dark matter extension of the electroweak sector
title_sort tensor gauge boson dark matter extension of the electroweak sector
url https://doi.org/10.1140/epjc/s10052-023-11791-6
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