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arXiv · 1508.01049

Cosmological and Particle Physics Constraints on a New Non-Abelian SU(3) Gauge Model for Ordinary/Dark Matter Interaction

O. Oliveira·C. A. Bertulani·M. S. Hussein·W. de Paula·T. Frederico
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Abstract

We propose a mirror model for ordinary and dark matter that assumes a new SU(3) gauge group of transformations, as a natural extension of the Standard Model (SM). A close study of big bang nucleosynthesis, baryon asymmetries, cosmic microwave background bounds, galaxy dynamics, together with the Standard Model assumptions, help us to set a limit on the mass and width of the new gauge boson. The cross section for the elastic scattering of a dark proton by an ordinary proton is estimated and compare to the WIMP--nucleon experimental upper bounds. It is observed that all experimental bounds for the various cross sections can be accommodated consistently within the gauge model. We also suggest a way for direct detection of the new gauge boson via one example of a SM forbidden process: $e^+ + p \rightarrow μ^+ + X$, where $X = Λ$ or $Λ_c$.

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O. Oliveira, C. A. Bertulani, M. S. Hussein, W. de Paula, T. Frederico. 2015-08-05. Cosmological and Particle Physics Constraints on a New Non-Abelian SU(3) Gauge Model for Ordinary/Dark Matter Interaction. https://doi.org/10.1007/s13538-016-0447-y

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